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Transcript
Conservation of Spiders (Araneae) in the Western
Australian Rangelands, with Particular
Reference to Disturbance by Fire
Peter R Langlands (B.Sc. Hons)
This thesis is presented for the degree of Doctor of Philosophy
of the University of Western Australia
School of Animal Biology
November 2010
Cover picture: A female Hoggicosa bicolor (Hogg, 1905)
SUMMARY
Fire is a common disturbance in many ecosystems and an integral part of arid Australia.
However, there are many gaps in the current knowledge of how the fauna and flora of
the arid zone respond to fire. This is particularly true for invertebrates, including
spiders, where there are several obstacles to successful biodiversity conservation.
Besides lack of knowledge of the response of spiders to fire, there is also a considerable
taxonomic impediment. That is, a majority of species are described long ago or not at
all. I set out to improve our knowledge for the conservation of spiders in arid Australia
by removing part of this taxonomic impediment and examining the long-term response
of spiders to fire.
To help remove the taxonomic impediment and facilitate my investigations of the postfire response of spiders, I revise the taxonomy and systematics of a genus of wolf
spiders. The Australian wolf spider genus Hoggicosa Roewer, 1960 with the type
species Hoggicosa errans (Hogg, 1905), is revised to include ten species. Hoggicosa is
comprised of burrowing lycosids, several constructing doors from sand or debris, and
are predominantly found in semi-arid to arid regions of Australia. Of nine previously
described species, three are synonymised with Hoggicosa castanea (Hogg, 1905) comb.
nov., and four new species are described. A phylogenetic analysis including nine
Hoggicosa species, 11 lycosine species from Australia and four from overseas, with
Arctosa cinerea Fabricius, 1777 as outgroup, supported the monophyly of Hoggicosa.
Proposed synapomorphies for Hoggicosa are a larger distance between the epigynum
anterior pockets compared to the width of the posterior transverse part in females, and a
large number of specialised setae on the tip of the cymbium in males. The analysis
found that an unusual sexual dimorphism for wolf spiders (females more colourful than
males), evident in four species of Hoggicosa, has evolved multiple times.
To examine the post-fire changes in assemblages of spiders I established a
chronosequence study in spinifex habitat of central Western Australia. Ground-active
spiders were pitfall-trapped over nine months in 27 sites representing experimental fires
(0 and 0.5 years) and wildfires (3, 5, 8 and 20 years post-fire). Three questions were
examined: 1) Is there a successional pattern following disturbance by fire? 2) If so, what
best explains this post-fire successional pattern? and 3) To what extent can the post-fire
response of spiders be predicted?
i
I examine the first question by assessing if the spider assemblage displays a
successional pattern, and if this is deterministic (i.e. if the assemblage converges to a
long unburnt state). There were significant non-linear changes in species richness and
evenness, along with marked changes in composition of spiders with increasing postfire age. For all three measures, the assemblage appears highly deterministic,
converging towards the long unburnt state. Similarity in richness, evenness and species
composition to the 20-year-old sites all increased with increasing time since fire (3 to 8
years). However, experimentally burnt sites did not fit this sequence neatly. Two
alternative hypotheses are proposed to explain this second trajectory: inertia within the
system, or the rapid migration and recolonization from nearby surrounding unburnt
areas.
A vast array of variables can act singly or in combination to influence an area‟s biota. In
arid Australia, fire and rainfall are two key and potentially interacting forces that
contribute in shaping assemblages of plants and animals. However, the degree to which
spatial processes, environmental variables and biotic processes combine with fire and
rainfall to shape assemblages of animals remains poorly quantified. As such, I assessed
and quantified which variables can best explain the observed post-fire patterns in
species richness and composition of spiders. Along with post-fire age, I examined the
short-term effect of rainfall, the influence of space, environmental variables (soil,
floristics, habitat structure) and biotic processes (predation by scorpions, small
insectivorous mammals and reptiles). Predictor variables explained 79% of the variation
in species richness and 32% in composition of spiders using distance-based redundancy
analysis. Variation partitioning identified post-fire age as explaining the largest
proportion of this variation, 61% for species richness and 78% for composition.
However, spatially and non-spatially structured vegetation variables (floristics and
habitat structure) explained much of this variation. Rainfall explained a large proportion
of the explained variation for species richness (59%), but not species composition
(30%). There was little variation attributable to predation (0 and 14% for species
richness and composition, respectively) or pure spatial structure (5 and 5%).
Developing a predictive understanding of how species assemblages respond to fire is a
key conservation goal. In moving from solely describing patterns following fire to
predicting changes, plant ecologists have successfully elucidated generalisations based
ii
on functional traits. Using species-traits might also allow better predictions for fauna
but there are few empirical tests of this approach. To examine the third question I tested
whether species-traits changed with post-fire age for spiders. I made a priori predictions
as to whether spiders with ten traits associated with survival, dispersal, reproduction,
resource-utilization and microhabitat occupation would increase or decrease with postfire age. I then tested these predictions using a direct (fourth-corner on individual traits
and composite traits) and an indirect approach (emergent groups), comparing the
benefits of each and also examining the degree to which traits were inter-correlated. For
the seven individual traits that were significant in the fourth-corner analysis, three
followed predictions (body size, abundance of burrow ambushers and burrowers were
greater in recently burnt sites); two were opposite (heavy sclerotisation of
cephalothorax and time to maturity were in greater abundance in long unburnt and
recently burnt sites respectively); and two displayed response patterns more complex
than predicted (abdominal scutes displayed a U-shaped response and dispersal ability a
hump shaped curve). However, within a given trait, there were few significant results
among post-fire ages. Several traits were inter-correlated and scores based on composite
traits used in a fourth-corner analysis found significant patterns, but slightly different to
those using individual traits. Changes in abundance with post-fire age were significant
for three of the five emergent groups. The fourth-corner analysis yielded more detailed
results, but overall the two approaches are considered complementary.
These studies make a substantial contribution of new knowledge to assist with the
conservation of spiders in the arid zone of Australia. I have removed the taxonomic
impediment for a charismatic and common genus of wolf spiders. In addition, I have
examined in detail the post-fire response of an assemblage of spiders in spinifex habitat.
The high degree of determinism in this assemblage and the strong correlation between
post-fire changes in the vegetation and spiders is promising for land managers. It
suggests that managers can directly influence the conservation of the spider fauna by
actively managing fire effects on habitat structure and floristics. The development of a
traits-based approach, which may contribute to predicting post-fire responses of spiders
in other habitats, was only moderately successful. However, the development of such a
mechanistic approach is novel and deserves further attention.
iii
CONTENTS
SUMMARY ....................................................................................................................... i
CONTENTS ..................................................................................................................... iv
ACKNOWLEDGEMENTS ............................................................................................. vi
STRUCTURE OF THESIS ............................................................................................viii
SECTION I: TAXONOMY AND SYSTEMATICS
General Introduction ..................................................................................................... 1
CHAPTER 1: Systematic revision of Hoggicosa Roewer, 1960, the Australian
„bicolor’ group of wolf spiders (Araneae: Lycosidae) .............................................. 5
Abstract ................................................................................................................. 6
Introduction ........................................................................................................... 7
Materials and Methods .......................................................................................... 9
Results ................................................................................................................. 12
Discussion ........................................................................................................... 14
Systematics ......................................................................................................... 17
References ........................................................................................................... 52
Appendix 1 .......................................................................................................... 83
Appendix 2 .......................................................................................................... 85
Appendix 3 .......................................................................................................... 88
Summary of Section I ................................................................................................ 100
SECTION II: ECOLOGY
General Introduction ................................................................................................. 102
CHAPTER 2: Is the successional trajectory of an arid spider assemblage following
fire deterministic? .................................................................................................. 109
Abstract ............................................................................................................. 110
Introduction ....................................................................................................... 111
Methods............................................................................................................. 113
Results ............................................................................................................... 117
Discussion ......................................................................................................... 119
References ......................................................................................................... 124
Appendix A ....................................................................................................... 137
Appendix B ....................................................................................................... 148
Appendix C ....................................................................................................... 139
Appendix D ....................................................................................................... 148
iv
CHAPTER 3: Untangling the drivers of structure in animal assemblages in arid
ecosystems: the influence of fire, rainfall, vegetation, predators and spatial
structure on spiders (Araneae) ............................................................................... 151
Abstract ............................................................................................................. 152
Introduction ....................................................................................................... 153
Materials and methods ...................................................................................... 156
Results ............................................................................................................... 160
Discussion ......................................................................................................... 163
References ......................................................................................................... 168
Appendix A ....................................................................................................... 183
Appendix B ....................................................................................................... 184
Appendix C ....................................................................................................... 185
Appendix D ....................................................................................................... 186
CHAPTER 4: Predicting the post-fire responses of animal assemblages: testing a
trait-based approach using spiders ......................................................................... 187
Summary ........................................................................................................... 188
Introduction ....................................................................................................... 189
Materials and Methods ...................................................................................... 192
Results ............................................................................................................... 197
Discussion ......................................................................................................... 199
Literature cited .................................................................................................. 205
Appendix S1...................................................................................................... 216
Appendix S2...................................................................................................... 218
Appendix S3...................................................................................................... 234
Appendix S4...................................................................................................... 235
Synthesis of Ecological Results and Future Research .............................................. 238
CONCLUSION ............................................................................................................. 243
v
ACKNOWLEDGEMENTS
Looking over the past years and back to when I started, I feel that I have changed and
grown enormously, not just academically, but as a person. Each of my supervisors has
contributed to these changes in their own way. I especially thank Bob Black, Barbara
York Main, Volker Framenau and Karl Brennan for all they have taught me, and all the
time they have spent with me over the years! Particularly, to Bob for his keen eye for
detail, to Barbara for her words of encouragement and to Volker for his patience in
teaching me taxonomy and systematics.
Special thanks to my supervisor and mentor Karl Brennan for his support. Our
conversations were so often engaging and stimulating and Karl never failed to suggest
solutions when problems arose. Thanks also to his family (Melinda Moir and Bridgette)
for their welcoming hospitality during my visits. I doubt I would have reached the end if
not for the trips to Kalgoorlie to write.
I thank Mark Harvey for providing me with workspace at the Western Australian
Museum, along with all those who made my time there an enjoyable one: Julianne
Waldock, Jung-Sun Yoo, Karen Edward, Ricardo Ott, Bill Humphreys, Mike Rix, Brian
Hanich and Terry Houston. I thank also the many arachnologists who assessed my
species identifications: Julianne Waldock, Volker Framenau and Ricardo Ott from the
Western Australian Museum; Barbara Baehr and Robert Raven from the Queensland
Museum and Barbara York Main from the University of Western Australia.
The Western Australian Department of Environment and Conservation provided vital
financial support, while staff past and present were invaluable. I thank the following:
Bruce Ward and Graeme „tubs‟ Liddlelow for their desert knowledge and support in the
field; Neil Burrows, Ian Kealley and Neville Hague for their support of the project; Ray
Cranfield for his identification of plants and field assistance as well as Mark Cowan for
identification of the vertebrate by-catch and stimulating discussions in the field. Graeme
Behn and Li Shu provided GIS assistance that was crucial in determining fire histories.
Brad Durrant and Nadine Guthrie generously loaned the pitfall traps.
I thank the staff of the Department of Environment and Conservation Kalgoorlie office
for their assistance in conducting experimental burns, with field trips and temporary
vi
office space: particularly Ryan Butler, Ian Kealley, Garry Hearle, Anthony Richardson,
Brad Barton, Julie Waters, Steve Toole and Luke Puertoliano.
To office companions and students past and present I extend thanks for all the company
and coffee breaks: particularly Scott Carver, Sharron Perks, Karen Edward, Mike Rix,
Janine Wojcieszek, Rachel Binks, Blair Parsons, Jen Francis, Aimee Silla, Andrew
Williams, Sean Tomlinson, Sean Stankowski, Mike Young, Danilo Harms and Bruno
Buzatto. I am grateful also to the many staff within the Animal Biology department who
have helped over the years: Kerry Knott, Natalie Byrne, Rob Hurn, Tom Stewart, Dale
Roberts, Helen Spafford and Graeme Martin. I also thank Mike Johnson and Jane
Prince for being on my review panel.
I am indepted to all the people who provided field assistance: Karen Debski, Amanda
McGinty, Fernanda Ferreira, Christopher Taylor, Eliane „Lica‟ Assis and Filomeno
„Phil‟ Cruz. I appreciated the great company and interesting discussions in the field of
Tom Bragg and Barbi Hayes.
I thank the attendees of Conservation Volunteers Australia for their assistance with the
backbreaking work of creating firebreaks on the October 2005 trip (Louise Robertson,
Alison Sparey, Graham Plowright, Marie-lina Muller, Andrea Schuster, Karen Lang,
Min Kim and Russell Gorton).
Additional satellite imagery was generously donated by Peter Sanders and Adrian Allen
at Satellite Remote Sensing Services, Department of Land Information. Rainfall data
was also provided free of charge by the Bureau of Meteorology, Perth, Western
Australia.
My Ph.D. research was funded by an Australian Postgraduate Award, with additional
funding provided by the School of Animal Biology at the University of Western
Australia, and the Department of Environment and Conservation. The Australian
Biological Resources Study (ABRS) provided a conference travel grant.
Finally, I thank my family (Bob, Natasha, Larissa, Andrew and Loretta plus
Christopher) for their unwavering financial, physical and emotional support over the
years and Jane for reviving my chirp!
vii
STRUCTURE OF THESIS
There are two sections to my thesis: a taxonomic/systematic section and an ecological
section. The primary focus of my work was ecological, but I undertook the taxonomic
study to alleviate problems with identifications and to allow the use of the species I
described in a detailed population study following fire. Therefore, my supervisors and I
envisioned that the two sections would connect neatly, with one or more of the species
described in the taxonomic component utilised in the ecological work. In addition, I
anticipated that acquiring skills in taxonomy would prove indispensable in my future
scientific career. Ultimately, the abundance and density of Hoggicosa wolf spiders was
too low for conducting a population study, despite many weeks searching throughout
the proposed Lorna Glen Conservation Park. Thus, although the direct connection
between the two sections did not eventuate, the broader and underlying importance of
taxonomic work for the conservation of spiders is self-evident. Ecological research
conducted at the community level requires a sound taxonomic and systematic
knowledge of the component species. I therefore consider both sections of this thesis
contribute substantially to the broad aim of improving knowledge to conserve spiders in
the arid zone of Australia.
This thesis is prepared as a series of papers for publication, with each chapter
representing a separate paper. For each paper, I have indicated the intended journal and
publication status, along with contributions from co-authors. As each journal has
slightly different formatting requirements, minor differences in formatting between
chapters will be noticeable, along with some repetition in the method parts. However,
the advantage of this approach is that I have honed my skills in preparing papers for
publication, the currency of modern science, and this format will aid the rapid
dissemination of my work.
viii
Publications arising from this thesis
Chapter 1
Langlands, P. R., and V. W. Framenau. 2010. Systematic revision of Hoggicosa
Roewer, 1960, the Australian 'bicolor' group of wolf spiders (Araneae:
Lycosidae). Zoological Journal of the Linnean Society 158:83-123
See enclosed CD for pdf
Chapter 2
Langlands, P. R., K. E. C. Brennan, and B. Ward. Is the successional trajectory of an
arid spider assemblage following fire deterministic? Accepted for Austral
Ecology pending minor revisions
Chapter 3
Langlands, P. R., K. E. C. Brennan, and B. Ward. Untangling the drivers of animal
assemblages in arid ecosystems: the influence of fire, rainfall, vegetation, higher
predators and spatial structure on spiders (Araneae). In preparation for
Ecography
Chapter 4
Langlands, P. R., K. E. C. Brennan, V. W. Framenau, and B. Y. Main. Predicting the
post-fire responses of animal assemblages: testing a trait-based approach using
spiders. Accepted for the Journal of Animal Ecology
ix
Declaration of contributions
For each manuscript, I was the main contributor and responsible for the experimental
design, data collection, analysis and interpretation of results and writing. Three of my
supervisors are co-authors (VW Framenau, KEC Brennan and BY Main) along with a
colleague from the Department of Environment and Conservation (B Ward). My coauthors contributed to the experimental design, interpretation of results and writing.
Author contributions to each manuscript:
Chapter 1: PRL = 85%, VWF = 15%
Chapter 2: PRL = 90%, KECB + BW = 10%
Chapter 3: PRL = 90%, KECB + BW = 10%
Chapter 4: PRL = 90%, KECB + VWF + BYM = 10%.
Each author has given permission for all work to be included in this thesis.
Signatures:
_____________________________
Peter R Langlands
(candidate)
_____________________________
Adj. Prof Bob Black
(co-ordinating supervisor)
x
SECTION I: TAXONOMY
AND SYSTEMATICS
SECTION I: TAXONOMY AND SYSTEMATICS
General Introduction
Australia has an extremely rich and diverse fauna of spiders with 78 families and
approximately 3300 currently described species (Raven et al. 2002, Yeates et al. 2003,
Chapman 2009). However, this represents only a fraction of the spider fauna, with the
vast majority, estimated at 67%, awaiting formal description (Chapman 2009). Wolf
spiders (Lycosidae) typify this scenario. Only 168 species of an estimated 400+ species
have been described (V. W. Framenau pers. comm.). This lack of taxonomic knowledge
is a major problem for ecologists wishing to study spiders, as sound taxonomy and
species descriptions form the basis of ecology and conservation (Wilson 1971, Kim
1993, Kim and Byrne 2006). This problem, often termed the taxonomic impediment
(New 1984, Wheeler et al. 2004, Evenhuis 2007), arises through two mechanisms, lack
of species descriptions (or species descriptions that are old or inaccessible) and lack of
taxonomic expertise (Kitching 1993, Brennan et al. 2004). Others however, have argued
that the use of parataxonomists and the identification of morphospecies, recognizable
taxonomic units or functional groups can address taxonomic impediments (Oliver and
Beattie 1993, 1996 a, b, Pik 1999), but this has also been hotly debated (Brower 1995,
Goldstein 1997, Oliver and Beattie 1997, Goldstein 1999, Beattie and Oliver 1999). The
stance I have taken is to sort to species level for all spider families and have these
identifications confirmed by taxonomic experts (See Acknowledgments). When no
scientific names could be found or recent taxonomic references were lacking, for
example the family Gnaphosidae, I assigned numerical codes for species. To reduce the
risk of over-splitting species I chose to exclude females and juveniles and identify
males only (Derraik et al. 2002). I set out to help remove this impediment for a common
genus of wolf spiders and in the process gain skills to allow me to identify spiders more
confidently to species level for my ecological work, where not surprisingly most species
(82%) were undescribed.
Wolf spiders were an ideal choice, as they are ubiquitous and abundant across all
habitats in Australia (Main 1976). The family has also received recent attention in
Australia, which provided a broad subfamily and generic framework (Framenau and
Vink 2001, Framenau 2002, Framenau 2006 a, b, c, Framenau and Yoo 2006, Murphy
et al. 2006, Framenau and Baehr 2007). Using this information, I selected a group, the
„bicolor group‟, which was thought to represent a distinct genus (McKay 1973, 1975,
1
Murphy et al. 2006). The „bicolor group‟ was also suitable as it contained a limited
number of species that was manageable in scope. Additionally, they are large, robust
spiders that are easy to handle and are common throughout the arid zone of Australia.
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Conservation Biology, 13, 1514-1514.
Brennan, K. E. C., Moir, M. L. & Majer, J. D. (2004) Exhaustive sampling in a
Southern Hemisphere global biodiversity hotspot: inventorying species richness
and assessing endemicity of the little known jarrah forest spiders. Pacific
Conservation Biology, 10, 241-260.
Brower, A. V. Z. (1995) Taxonomic minimalism. Trends in Ecology & Evolution, 10,
203-203.
Chapman, A. D. (2009) Numbers of Living Species in Australia and the World, 2nd
edition, Australian Biological Resources Study, Canberra, Australia.
Derraik, J. G. B., Closs, G. P., Dickinson, K. J. M., Sirvid, P., Barratt, B. I. P. &
Patrick, B. H. (2002) Arthropod morphospecies versus taxonomic species: a
case study with Araneae, Coleoptera and Lepidoptera. Conservation Biology,
16, 1015-1023.
Evenhuis, N.L. (2007) Helping solve the “other” taxonomic impediment: completing
the Eight Steps to Total Enlightenment and Taxonomic Nirvana. Zootaxa, 1407,
3-12.
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Lycosidae). Invertebrate Systematics, 16, 209-235.
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(Araneae: Lycosidae). Zootaxa, 1281, 55-67.
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(Araneae, Lycosidae). Journal of Natural History, 40, 273-292.
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Roewer, 1960 (Araneae: Lycosidae). Zootaxa, 1304, 1-20.
Framenau, V. W. & Baehr, B. C. (2007) Revision of the Australian wolf spider genus
Dingosa Roewer, 1955 (Araneae, Lycosidae). Journal of Natural History, 41,
1603-1629.
Framenau, V. W. & Vink, C. J. (2001) Revision of the wolf spider genus Venatrix
Roewer (Araneae: Lycosidae). Invertebrate Systematics, 15, 927-970.
2
Framenau, V. W. & Yoo, J.-S. (2006) Systematics of the new Australian wolf spider
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3
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4
CHAPTER 1
Systematic revision of Hoggicosa Roewer, 1960, the
Australian ‘bicolor’ group of wolf spiders (Araneae:
Lycosidae)
Peter R Langlands
Volker W Framenau
Zoological Journal of the Linnean Society, 2010, 158, 83–123
5
ABSTRACT
The Australian wolf spider genus Hoggicosa Roewer, 1960 with the type species
Hoggicosa errans (Hogg, 1905) is revised to include ten species: Hoggicosa alfi sp.
nov.; Hoggicosa castanea (Hogg, 1905) comb. nov. (= Lycosa errans Hogg, 1905 syn.
nov.; = Lycosa perinflata Pulleine, 1922 syn. nov.; = Lycosa skeeti Pulleine, 1922 syn.
nov.); Hoggicosa bicolor (Hogg, 1905) comb. nov.; Hoggicosa brennani sp. nov.;
Hoggicosa duracki (McKay, 1975) comb. nov.; Hoggicosa forresti (McKay, 1973)
comb. nov.; Hoggicosa natashae sp. nov.; Hoggicosa snelli (McKay, 1975) comb.
nov.; Hoggicosa storri (McKay, 1973) comb. nov.; and Hoggicosa wolodymyri sp.
nov. The Namibian Hoggicosa exigua Roewer, 1960 is transferred to Hogna, Hogna
exigua (Roewer, 1960) comb. nov. A phylogenetic analysis including nine Hoggicosa
species, 11 lycosine species from Australia and four from overseas, with Arctosa
cinerea Fabricius, 1777 as outgroup, supported the monophyly of Hoggicosa, with a
larger distance between the epigynum anterior pockets compared to the width of the
posterior transverse part. The analysis found that an unusual sexual dimorphism for
wolf spiders (females more colourful than males), evident in four species of Hoggicosa,
has evolved multiple times. Hoggicosa are burrowing lycosids, several constructing
doors from sand or debris, and are predominantly found in semi-arid to arid regions of
Australia.
6
INTRODUCTION
Australia possesses a rich fauna of wolf spiders with 156 currently described species in
24 genera and four subfamilies: Artoriinae Framenau, 2007; Venoniinae Lehtinen &
Hippa, 1979; Zoicinae Lehtinen & Hippa, 1979; and Lycosinae Sundevall, 1833
(Framenau, 2007). The latter is the most diverse subfamily in Australia with 109
described species in 17 genera, although the current count represents possibly fewer
than half of the species present in collections (V. W. Framenau, unpubl. data). The
Lycosinae are defined by two synapomorphies of the tegular apophysis of the male
pedipalp, i.e. its transverse orientation, with ventrally directed spur and a sinuous
channel on its dorsal surface (Dondale, 1986). Knowledge of Australian Lycosinae is
poor, although there have been several recent generic revisions, including Dingosa
Roewer, 1955, Knoelle Framenau, 2006, Mainosa Framenau, 2006 and Tuberculosa
Framenau & Yoo, 2006 and Venatrix Roewer, 1960 (Framenau & Vink, 2001;
Framenau, 2006a, b; Framenau & Yoo, 2006; Framenau & Baehr, 2007). Molecular
studies have suggested two distinct clades of Australian Lycosinae; one has an oriental
origin (Venatrix and Tuberculosa) and the remaining genera represent a Gondwanan
clade with the closest relative in the taxon sampled, Pavocosa gallopavo (Mello-Leitão,
1941), from South America (see Murphy et al., 2006; Gotch et al., 2008).
Hoggicosa Roewer, 1960 clearly conforms to the subfamily diagnosis of the Lycosinae
(Dondale, 1986). The genus was initially proposed as nomen nudum by Roewer (1955).
Later it was formally described with the Australian Lycosa errans Hogg, 1905 as type
species (Roewer, 1960) along with a second species from Namibia, Hoggicosa exigua
Roewer, 1960. Roewer distinguished Hoggicosa by the shape of the labium (as long as
wide) in combination with the curvature of the anterior eye row (straight). The somatic
characters that Roewer (1959, 1960) used to diagnose many of his genera have since
been found to be of limited value for wolf spider classification compared with more
recently employed genitalic characters (see Vink, 2001; Stratton, 2005). Hoggicosa was
later considered a junior synonym of Arkalosula Roewer, 1960, which is itself a junior
synonym of Arctosa C. L. Koch, 1847 (Guy, 1966: 64). Guy‟s (1966) taxonomic
changes, however, were not accepted by later cataloguers (e.g. Brignoli, 1983; Platnick,
2009).
In a review of a well-defined Australian group of wolf spiders that he called the „bicolor
group‟ based on the striking colour combination of some females (see Fig. 1), McKay
7
(1973) transferred Hoggicosa errans back to Lycosa without providing a taxonomic
justification. However, McKay (1973) suggested close affinities of his „bicolor group‟
with Geolycosa Montgomery, 1904. Later McKay (1975) added two more species to the
„bicolor group‟ and described males, apparently less conspicuously coloured than
females, for the first time.
Sexual dimorphism in wolf spiders is evident in a multitude of forms, with most
differences between males and females being attributed to reproductive roles (sexual
selection). Females of ground dwelling spiders, including lycosids, are generally larger
than their male counterparts, explained by a fecundity advantage of larger females
(Prenter, Montgomery & Elwood, 1997; Prenter, Elwood & Montgomery, 1998, 1999).
Sexual dimorphism in wolf spiders also exists in relative size of chelicerae and venom
glands (Walker & Rypstra, 2001, 2002) and relative length of legs (Framenau, 2005).
Some dimorphic colour patterns augment body size and condition and have been argued
to play an important role in the mating behaviour of wolf spiders (Moya-Laraño, Taylor
& Fernandez-Montraveta, 2003). Male wolf spiders generally have more conspicuous
colour patterns than females, although the patterns are not pronounced in many species.
This may play an important role in mate choice by females; for example, fore leg
ornamentation of male lycosids was reviewed by Framenau & Hebets (2007). More
cryptic colours of females may also have evolved through natural selection; wolf spider
females exhibit prolonged brood care and cryptic colouration may protect the females
and their clutch from predators such as birds, reptiles, and predatory insects. Some
Hoggicosa species, however, show a remarkable reversed colour dimorphism. Females
of Hoggicosa bicolor (similarly coloured as penultimate males, Fig. 1A), Hoggicosa
storri (similarly coloured as penultimate males, Fig. 1D), Hoggicosa castanea, and
Hoggicosa forresti (McKay, 1973, fig. 1F) are much more colourful than their male
counterparts (Fig. 1B, E), but the evolution of these striking patterns has not been
studied.
This paper revises the taxonomy and systematics of Hoggicosa, which is here reestablished as a valid genus. We test the monophyly of this genus with a phylogenetic
analysis including 11 Australian representatives of the subfamily Lycosinae and
representatives of the northern hemisphere genera Lycosa and Geolycosa, with which
Hoggicosa was previously associated. This phylogenetic analysis also allowed us to test
8
the origin of the striking colour dimorphism of males and females, evident in four
species of Hoggicosa.
MATERIAL AND METHODS
This study is based on an examination of more than 20 000 records of wolf spiders in all
Australian museums as part of an extensive revision of the Australian Lycosidae.
Descriptions are based on spiders stored in 70% ethanol, which were studied under a
Leica MZ6 stereo microscope. For examination of female internal genitalia, epigynes
were placed in lactic acid overnight. Digital images were taken using a Leica DFC 500
digital camera attached to a Leica MZ16A stereo microscope. To increase depth of
field, multiple images were merged using the software program AutoMontage Pro
Version 5.02 (p). These images were then placed into Adobe Illustrator CS3 and
electronic drawings compiled by manually tracing over the structures in the image. For
clarity, setae without diagnostic value have been omitted from all drawings. Male
pedipalps mainly differ by details of the median apophysis and palea, but these details
are not discernable in retrolateral view; therefore, although generally illustrated in
taxonomic papers of Lycosidae, these views are omitted here. All measurements are in
mm.
Scanning electron micrographs (SEMs) were taken using a Philips XL30 ESEM at the
Centre for Microscopy and Microanalysis, University of Western Australia. In
preparation for SEMs, specimens were placed in 100% ethanol overnight. They were
then cleaned ultrasonically for 2 min and critically point dried. Specimens were then
mounted on stubs using carbon tabs and coated with 10–15 nm of gold.
Morphological nomenclature follows Framenau & Baehr (2007), but some terms are
introduced here for the first time. We identify three parts of the tegular apophysis: a
„ventral spur‟, an „apical point‟, and „ridge‟ joining these (see Fig. 5A). The pars
pendula is a membranous flap accompanying the embolus on its apical edge (in relation
to the pedipalp) (see Dondale & Redner, 1983), which often joins the palea basally. We
found a secondary structure basal to the terminal apophysis in all Hoggicosa, which we
call the „subterminal apophysis‟ (see Figs 7A–D, 13B). This structure was erroneously
labelled pars pendula in the recent description of the genus Knoelle (Framenau, 2006b,
fig. 8).
9
Abbreviations
Anatomy
AE, anterior eyes; ALE, anterior lateral eyes; AME, anterior median eyes; OL,
opisthosoma length; OW, opisthosoma width; PL, prosoma length; PW, prosoma width;
PE, posterior eyes; PLE, posterior lateral eyes; PME, posterior median eyes; TL, total
length.
Institutions
AM, Australian Museum, Sydney; ANIC, Australian National Insect Collection,
Canberra; NMV, Museum Victoria, Melbourne; NTMAG, Northern Territory Museum
and Art Gallery, Darwin; SAM, South Australian Museum, Adelaide; QM, Queensland
Museum, Brisbane; WAM, Western Australian Museum, Perth; Distribution; NSW,
New South Wales; NT, Northern Territory; Qld, Queensland; SA, South Australia; Vic,
Victoria; WA, Western Australia.
Phylogenetic Analysis
Taxa
A number of factors determined which taxa in addition to nine Hoggicosa species were
included in the analysis (Hoggicosa natashae sp. nov. was excluded as only females are
known).
1. We included most Australian genera that were part of a Gondwanan clade, to which
Hoggicosa belonged, in a molecular phylogeny of the Lycosidae (Murphy et al., 2006):
Hogna crispipes L. Koch, 1877, Lycosa godeffroyi L. Koch, 1865, Lycosa leuckartii
(Thorell, 1870), Knoelle clara (L. Koch, 1877), and the „Grey Wolf Spider‟ („New
Genus 6‟ in Murphy et al., 2006; see also Framenau & Baehr, 2007). This allowed
testing of the relationships found by Murphy et al. (2006) with our morphological
character set.
2. Based on morphological and behavioural characters, two putative Australian sister
genera were included in the analysis. Males of the monotypic genus Knoelle also
possess backwards bent macrosetae on the cymbium tip, but in a larger patch than
Hoggicosa (Framenau, 2006b). The undescribed „Grey Wolf Spider‟ has similar
somatic morphology and burrowing behaviour as Hoggicosa species.
3. Two Australian lycosine genera were recently reviewed, which allowed an
appropriate consideration within our phylogenetic analysis: Mainosa Framenau, 2006
and Dingosa Roewer, 1955 (Appendix 1).
10
4. We included the type species of the Australian lycosine genus Venator Hogg, 1900,
V. spenceri Hogg, 1900, and a putative conspecific with very similar somatic and
genitalic morphology, Hogna immansueta (Simon, 1909).
5. Species of Hoggicosa were previously associated with two genera, Lycosa
(Mediterranean; Zyuzin & Logunov, 2000) and Geolycosa (Holarctic; Wallace, 1942;
Zyuzin & Logunov, 2000) and we included representatives of both to test their
association with Hoggicosa. Male specimens of Lycosa tarantula (Linnaeus, 1758) and
Lycosa praegrandis (C. L. Koch, 1836) were unavailable for study, so male characters
were scored from secondary sources (Zyuzin & Logunov, 2000; Álvares, 2006).
The limits of the Lycosinae are unclear, and this subfamily may include the traditional
Pardosinae and Hippasinae (see Murphy et al., 2006). Therefore, we chose the Holarctic
species Arctosa cinerea (Fabricius, 1777) (type species of Arctosa C. L. Koch, 1847) as
outgroup, as this genus is basal to a wider concept of the Lycosinae (Murphy et al.,
2006).
Characters
There are only a limited number of phylogenetic, cladistic, or phenetic studies exploring
characters in the morphologically conservative family Lycosidae: Vink, 2002; Vink &
Paterson, 2003; Stratton, 2005; Framenau & Yoo, 2006; Yoo & Framenau, 2006 (see
also Roewer, 1959; Casanueva, 1980). We tested these characters and explored many
new ones as part of our phylogenetic analysis. A total of 27 characters remained
parsimoniously informative for the 25 species included in our analysis (Table 1;
Appendix 2). Eight characters were based on somatic morphology, 16 on genitalic
morphology (13 male and three female), and three on burrowing behaviour. We could
not score characters relating to the subterminal apophysis of the male pedipalp when
relying on secondary sources, therefore these were scored „?‟ for L. tarantula and L.
praegrandis.
Analyses
The character matrix was edited using Nexus data editor (Page, 2001) and exported for
phylogenetic analysis to TNT version 1.1 (Goloboff, Farris & Nixon, 2003, Willi
Hennig Society version). We used the „traditional search‟ option with the following
settings: number of replicates („repls‟) 1000, „trees to save per replication‟ at 10,
„collapse trees after search‟ with default collapsing rule (min. length = 0), „replace
11
existing trees‟, and maximum trees in memory set to 100 000. A strict consensus tree
was exported to Win-Clada vers. 1.00.08 (Nixon, 2002) for character exploration.
Bremer support (Bremer, 1994) and relative Bremer support (Goloboff & Farris, 2001)
values were calculated using TNT.
RESULTS
Hoggicosa now includes ten species of which four are described as new (Table 2). The
type species Lycosa errans, but also Lycosa perinflata Pulleine, 1922 and Lycosa skeeti
Pulleine, 1922 are synonymized with Hoggicosa castanea comb. nov. The males of
Hoggicosa bicolor comb. nov., Hoggicosa castanea, Hoggicosa storri comb. nov., and
Hoggicosa forresti comb. nov. are described for the first time. All Hoggicosa species
construct burrows, some with trap doors, and are predominantly found in the more arid
parts of Australia (Table 2).
Phylogeny
The phylogenetic analysis generated 26 equally parsimonious trees [length (L) = 96,
consistency index (CI) = 38, retention index (RI) = 64]. The resulting strict consensus
tree (L = 113, CI = 32, RI = 53) had little resolution in resolving relationships amongst
genera; however, Hoggicosa was monophyletic (Fig. 2). Although Bremer support
values for Hoggicosa are low, it is supported by one unambiguous synapomorphy: the
distance between the anterior pockets of the female epigynum is greater than the width
of the posterior transverse part (character 24). The genus is also unified by five
homoplasious characters: the cephalic region of the carapace is elevated, strongly
sloping away from the eyes in lateral view (1), the cymbium tip has ten to 30
macrosetae (10), the cymbium tip macrosetae are curved dorsally (11), the tip of
terminal apophysis comes to a sharp point (17), and the subterminal apophysis is
beneath the terminal apophysis and difficult to see in ventral view (19).
Hoggicosa wolodymyri sp. nov. was found to be sister to all other Hoggicosa, which
were defined by three homoplasious characters: the colour of the ventral abdomen of
females is uniformly dark (8), the ridge connecting the ventral spur and apical tip on the
tegular apophysis is curved (14), and trapdoors are present on burrows (26). Likewise,
H. forresti was found to be sister to the remaining Hoggicosa species, which were
defined by the presence of a light coloured cardiac or chevron mark on the dorsal
abdomen of females (6) (Fig. 2).
12
The remaining Hoggicosa species formed two groups. One containing Hoggicosa alfi
sp. nov., H. castanea, and Hoggicosa duracki comb. nov. is defined by the
nonhomoplasious character of a thick and opaque pars pendula (20). The group
containing H. bicolor, Hoggicosa brennani sp. nov., Hoggicosa snelli comb. nov., and
H. storri is defined by two homoplasious characters: the absence of a radial pattern on
the carapace (2) and the subterminal apophysis is easily visible next to the terminal
apophysis in ventral view (19).
Hoggicosa species with a distinct colour dimorphism between adult males and females
(H. bicolor, H. castanea, H. forresti, and H. storri, character 4) did not form a
monophyletic group, suggesting this colour pattern has evolved multiple times. Under
fast (ACCTRAN) character optimization this trait appears independently three times
and is lost once (Fig. 2), whereas under slow (DELTRAN) optimization the character
appears four times independently (Fig. 2). When the analysis was repeated without this
character included there was no difference in the resulting topology.
Lycosa was found to be paraphyletic, with the Australian representatives (Lycosa
godeffroyi and Lycosa leuckartii) not grouping with the type species L. tarantula (Fig.
2). Lycosa tarantula and L. praegrandis formed a monophyletic group based on six
homoplasious characters.
The two species of Dingosa and Geolycosa, along with Mainosa longipes (L. Koch,
1878) formed a monophyletic group supported by two nonhomoplasious characters, the
absence of macrosetae on the cymbium tip (9) and the presence of a burrow palisade
(27). Two of the Hogna species (Hogna crispipes and Hogna kuyani Framenau, Gotch
& Austin, 2006) were monophyletic based on the nonhomoplasious character of the
ventrally curved cymbium macrosetae. The third Hogna species (Hogna immansueta)
was found to group with the type species of Venator based on eight homoplasious
characters (Fig. 2). The representative of an undescribed Australian genus „Grey Wolf
Spider‟ and the monotypic Knoelle clara (L. Koch, 1877) were both placed in the
unresolved base of the tree.
13
DISCUSSION
The Australian wolf spider genus Hoggicosa Roewer, 1960 with the type species H.
errans (Hogg, 1905) is revalidated and revised to include ten species. The revision of
Hoggicosa is significant in relation to the taxonomy of the Australian wolf spider fauna.
Prior to this revision, 33 Australian species were misplaced in the putative
Mediterranean genus Lycosa. Nine of these species are treated in this revision and
removed from Lycosa, reducing the species of this genus in Australia by nearly a third.
Still, the Australian Lycosinae remain poorly known with many undescribed species
and genera, particularly from the arid interior, present in Australian collections (V. W.
Framenau, unpubl. data).
Monophyly of the genus Hoggicosa
The results of the phylogenetic analysis show clearly that Hoggicosa is a monophyletic
genus unambiguously supported by the shape of the female epigyne (distance between
anterior pockets greater than the width of the posterior transverse part, character 24).
The monophyly of Hoggicosa confirms the results of a recent molecular phylogeny that
included two Hoggicosa species (H. bicolor and H. forresti), the grouping of which was
found to be strongly supported (L. bicolor and L. castanea in Murphy et al., 2006). Our
morphological examination suggests a second synapomorphy for Hoggicosa, which is
not evident in our phylogenetic analysis as it combines two characters. This second
synapomorphy consists of ten to 30 cymbium macrosetae (character 10) which are bent
dorsally (character 11).
Relationships of Hoggicosa to other Lycosine genera
The systematic analysis resulted in an overall poor resolution of relationships amongst
genera, which appears to reflect the conservative nature of wolf spider morphology (e.g.
Vink, 2001; Stratton, 2005). Indeed, resolving relationships within the Lycosinae poses
a number of problems. A recent molecular attempt found that Lycosinae contain
paralogous copies of the 28S rRNA gene, making this gene unsuitable for analysis
(Murphy et al., 2006). A combined effort employing morphological character sets and
molecular markers may solve relationships in this morphologically conservative group,
as exemplified for the New Zealand Artoriinae (Vink & Paterson, 2003). Additional
phylogenetic signal may also be provided by morphological characters that we were not
able to explore as part of the current study. For example, spinneret morphology has
been used in phylogenetic analyses of other entelegyne spiders (e.g. Scharff &
14
Coddington, 1997; Griswold et al., 2005) and shows promising intergeneric differences
within wolf spiders (Townley & Tillinghast, 2003).
We did not find an unambiguous sister group to Hoggicosa based on our character and
taxon sample. Based on similarities in morphology and burrowing behaviour we
included Knoelle clara and a representative of an undescribed Australian genus „Grey
Wolf Spider‟ as potential sister taxa. But neither of these nor McKay‟s (1973) previous
suggestion of Geolycosa were supported as sister group by our phylogeny (Fig. 2).
Molecular studies suggest that Australian Hogna may be closely related to Hoggicosa.
The maximum parsimony analysis of molecular data by Murphy et al. (2006) found
Hogna crispipes as sister to two Hoggicosa representatives. Adding to these results,
Gotch et al. (2008) found that Hogna kuyani was sister to Hoggicosa, although the
posterior probability of this relationship was low (54%), and Hogna crispipes was basal
to both. These two Hogna species (Hogna crispipes and Hogna kuyani) were included
in our phylogeny and found to form a monophyletic group, but a sister group
relationship with Hoggicosa was not supported. In addition, a third species currently
listed in Hogna (Hogna immansueta) was found to group with the type species of
Venator, suggesting additional taxonomic problems within the six Australian species
currently placed in Hogna.
Our analysis clearly shows that some Australian species currently listed in Lycosa do
not form a monophyletic group with the type species of the genus, L. tarantula and a
congeneric L. praegrandis. Lycosa godeffroyi and L. leuckartii were placed separately
in the unresolved base of the tree, contrary to the molecular results of Murphy et al.
(2006) who found very strong support for the monophyly of these two species. They
represent a very diverse clade of common Australian Lycosinae characterized by a
typical „Union-Jack-colour pattern‟ on the cephalothorax with alternating dark and light
radial lines (character 2). Tasmanicosa tasmanica (Hogg, 1905), the type species of
Tasmanicosa, is part of this group and the genus Tasmanicosa is currently under
revision by the junior author.
The grouping of the North American representatives of Geolycosa with the Australian
genera Dingosa and Mainosa was surprising and may indicate a case of convergence.
This group was defined by the lack of cymbium macrosetae and the presence of burrow
palisades, which is an uncommon burrow modification in lycosids. All these species
15
live in sandy habitats and this shared burrowing behaviour and putative associated
morphology may be a result of adaptations to live in this substrate. Neither Dingosa nor
Mainosa were represented in Murphy et al. (2006), but Geolycosa missouriensis which
was included, was found to be the basal most lycosine (parsimony analysis) or sister to
Rabidosa (Bayesian analysis).
The revalidation of Hoggicosa places L. exigua (Roewer, 1960) from Namibia back into
Hoggicosa. A critical review of Roewer‟s (1960: 773–774, fig. 432A, B) original
description of Hoggicosa exigua clearly shows that the epigyne is not like that of
Hoggicosa or Lycosa (e.g. Zyuzin & Logunov, 2000), but much more reminiscent of
Hogna (e.g. Fuhn & Niculescu-Burlacu, 1971 for the type species of Hogna, Hogna
radiata Latreille, 1817 and Framenau et al., 2006 for Australian Hogna). We therefore
transfer Hoggicosa exigua to Hogna, Hogna exigua (Roewer, 1960) pending a revision
of the African Lycosidae related to Hogna. Unfortunately, we were not able to include
Hogna exigua in our phylogenetic analysis to confirm this transfer.
Evolution of sexual dimorphism in colour pattern
Originally distinguished by McKay (1973) as the „bicolor group‟ because of the striking
leg and body colouration of females in several species, the phylogenetic analysis under
both fast and slow optimization suggests this trait to have evolved multiple times. The
four species which display marked difference in colouration between adult males and
females (H. bicolor, H. castanea, H. forresti and H. storri, Fig. 1A, B, D, E) did not
form a distinct group. It is proposed that this trait has originated multiple times within
Hoggicosa suggesting high evolutionary pressure on conspicuous female colour
patterns or reduction in colouration of males. Whether this dimorphism is a result of
sexual or natural selection (or both) remains unresolved and requires detailed studies
into the mating behaviour and natural history of these species. If the striking colour
pattern is a result of sexual selection and subject to male mate choice, this would be a
remarkable example in sexual role reversal in spiders. For example, alternating light and
dark bands on the ventral side of the male wolf spider L. tarantula have been found to
correlate highly with body size and condition (Moya-Laraño et al., 2003). However, it
is also perceivable that a lack of colouration in males provides camouflage in their
active search for a female mate, although Hoggicosa appear to be predominantly active
at night (V. W. Framenau, pers. observ.).
16
Biogeography of Hoggicosa
All Hoggicosa species display broad geographical distributions, with some found over
all of inland Australia (H. castanea, H. alfi, and H. bicolor, Figs 10, 12, 14). This is not
surprising as wolf spiders are capable of ballooning (Greenstone, 1982) and are highly
mobile. With a distribution typical of Eyrean fauna (Heatwole, 1987) it is possible that
speciation in Hoggicosa occurred following the aridification of Australia, as seen in
many other Australian groups of fauna and flora (see review by Byrne et al., 2008).
SYSTEMATICS
FAMILY LYCOSIDAE SUNDEVALL, 1833
SUBFAMILY LYCOSINAE SUNDEVALL, 1833
GENUS HOGGICOSA ROEWER, 1960
Hoggicosa Roewer, 1955: 247 (nomen nudum) – Roewer, 1960: 772.
Type species: Lycosa errans Hogg, 1905 (by original designation). Gender feminine.
Diagnosis: Hoggicosa differs from other Lycosinae by a combination of genitalic and
somatic characters. A putative synapomorphy is proposed based on the female epigyne,
with the distance between the anterior pockets greater than the width of the posterior
transverse part (Figs 8C, 11C). An undescribed genus from Brazil shares this trait;
however, the anterior pockets extend along the anterior margin of the epigyne and join
in a groove, forming somewhat of an „m‟ shape (see Álvares, 2006: figs 127–150). A
second synapomorphy is a patch of ten to 30 dorsally curved macrosetae on the tip of
the cymbium in males (Fig. 1I). In lateral view, the shield of the prosoma is highest in
the cephalic region sloping gently towards posterior end (Fig. 3A). The prosoma is
uniform in colour or with indistinct radial pattern; median or lateral bands are absent.
Females of several species show striking contrast in the colouration of the legs and
opisthosoma (similarly coloured as penultimate males, Fig. 1A, D, F).
Most similar to Hoggicosa are the monotypic genus Knoelle and an undescribed
Australian genus represented by the „Grey Wolf Spider‟ (see Framenau & Baehr, 2007).
Knoelle also possess backwards bent macrosetae on the cymbium tip, but in a much
larger patch than in Hoggicosa (see Framenau, 2006b, fig. 2). Specimens of the
currently undescribed genus including the „Grey Wolf Spider‟ [Hickman, 1967:
17
misidentified as Dingosa simsoni (Simon, 1898)] are of similar size and shape as
Hoggicosa species and build burrows with trapdoors, but they differ by the
synapomorphies of Hoggicosa.
Description: Large and robust wolf spiders, TL 11.6–21.6 in males and 14.4–25.6 in
females. Prosoma longer than wide, length 6.4–11.4 in males and 6.9–10.7 in females.
Dorsal shield of prosoma highest in cephalic region, sloping gently towards posterior
end (Fig. 3A). Dorsal shield of prosoma uniform in colour or with faint radial pattern
(sometimes artificially pronounced when preserved in ethanol), without median or
marginal bands. AE row strongly procurved. PME greater than PLE and PME narrower
than PLE row. Labium as long as wide or slightly longer than wide. Chelicerae with
three promarginal teeth, the middle largest, and three retromarginal teeth of equal size.
Male leg colouration uniform, females of some species with alternating light and dark
metatarsus, also part of tibia in females. Legs III and IV with scopulae on tarsus and
half of metatarsus, all of the metatarsus in females.
Natural history: Hoggicosa are predominately found through semi-arid and arid regions
of Australia. All species build burrows and many construct doors from sand, with H.
snelli using pebbles or debris as a door (McKay, 1975). As the patch of macrosetae on
the male cymbium is found only in adults, it is possible that these are used for courtship
behaviour. We have made one observation of an attempted mating between a male and
female of H. alfi. When approaching the female, the male used his palps to stroke the
ground rapidly towards his body. This was carried out in repeated short bursts of less
than a second, and created small „dugouts‟ in the soft sand.
Hoggicosa are easily kept in the laboratory but can be difficult to rear past the
penultimate stage. Our observations suggest that moulting can be triggered by hot and
humid weather conditions.
Distribution: Australia.
18
KEY TO MALES OF HOGGICOSA
(Males of H. natashae are currently unknown)
1. Terminal apophysis curved apically, with tip of terminal apophysis located apically
of its connection to the palea (Figs 8B, 13A)....................................................................2
Terminal apophysis not curved apically, pointing retrolaterally, with tip of terminal
apophysis level with connection to palea (Figs 11A, 16A)...............................................8
2. Subterminal apophysis large and easily visible next to terminal apophysis in ventral
view (Fig. 13B)..................................................................................................................3
Subterminal apophysis small and hard to see beneath terminal apophysis in ventral view
(Figs 7A–D, 8B)................................................................................................................6
3. Tegular apophysis with straight ridge between ventral process and apical point (Fig.
6A–D)................................................................................................................................4
Tegular apophysis with curved ridge between ventral process and apical point (Fig. 5A–
C).......................................................................................................................................5
4. Ventral abdomen cream with black epigastric stripe (Fig. 4F)..........................H. snelli
Ventral abdomen black.......................................................................................H. bicolor
5. Ventral abdomen all black, tegular apophysis with rounded ventral process (Fig. 5G–
H)...........................................................................................................................H. storri
Ventral abdomen pale, although may have faint „V‟ pattern or spots in black (Fig. 4E),
tegular apophysis with large flange on ventral process (Fig. 5C–D)...............H. brennani
6. Tegular apophysis with curved ridge between ventral process and apical point (Fig.
5A–E), ventral abdomen with black patch........................................................................7
Tegular apophysis with straight ridge between ventral process and apical point (Fig.
5F), ventral abdomen cream or with a few black dots.................................H. wolodymyri
7. Prominent black stripe (cardiac or chevron mark) on dorsal abdomen (Fig. 1C), pars
pendula transparent and joined to embolus below embolus tip (Fig. 7C)..........H. forresti
Tan or brown stripe on dorsal abdomen, pars pendula opaque and joined to embolus at
tip (Fig. 7A)......................................................................................................H. castanea
19
8. Ventral process of tegular apophysis with bifurcate tip (Fig. 6G, H), terminal
apophysis very short and robust (Fig. 16A).......................................................H. duracki
Ventral process of tegular apophysis with rounded end (Fig. 6E), terminal apophysis
elongate and pointed, pars pendula with oval dark patch (Fig. 11B)........................H. alfi
KEY TO FEMALES OF HOGGICOSA
Body and leg colouration can be important for distinguishing females, which have very
similar epigyne morphology amongst species and are somewhat variable within species.
1. Ventral abdomen all black or with large patch of black extending to spinnerets on
ventral surface (Fig. 4B)....................................................................................................2
Ventral abdomen all pale (cream, yellow, or light orange) or with some black lines or
dots only (Fig. 4E–F).........................................................................................................7
2. Abdomen entirely black except for a pale (yellowish or cream) anterior median stripe
on the dorsal surface, femur, and part of patella black, with remainder of leg pale (Fig.
1A)......................................................................................................................H. bicolor
Dorsal abdomen pale with black transverse stripes, mottled brown or grey with
transverse lines, or black with pale stripes down lateral sides; leg colouration grey,
brown, or if alternating dark and pale segments the patella and tibia are of the same
colour.................................................................................................................................3
3. Abdomen entirely black except for pale stripes along either side extending from
spinnerets, patella and tibia black with rest of leg pale.........................................H. storri
Dorsal abdomen pale with black transverse stripes, mottled brown or grey with
transverse lines, or with black anterior median stripe; leg colouration grey, brown or if
alternating dark and pale segments with pale tibia and patella……………………….....4
4. Dorsal abdomen with prominent black stripe (cardiac or chevron mark) (Fig. 1C)
........................................................................................................................... H. forresti
Dorsal abdomen without black stripe................................................................................5
20
5. Dorsal abdomen pale with black transverse lines, epigynum with long anterior
pockets (Figs 1F, 19A–B)................................................................................H. natashae
Dorsal abdomen mottled brown or grey with transverse lines or black
dots.....................6
6. Anterior pockets of epigynum much wider than posterior transverse part (Fig. 8C)
..........................................................................................................................H. castanea
Anterior pockets of epigynum only slightly wider than posterior transverse part (Fig.
11C) ..........................................................................................................................H. alfi
7. Dorsal abdomen cream or with faint black dots only ...................................................8
Dorsal abdomen with median anterior stripe and transverse markings (Fig. 4D, H, I) ....9
8. Ventral abdomen with black line posterior to epigastric furrow (Fig. 4F)........H. snelli
Ventral abdomen without black epigastric line..................................................H. duracki
9. Legs pale orange or yellow, epigynum small with anterior pockets only slightly wider
than posterior transverse part (Fig. 24C).....................................................H. wolodymyri
Legs brown or grey, epigynum large with anterior pockets much wider than posterior
transverse part (Fig. 15C).................................................................................H. brennani
21
HOGGICOSA CASTANEA (HOGG, 1905) COMB. NOV.
(FIGS 1I, 3A, B, 4A–C, 5A, B, 7A, 8A–D, 9A, B, 10)
Lycosa castanea Hogg, 1905: 577–579, fig. 83A–B; Rainbow, 1911: 266; Bonnet,
1957: 2637; McKay, 1973: 396, fig. 3J; McKay, 1985: 75; Platnick, 1993: 487.
Lycosa errans Hogg, 1905: 579, fig. 84; Rainbow, 1911: 267; Roewer, 1955: 247;
Bonnet, 1957: 2640; McKay, 1973: 379, 394–395, fig. 3I. syn. nov.
Lycosa skeeti Pulleine, 1922: 83, pl. 5, fig. 1; Bonnet, 1957: 2664; McKay, 1973: 397–
398, fig. 3K–L. syn. nov.
Lycosa perinflata Pulleine, 1922: 84, pl. 5, fig. 2; Bonnet, 1957: 2657; McKay, 1973:
395, fig. 3F–H. syn. nov.
Allocosa castanea Roewer, 1955: 206.
Types: Holotypes. Hoggicosa castanea, ♀ from Australia: no locality given, no date
(SAM NN015).
L. errans, ♀ from Australia: no locality given [Hogg, 1905: „(without locality) sent
from Adelaide‟], no date (SAM NN016). L. skeeti, ♀ from South Australia: Wilson,
Flinders Ranges, 31°60′S, 138°21′E, iv.1908 (SAM NN019); L. perinflata, ♀ from
South Australia: Whyte Yarcowie, 33°13′S, 138°53′E, i.1908 (SAM NN017).
Other material examined: 179 males, 134 females, and five juveniles from 232 records
(Appendix 3).
Diagnosis: Hoggicosa castanea is most similar to H. brennani and H. forresti. The
subterminal apophysis of H. castanea is very small and reduced (Fig. 7A), whereas it is
much longer in H. brennani and H. forresti (Figs 7C, 15B). The pars pendula in H.
castanea is opaque and joins at the embolus tip (Fig. 7A), whereas in H. brennani and
H. forresti it is transparent and joins below the embolus tip (Figs 7C, 15B). Hoggicosa
forresti may be distinguished by the presence of a black stripe on the dorsal abdomen,
which is absent in both H. castanea and H. brennani. The venter of H. castanea, which
is black (Fig. 4B), may also be used to distinguish it from H. brennani, in which it is
pale with dark patches (Fig. 4E).
22
Description: Male: Based on SAM NN19314, Gluepot Station, Gluepot Homestead,
33°44′51′S, 140°01′07′E, South Australia (SA). Dorsal shield of prosoma brown, with
faint radial pattern, covered with black setae. Sternum and labium brown with scattered
black setae. Chelicerae dark brown with white setae. Legs brown, but ventral side of
femur paler. Opisthosoma dorsally greyish-black, with mottled pale and brown patches.
Grey median longitudinal band in anterior half with partial border of black. Remainder
of opisthosoma with faint transverse lines angled to posterior (Fig. 4A). Opisthosoma
laterally cream with black setae. Venter cream with darker central area, which does not
reach spinnerets, all covered in white setae. Terminal apophysis of pedipalps curved
slightly apically, commonly with slight twist in tip (Figs 7A, 8B). Pars pendula obvious,
opaque, and connected to embolus at embolus tip (Fig. 7A). Subterminal apophysis
present, but reduced and difficult to see under the terminal apophysis. Tegular
apophysis with rounded ventral process located centrally and projecting perpendicular.
Prominent ridge curving from ventral process to apical point (Fig. 5A).
Female: Based on SAM NN15185, Fisherman Point, Lincoln National Park, 34°45′S,
135°59′E, SA. Dorsal shield of prosoma as male but with black and white setae.
Sternum, labium, chelicerae, and legs as male. Opisthosoma dorsally as male.
Opisthosoma laterally cream with white setae and occasional black dots. Venter cream
with a black patch covered in black setae. Epigyne with small anterior pockets, often
located anterior to and far from posterior transverse part (Fig. 8C). Internal epigyne
with wide spermathecal heads (Fig. 8D). Variation: Hoggicosa castanea displays a
large range of body colouration, particularly between specimens from Western and
South Australia. Specimens from Western Australia can display a much paler dorsal
abdomen colouration (Fig. 4C) compared with that typical of H. castanea (Fig. 4A).
Some specimens from the Pilbara region of Western Australia were found to have a
reduced black pattern on the ventral abdomen. In addition, female specimens from
southern Western Australia can also display leg markings similar to that of H. forresti.
The tegular apophysis of H. castanea also differs slightly in the west of its range with a
broader ventral process and longer apical point (Fig. 5A vs. 5B). Although displaying
these differences amongst locations, the palea region and attachment of the pars
pendula, which is the most powerful character in distinguishing species, was identical
amongst all male specimens and we currently consider these conspecific.
23
Remarks: Examination of the holotypes of L. errans, L. perinflata, and L. skeeti showed
that they conform to the variation in epigynes and colouration found in all currently
available material of H. castanea. This confirms McKay‟s (1973) suggestion that L.
errans and L. perinflata are junior synonyms of H. castanea. McKay (1973) also
suggested that L. skeeti may be a subspecies of L. bicolor, but we cannot confirm this
assumption. We give L. castanea precedence over L. errans as it was established in
preceding pages of the same publication.
Measurements: ♂ NN19324 (♀ holotype): TL, 17.8 (18.6); PL, 9.3 (9.3); PW, 7.6 (7.8).
Eyes: AME, 0.50 (0.50); ALE, 0.27 (0.36); PME, 1.04 (1.00); PLE, 0.86 (0.91).
Sternum (length/width): 4.1/3.6 (4.1/3.7). Labium (length/width): 1.4/1.4 (1.6/1.6). OL,
8.6 (9.3); OW, 5.0 (6.4). Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 4.6 + 4.4 + – + 3.6 = 12.6; I, 9.3 + 11.1 + 8.7 + 4.7 =
33.8; II, 8.8 + 10.6 + 8.6 + 4.6 = 32.6; III, 8.1 + 9.3 + 8.7 + 4.4 = 30.5; IV, 10.1 + 11.4
+ 11.7 + 4.8 = 38.0 (pedipalp, 4.3 + 4.6 + – + 3.1 = 12.0; I, 8.6 + 10.3 + 6.8 + 4.0 =
29.7; II, 8.4 + 9.7 + 7.0 + 3.8 = 28.9; III, 7.7 + 8.7 + 7.3 + 3.8 = 27.5; IV, 9.7 + 11.0 +
10.1 + 4.3 = 35.1).
♂ (♀) (range, mean ± SD): TL, 14.3–20.7, 18.0 ± 1.8; PL, 8.0–10.7, 9.6 ± 0.8; PW, 6.3–
8.6, 7.7 ± 0.7; N = 10 (TL, 17.9–25.3, 20.7 ± 2.0; PL, 10.0–11.3, 10.6 ± 0.4; PW, 8.4–
9.4, 8.9 ± 0.4; N = 11).
Natural history: Hoggicosa castanea has been collected from areas with white sand and
limestone, red sandy loam, clay, or coastal dunes and rocky hills. This species has been
found in association with Acacia, Melaleuca, and Black Box (Eucalyptus largiflorens)
woodlands, as well as Callitris, Mulga (Acacia anuera), Mallee (Eucalyptus), and
Spinifex (Triodia) habitats. Adult females have been collected all year round with adult
males present from November to May. They build burrows with trapdoors, which can
be very well camouflaged (Fig. 9A, B).
Distribution: New South Wales, Northern Territory, South Australia, Victoria,
Queensland, and Western Australia (Fig. 10).
24
HOGGICOSA ALFI SP. NOV.
(FIGS 1G, H, 6E, F, 11A–E, 12)
Types: Holotype. ♂ from Western Australia: Lorna Glen Station, 26°12′04′S,
121°18′14′E, 31.x.–7.xi.2002, M.A. Cowan et al. (WAM T77405).
Paratypes. 1 ♀ (WAM T77406) and 4 ♂s (WAM T53919), same data as holotype.
Other material examined: 397 males, 53 females, and 20 juveniles from 191 records
(Appendix 3).
Etymology: The specific epithet is a patronym in honour of the senior author‟s recently
deceased grandfather, Alf Cain, in appreciation for teaching me how to fish and the
importance of a firm handshake.
Diagnosis: Males of H. alfi can be distinguished from all other Hoggicosa by the
presence of a dark oval patch on the pars pendula and an elongated terminal apophysis
which points retrolaterally with only a slight apical bend (Fig. 11A, B). Females can be
distinguished from all other Hoggicosa by the unique shape of the epigynum, which has
broad anterior pockets and a comparatively wide posterior transverse part (Fig. 11C).
Description: Male: Based on holotype. Dorsal shield of prosoma orange-brown, darker
in eye quadrangle, with a faint radial pattern; covered with short black setae. Sternum
and labium dark brown with scattered black setae. Chelicerae dark brown with white
setae. Legs orange-brown. Opisthosoma dorsally mottled grey. Brown median
longitudinal band at anterior end with faint transverse lines covering rest of
opisthosoma (Fig. 1G). Cover of grey setae with longer black bristles scattered
throughout. Opisthosoma laterally cream, venter black. Terminal apophysis of pedipalp
pointing retrolaterally (Fig. 11A). Pars pendula connected to embolus near embolus tip,
with unique dark oval patch (Fig. 11B). Subterminal apophysis small and only partly
visible under terminal apophysis (Fig. 11B). Tegular apophysis with large rounded
ventral process located towards apical point, with continuous ridge curving to the apical
point (Fig. 6E).
25
Female: Based on paratype. Dorsal shield of prosoma similar to male but with darker
radial pattern and cover of fine white setae. Sternum, labium, and chelicerae as male.
Legs orange-brown, with the prolateral surface of the femur (especially leg I) darker.
Ventral surface of patella darker than femur, less so for leg I. Opisthosoma dorsally pale
(yellowish-cream) with scattered black dots and a faint anterior median band (Fig. 1H).
Covered with grey setae, black setae forming dots from which a black bristle extends.
Opisthosoma laterally cream with some black patches, venter black. Epigyne with broad
anterior pockets, the base of which the median septum enters almost at right angles (Fig.
11C). Posterior transverse part large and long. Internal epigyne with spermathecae
wider than anterior pockets (Fig. 11D).
Variation: The tegular apophysis and terminal apophysis of males are somewhat
variable within this species. The terminal apophysis of some males points more
retrolaterally (little curve apically). The ridge between the ventral process of the tegular
apophysis and apical point can also point retrolaterally with little curve (see Fig. 6E, F).
The size of the female epigynum can vary (Fig. 11C, E). The opisthosoma of some
females may be mottled and darker than described above.
Measurements: ♂ holotype (♀ paratype): TL, 16.8 (21.3); PL, 9.7 (10.1); PW, 7.1 (7.3).
Eyes: AME, 0.5 (0.54); ALE, 0.27 (0.36); PME, 0.95 (1.23); PLE, 0.82 (1.14). Sternum
(length/width): 4.3/3.4 (4.1/3.4). Labium (length/width): 1.2/1.1 (1.6/1.4). OL, 7.1
(11.1); OW, 4.3 (8.3). Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 4.4 + 3.8 + – + 3.1 = 11.3; I, 8.6 + 9.7 + 8.0 + 4.4 =
30.7; II, 8.0 + 9.7 + 7.8 + 4.4 = 29.9; III, 7.8 + 8.6 +7.8 + 4.3 = 28.5; IV, 9.3 + 10.7 +
10.0 + 4.4 = 34.4 (pedipalp, 4.6 + 4.3 + – + 3.0 = 11.9; I, 7.8 + 9.3 + 6.0 + 3.1 = 26.2;
II, 7.6 + 9.0 + 6.0 + 3.3 = 25.9; III, 7.1 + 8.6 + 6.4 + 3.6 = 25.7; IV, 8.4 + 10.3 + 8.6 +
3.6 = 30.9).
♂ (♀) (range, mean ± SD): TL, 14.3–20.0, 17.4 ± 1.4; PL, 7.9–10.1, 9.2 ± 0.7; PW, 6.0–
7.9, 7.0 ± 0.5; N = 25 (TL, 15.7–22.4, 18.1 ± 1.9; PL, 7.6–11.0, 9.2 ± 1.0; PW, 5.7–7.9,
6.9 ± 0.7; N = 13).
Natural history: Hoggicosa alfi has been collected from yellow sand plains, red dunes,
interdunes, claypan edges, and stony tablelands. Specimens have been recorded in
association with Callitris woodland, Mallee (Eucalyptus), Grevillea, and Banksia with
Verticordia, Mulga (Acacia aneura), and Spinifex (Triodia) vegetation. Adult males
26
have been collected from September to December with adult females caught through
August to May. This species excavates burrows, but does not seal them with doors.
Distribution: New South Wales, Queensland, South Australia, and Western Australia
(Fig. 12).
27
HOGGICOSA BICOLOR (HOGG, 1905) COMB. NOV.
(FIGS 1A, B, 2A, 13A–D, 14)
Lycosa bicolor Hogg, 1905: 580–582, fig. 85A–B; Rainbow, 1911: 266; Strand, 1913:
618; Bonnet, 1957: 2636; McKay, 1973: 378, 381–385, figs 1A–E, 2A–C; Main, 1976:
149, 231; McKay, 1985: 75; Platnick, 1993: 486.
Allocosa bicolor Roewer, 1955: 205.
Types: Lectotype (designated by McKay, 1973). ♀ from South Australia: no locality
given, no date (SAM NN012).
Paralectotypes. South Australia: 1 ♀, no locality given, no date (SAM NN011); 1
juvenile, no locality given, no date (SAM NN013).
Other material examined: 335 males, 95 females, and 35 juveniles from 283 records
(Appendix 3).
Diagnosis: The male palp of H. bicolor is most similar to H. snelli, but these two
species can be easy distinguished by abdomen colouration. Male H. bicolor have a grey
opisthosoma and black venter, whereas male H. snelli have a cream opisthosoma and
venter with a black epigastric stripe (Fig. 4F). Females and juveniles can be readily
distinguished from all other Hoggicosa species by the striking colouration of the legs
and abdomen (Fig. 1A).
Description: Male: Based on WAM T62336, Mt Vernon Station, 24°30′S, 118°30′E,
Western Australia (WA). Dorsal shield of prosoma brown, covered in short black and
white setae. Sternum and labium brown with scattered black setae. Chelicerae dark
brown with white setae. Legs brown. Opisthosoma grey with cover of grey and black
setae (Fig. 1B). Opisthosoma laterally with faint longitudinal lines and black and white
setae. Venter black with black setae. Terminal apophysis of pedipalp large and strongly
curved apically (Fig. 13A). Pars pendula thin, transparent, and connected to embolus
near embolus base (Fig. 13B). Subterminal apophysis large and easily visible next to
terminal apophysis. Tegular apophysis with small, pointed ventral process, located close
to apical point. Straight ridge between ventral process and apical point (Fig. 6A).
28
Female: Based on WAM T62336, data as above. Dorsal shield of prosoma reddishbrown, darker in eye quadrangle, cover of fine white setae. Sternum, labium, and
chelicerae as male. Femur and first part of patella of all legs black–dark brown, with
remainder of leg cream (can have almost yellow tinge when alive) (Fig. 1A).
Opisthosoma dorsally black covered in fine black setae, with prominent cream anterior
median lanceolate stripe (Fig. 1A). Opisthosoma laterally and ventrally black with black
setae. Epigynum simple, with small anterior pockets located close to median septum
(Fig. 13C). Internal epigyne with large spermathecal heads, which are very close to the
anterior pockets (Fig. 13D).
Variation: The size and shape of the pale lanceolate stripe on the opisthosoma of
females can vary amongst individuals from a small streak at the anterior end to a large
band nearly reaching the spinnerets and covering most of the dorsal surface (see
McKay, 1973, fig. 1B–E). Females and juveniles may sometimes have cream markings
on the black dorsal femur (Fig. 1A).
Remarks: As the lectotype female is in poor condition, a representative male and female
have been used for the redescription of H. bicolor.
Measurements: ♂ (♀): TL, 18.6 (25.4); PL, 10.0 (11.8); PW, 7.6 (8.6). Eyes: AME,
0.54 (0.59); ALE, 0.27 (0.36); PME, 1.36 (1.41); PLE, 1.09 (1.27). Sternum
(length/width): 4.6/3.3 (4.8/3.6). Labium (length/width): 1.4/1.3 (1.8 /1.8). OL, 8.6
(13.6); OW, 5.0 (8.8). Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 5.1 + 5.3 + – + 3.6 = 14.0; I, 8.6 + 10.7 + 8.6 + 4.6 =
32.5; II, 8.6 + 10.6 + 8.1 + 4.6 = 31.9; III, 7.8 + 9.3 + 7.8 + 4.6 = 29.5; IV, 10.0 + 11.4
+ 10.3 + 5.0 = 36.7 (pedipalp, 5.4 + 5.7 + – + 3.6 = 14.7; I, 9.6 + 11.6 + 7.4 + 4.3 =
32.9; II, 9.3 + 11.4 + 7.6 + 4.3 = 32.6; III, 8.6 + 9.8 + 7.8 + 4.1 = 30.3; IV, 10.4 + 12.8
+ 10.7 + 4.8 = 38.7).
♂ (♀) (range, mean ± SD): TL, 13.6–18.6, 16.2 ± 1.4; PL, 7.4–10.0, 8.8 ± 0.7; PW, 5.4–
7.1, 6.5 ± 0.5; N = 23 (TL, 15.0–25.0, 20.2 ± 3.0; PL, 7.9–12.0, 10.0 ± 1.4; PW, 5.9–
9.1, 7.6 ± 1.0; N = 13).
Natural history: Hoggicosa bicolor has been collected from areas with sandy plains, red
sand, claypans, and stony soil. Found in locations with Mulga (A. aneura) and A.
estrophiolata, Ironwood (A. estrophiolata) woodland, Eucalyptus socialis, chenopod
29
scrubland (Atriplex and Mairean), and Spinifex (Triodia irritans). Adult females have
been collected all year round with adult males recorded from August to April. This
species has been dug up from burrows with and without doors.
Distribution: New South Wales, Northern Territory, Queensland, South Australia, and
Western Australia (Fig. 14).
30
HOGGICOSA BRENNANI SP. NOV.
(FIGS 4D, E, 5C, D, 15A–D, 18)
Types: Holotype. ♂ from South Australia: 1.5 km south-west Middle dam, Taylorville
Station, 33°53′10′S, 140°18′32′E, 8–13.xii.2000, Royal Geographic Society of South
Australia (RGS)/Bookmark Survey, TV04 (SAM NN17017).
Paratype. ♀ from South Australia: Casuarina Dam, Taylorville Station, 33°53′10′S,
140°18′32′E, 10.x.2000, RGS/Bookmark Survey, TV-camp, burrow with trapdoor
(SAM NN17029).
Other material examined: 53 males, 27 females, and four juveniles from 64 records
(Appendix 3).
Etymology: The specific epithet is a patronym in honour of Karl E. C. Brennan in
recognition of his work on the ecology of Australian spiders. The senior author also
thanks him for his support and friendship.
Diagnosis: The pedipalps of H. brennani most closely resemble those of H. castanea
and H. forresti. The pars pendula, which is transparent in H. brennani and joins below
the embolus tip (Fig. 15B), may be used to distinguish it from H. castanea, in which it
is opaque and joins at the embolus tip. In addition the subterminal apophysis of H.
brennani is much longer than that of H. castanea (Figs 7A, 8B). The ventral process on
the tegular apophysis of H. brennani has a flange on the prolateral side which is absent
in H. forresti (Fig. 5C, D vs. 5E). Male and female H. brennani have a pale venter with
dark patterning, whereas H. castanea and H. forresti have a black venter (Fig. 4B vs.
4D).
Description: Male: Based on holotype. Dorsal shield of prosoma orange-brown in
colour, darker in eye quadrangle, with black and white setae. Sternum pale orange,
labium brown, both with scattered black setae. Chelicerae dark brown with white setae.
Legs brown. Opisthosoma dorsally mottled. Brown median longitudinal stripe at
anterior end with partial edging of black. Faint transverse lines (grey/black) over rest of
opisthosoma (Fig. 4D). Cover of black, grey, and white setae. Opisthosoma laterally
cream with scattered black patches. Venter cream with faint V-shape made of black
patches of black setae (Fig. 4E). Terminal apophysis of pedipalp curved apically (Fig.
31
15A). Pars pendula transparent and connected to embolus just below embolus tip (Fig.
15B). Subterminal apophysis next to terminal apophysis (Fig. 15B). Tegular apophysis
with a large ventral process located centrally and pointing away from tip of tegular
apophysis. Ventral process with flange on prolateral side, which has a characteristic
notch when viewed from anterior of pedipalp (Fig. 5C, D). Ridge from ventral process
to apical point present and curved (Fig. 5C).
Female: Based on paratype. Dorsal shield of prosoma as male. Sternum, labium,
chelicerae, and legs as male. Opisthosoma dorsally and laterally as male (Fig. 4D, F).
Venter cream with some scattered black dots that have a long black setae extending.
Epigyne with small anterior pockets greater in width than posterior transverse part (Fig.
15C). Internal epigyne with clearly defined channel from anterior pockets to
spermatheca (Fig. 15D).
Variation: The abdomen colouration of H. brennani can vary. In some specimens the
dorsal markings may be much paler and the ventral abdomen nearly completely cream.
Likewise, some specimens display a more pronounced ventral marking with a greater
number of black dots and enhanced black lines.
Measurements: ♂ holotype (♀ paratype): TL, 19.8 (18.4); PL, 9.8 (9.6); PW, 7.9 (7.6).
Eyes: AME, 0.46 (0.50); ALE, 0.31 (0.42); PME, 0.96 (1.15); PLE, 0.77 (1.00).
Sternum (length/width): 4.5/3.9 (4.1/3.6). Labium (length/width): 1.6/1.4 (1.6/1.5). OL,
10.0 (8.8); OW, 6.2 (6.1). Legs, lengths of segments (femur + patella/tibia + metatarsus
+ tarsus = total length): pedipalp, 5.1 + 5.2 + – + 4.0 = 14.3; I, 9.9 + 12.0 + 9.2 + 5.2 =
36.3; II, 9.6 + 11.6 + 9.0 + 5.1 = 35.3; III, 8.4 + 10.0 + 9.2 + 4.7 = 32.3; IV, 10.0 + 12.1
+ 11.2 + 5.4 = 38.7 (pedipalp, 4.9 + 5.0 + – + 3.6 = 13.5; I, 8.8 + 9.9 + 6.2 + 3.8 = 28.7;
II, 8.1 + 9.4 + 6.4 + 3.8 = 27.7; III, 7.2 + 8.5 + 7.4 + 3.6 = 26.7; IV, 9.0 + 10.6 + 9.4 +
4.4 = 33.4).
♂ (♀) (range, mean ± SD): TL, 14.3–20.0, 17.1 ± 2.3; PL, 7.5–11.4, 9.0 ± 1.3; PW, 6.1–
9.0, 7.1 ± 1.0; N = 8 (TL, 18.1–25.6, 20.4 ± 3.0; PL, 8.8–11.9, 9.8 ± 1.3; PW, 6.9–9.4,
7.8 ± 1.0; N = 5).
32
Natural history: Hoggicosa brennani has been recorded from sand and dune locations
with records of Mallee (Eucalyptus) vegetation with mixed understorey and Spinifex
(Triodia). Adult females have been collected all year round with adult males found from
October to March. This species builds burrows with trapdoors.
Distribution: New South Wales, Queensland, and South Australia (Fig. 18).
33
HOGGICOSA DURACKI (MCKAY, 1975) COMB. NOV.
(FIGS 6G, H, 7B, 16A–E, 18)
Lycosa duracki McKay, 1975: 313–316, fig. 2A–E; Brignoli,
1983: 450; McKay, 1985: 76.
Types: Holotype. ♀ from Western Australia: Old Argyle Downs Station (today
submerged under Argyle Dam), Ord River, 16°12′S, 128°48′E, 23.x.1971, R. J. McKay,
W. H. Butler, with young spiderlings (WAM 74/494).
Paratypes. 1 ♂ and 2 ♀s from same location as holotype: 5.x.1971 (WAM 74/495-7).
Other material examined: Six males and three females from five records (Appendix 3).
Diagnosis: Males can be distinguished from the similarly coloured H. snelli by a very
short terminal apophysis (Fig. 16A) and a large tegular apophysis, which has a ventral
process with a bifurcate tip (Fig. 6G, H). Both sexes can be distinguished from H. snelli
by the plain cream venter which lacks the black stripe of H. snelli (Fig. 4F).
Description: Male: Based on paratype. Dorsal shield of prosoma pale orange, covered
in fine black and white setae. Sternum pale orange, labium orange-brown, both with
scattered black setae. Chelicerae dark brown with white setae. Legs pale orange-yellow.
Opisthosoma dorsally cream, cover of fine black setae with longer black bristles
scattered throughout. Opisthosoma laterally cream, venter cream with white setae.
Terminal apophysis of pedipalp very short, robust, and pointing retrolaterally (Fig. 16A,
B). Pars pendula thick and opaque, connected to embolus at embolus tip (Fig. 7B).
Large tegular apophysis with a long ventral process located basally and pointing
strongly away from tip of tegular apophysis. Ventral process with a bifurcate tip and no
continuous ridge to the apical point (Fig. 6G, H).
Female: Based on holotype. Dorsal shield of prosoma pale orange-yellow with fine
white setae. Sternum, labium, and chelicerae as male. Legs pale yellow. Opisthosoma
dorsally cream, covered with white setae and scattered longer black bristles.
Opisthosoma laterally cream, venter cream with two faint dark spots at anterior end.
Epigyne with small anterior pockets, close to the median septum (Fig. 16E).
34
Remarks: The epigyne of one of the female Paratypes (WAM 74/496, Fig. 16C, D) is
vastly different to that of the holotype (Fig. 16E). Unfortunately, the epigyne of the
second female paratype (WAM 74/497) is missing, but from McKay‟s (1975: fig. 2E)
figure of the ventral view it appears to match that of the holotype. This difference may
indicate that the epigynes of H. duracki are highly variable. However, the elongated
structure of the ventral process on the tegular apophysis of the male specimens appears
unlikely to „match‟ the holotype epigyne (see Zyuzin, 1993). The dimensions of the
tegular apophysis fit better with that of the paratype epigyne figured here (Fig. 16C).
Therefore, the females of H. duracki may represent two species, but given the current
lack of material, in particular a morphologically different male, we currently consider
them as conspecific.
Measurements: ♂ paratype (♀ holotype): TL, 18.8 (19.4); PL, 9.4 (10.6); PW, 8.0 (8.0).
Eyes: AME, 0.50 (0.62); ALE, 0.35 (0.38); PME, 1.15 (1.35); PLE, 0.81 (1.23).
Sternum (length/width): 4.4/4.0 (4.9/3.8). Labium (length/width): 1.5/1.3 (1.5/1.5). OL,
9.4 (8.8); OW, 5.7 (6.2). Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 4.4 + 4.3 + – + 3.8 = 12.5; I, 9.4 + 11.4 + 9.4 + 4.7 =
34.9; II, 9.1 + 10.8 + 9.4 + 4.7 = 34.0; III, 8.6 + 9.8 + 9.3 + 4.4 = 32.1; IV, 10.1 + 11.8
+ 11.4 + 4.8 = 38.1 (pedipalp, 5.0 + 5.0 + – + 3.6 = 13.6; I, 8.2 + 10.2 + 6.2 + 3.4 =
28.0; II, 7.9 + 9.6 + 6.2 + 3.6 = 27.3; III, 7.5 + 8.8 + 6.2 + 3.8 = 26.3; IV, 8.8 + 10.6 +
8.1 + 4.4 = 31.9).
♂ (♀) (range, mean ± SD): TL, 15.7–18.8, 16.8 ± 1.3; PL, 7.9–9.4, 8.7 ± 0.7; PW, 6.1–
8.0, 7.2 ± 0.8; N = 4 (TL, 19.4–19.8, 19.5 ± 0.2; PL, 9.5–10.6, 10.0 ± 0.6; PW, 7.4–8.1,
7.8 ± 0.4; N = 3).
Natural history: Hoggicosa duracki have been collected from bare gravel slopes and
ridges without vegetation in heavy clay-gravel. Burrows were 15–20 cm deep and up to
14 mm diameter with or without hinged doors (McKay, 1973). Mature males and
females have been collected in October and November. The holotype female was
collected with young in October.
Distribution: Northern Western Australia (Fig. 18).
35
HOGGICOSA FORRESTI (MCKAY, 1973) COMB. NOV.
(FIGS 1C, 5E, 17A–D, 18)
Lycosa forresti McKay, 1973: 385–389, figs 1F–G, 2D–G; Main, 1976: 138–141, 149,
231, fig. 37B, plate B7; Brignoli, 1983: 450; McKay, 1985: 77.
Types: Holotype. ♀ from Western Australia: 8 miles west of Moorine Rock, 8.i.1970,
W. H. Butler (WAM 70/44).
Paratypes. Western Australia: 1 ♀, Buntine Reserve, c. 3 miles east of Buntine Railway
Station, 29°59′S, 116°42′E (WAM 72/635); 2 ♀, 1 juvenile (juv.), Buntine Reserve, c. 3
miles east of Buntine Railway Station, 29°59′S, 116°42′E (WAM 72/639-41); 1 ♀,
Hyden, 32°27′S, 118°52′E (WAM 69/801); 1 juv., Lake Moore, near south end,
30°20′S, 117°58′E (WAM 71/198); 1 ♀, Nevoria mine, 10 miles east-south-east Marvel
Loch, 31°30′S, 119°34′E (WAM 70/30); 1 ♀, Mt Magnet, 323 mile peg, 28°03′S,
117°50′E (WAM 69/467); 1 ♀, Rudall River, 22°28′S, 122°29′E (WAM 71/1151); 1 ♀,
Southern Cross, 31°14′S, 119°19′E (WAM 72/634); 1 ♀, Southern Cross, 6 miles east,
31°16′S, 119°25′E (WAM 69/40); 1 juv., Tammin, 31°38′S, 117°29′E (WAM 69/38); 1
juv., Wongan Hills, 106.6 miles north-east, (WAM 69/792); 1 ♀, Wongan Hills, Ballidu
Road, 135 mile peg, 30°54′S, 116°43′E (WAM 69/827); 1 juv., Wongan Hills - Ballidu
Road, 135 mile peg, 30°54′S, 116°43′E (WAM 69/828); 1 juv., Wubin, 30°07′S,
116°38′E (WAM 69/41); 1 juv., Wubin, 20 miles north-east, 29°54′S, 116°52′E (WAM
69/43); 1 ♀, Wubin, 10 miles north-east, 30°00′S, 116°31′E (WAM 69/456); 1 ♀,
Yandil Station, 26°22′S, 119°49′E (WAM 38/916); 1 ♀, 6 juv., Yellowdine, 38 miles
south, 31°51′S, 119°39′E (WAM 71/69-75). Misidentification, these are H. alfi: 1 ♀, Mt
Magnet, 323 mile peg, 28°03′S, 117°50′E (WAM 69/791); 1 ♀, Paynes Find area, 323
mile peg, 29°15′S, 117°41′E (WAM 70/186).
Misidentification, these are H. castanea: 1 ♀, Morawa, 29°13′S, 116°00′E (WAM
70/172); 1 ♀, Mt Magnet, 323 mile peg, 28°03′S, 117°50′E (WAM 69/46); 1 ♀, Kulin,
32°40′S, 118°9′E (WAM T53819; 33/1607); 1 ♀, Coonana, 12 miles north-west,
30°54′S, 123°01′E (WAM 69/35); 1 ♀, Laverton, Police Station, 28°38′S, 122°24′E
(WAM 26/716, published as WAM 26/717 in McKay, 1973); 1 ♀, Marloo Station,
28°19′S, 116°11′E (WAM 69/42). Currently missing: 1 ♀, Carrabin (WAM 69/37); 1
juv., no locality (WAM 71/76); 1 ♂, no locality (WAM 69/465).
36
Other material examined: 64 males, 48 females, and 19 juveniles from 105 records
(Appendix 3).
Diagnosis: Most similar to H. forresti are H. brennani and H. castanea. Males and
females of H. forresti may be distinguished from both by the presence of a prominent
black lanceolate stripe on the anterior of the dorsal abdomen (Fig. 1C). In addition, H.
brennani has a pale venter with dark patterning compared with the black venter of H.
forresti and H. castanea. McKay (1973) indicated the leg colouration of forresti, with a
pale diamond on the femur, as a diagnostic feature, but females of H. castanea can also
display this leg coloration, but lack a dark lanceolate stripe. Males of H. forresti may be
distinguished from H. castanea by the pars pendula, which is thin and transparent and
joins below the embolus tip (Fig. 7C), whereas in H. castanea it is thick and opaque and
joins at the tip of the embolus (Fig. 7A). The tegular apophysis may be used to
distinguish H. brennani males, which have a flange on the ventral process (Fig. 5C, D)
that is lacking in H. forresti (Fig. 5E).
Description: Male: Based on WAM T47762, North Baandee Nature Reserve, 31°38′S,
117°43′E, WA. Dorsal shield of prosoma brown, faint radial pattern, covered with black
and white setae. Sternum light brown, labium brown, with scattered black setae.
Chelicerae dark brown with white setae. Legs brown with black setae, pale diamond
shape at base of femurs. Also pale with white setae on retrolateral side of ventral
surface of legs I and II. Opisthosoma dorsally mottled grey. Black median lanceolate
stripe at anterior end with black setae (Fig. 1C). Cover of black and white setae.
Opisthosoma laterally cream with white setae. Venter with black triangular patch
extending to spinnerets. Terminal apophysis of pedipalps strongly curved apically (Fig.
17A, B). Pars pendula transparent and connected to embolus just below embolus tip
(Fig. 7C). Subterminal apophysis present, but small and difficult to see beneath terminal
apophysis (Fig. 7C). Tegular apophysis with rounded ventral process projecting
perpendicular. Prominent curved ridge between ventral process and apical point (Fig.
5E).
Female: Based on WAM T47762, data as above. Dorsal shield of prosoma pale orange
with white setae covering. Sternum, labium, and chelicerae as male. Legs dark brown
with black setae, same pale diamond shape on femur as male. Ventral side of legs on
37
femur and patella brown, remainder pale. Opisthosoma dorsally as male with faint
transverse rows from end of black stripe to spinnerets. Opisthosoma laterally cream
with some black patches. Venter as male. Epigyne with broad anterior pockets (Fig.
17C). Internal epigyne with large ovoid anterior pockets and „s‟ shaped sclerotized
median septum channels (Fig. 17D).
Variation: The carapace of males can be darker with a more obvious radial pattern;
some display a less obvious leg pattern or lack it altogether with grey/brown legs. The
dorsal opisthosoma can vary but always has a dark lanceolate stripe. The dark
lanceolate stripe is sometimes surrounded by cream or with black extensions in the
middle (bulges). The length between the process and the tip of the tegular apophysis can
vary, but the pars pendula and subterminal apophysis are always the same.
Remarks: McKay (1973) noted atypical specimens from Forrest, Rawlinna, and
Fitzgerald River in his description. Our examination of these specimens identified them
as H. castanea.
Measurements: ♂ (♀) both T47762: TL, 18.1 (20.3); PL, 9.6 (11.0); PW, 8.0 (8.6).
Eyes: AME, 0.54 (0.54); ALE, 0.32 (0.36); PME, 0.95 (1.32); PLE, 0.91 (1.14).
Sternum (length/width): 4.1/3.6 (4.8/4.0). Labium (length/width): 1.45/1.36 (1.59/1.59).
OL, 8.6 (9.3); OW, 4.3 (6.0). Legs, lengths of segments (femur + patella/tibia +
metatarsus + tarsus = total length): pedipalp, 4.6 + 4.3 + – + 3.6 = 12.5; I, 9.7 + 11.4 +
9.3 + 5.0 = 35.4; II, 9.3 + 10.8 + 9.3 + 4.8 = 34.2; III, 8.6 + 10.0 + 9.6 + 4.8 = 33.0; IV,
10.7 + 12.1 + 12.1 + 5.6 = 40.5 (pedipalp, 5.0 + 5.0 + – + 3.6 = 13.6; I, 9.3 + 11.4 + 7.1
+ 4.3 = 32.1; II, 8.8 + 10.7 + 7.1 + 4.3 = 30.9; III, 7.8 + 9.7 + 8.3 + 4.3 = 30.1; IV, 10.0
+ 12.1 + 11.4 + 5.0 = 38.5).
♂ (♀) (range, mean ± SD): TL, 13.6–20.0, 16.8 ± 1.7; PL, 7.9–10.3, 9.0 ± 0.7; PW, 6.3–
8.3, 7.3 ± 0.6; N = 31 (TL, 17.1–22.4, 20.4 ± 1.3; PL, 9.3–11.4, 10.5 ± 0.6; PW, 7.1–
9.4, 8.6 ± 0.6; N = 18).
Natural history: Hoggicosa forresti has been collected from gritty, stony, and fine
clayey loams as well as sandplains. Found in woodlands of Gimlet (Eucalyptus
salubris), Salmon Gum (E. salmonophloia), and E. dundasii as well as Mallee
(Eucalyptus) and Spinifex (Triodia). Adult females were collected all year round and
38
adult males from November to May. This species excavates burrows armed with a
trapdoor (see Main, 1976, fig. 37B).
Distribution: Southern Western Australia and South Australia (Fig. 18). The record of a
specimen from Cottesloe, Perth (WAM 22/5) is considered dubious and may be
mislabelled.
39
HOGGICOSA NATASHAE SP. NOV.
(Figs 1F, 19A–D, 20, 22)
Types: Holotype. ♀ from South Australia: Lake Gilles, 32°41′20′S, 136°55′20′E,
9.xii.1994, P. Hudson (SAM NN14785).
Paratypes. South Australia: 1 ♀ from Lake Gilles, 32°41′20′S, 136°55′20′E, 15.v.1993,
P. Hudson (SAM NN14786); 1 ♀ from Lake Gilles, 32°43′S, 136°47′E, i.1996, P.
Hudson (SAM NN13801).
Other material examined: Seven females and one juvenile from six records (Appendix
3).
Etymology: The specific epithet is a matronym in honour of the senior author‟s mother,
Natasha Langlands, in appreciation for all her love and support.
Diagnosis: This species can be distinguished from all other Hoggicosa by its striking
dorsal abdominal pattern, which consists of black transverse markings on a pale cream
abdomen (Fig. 1F). In addition, the anterior pockets of the epigynum are much larger
than in any other species (Fig. 19A).
Description: Male: Currently unknown.
Female: Based on holotype. Dorsal shield of prosoma orange-brown, darker in eye
quadrangle, faint radial pattern and cover of white setae. Sternum and labium brown
with scattered black setae. Chelicerae dark brown with white setae. Legs grey.
Opisthosoma dorsally cream with black transverse lines (Fig. 1F). Opisthosoma
laterally and ventrally cream. Epigynum with broad and very elongate anterior pockets
(Fig. 19A). Internal epigyne with spermatheca slightly wider than anterior pockets (Fig.
19B).
Remarks: A juvenile female displays the same dorsal abdominal pattern.
40
Measurements: ♀ holotype: TL, 19.0; PL, 9.0; PW, 6.8. Eyes: AME, 0.50; ALE, 0.36;
PME, 1.04; PLE, 1.00. Sternum (length/width): 3.8/3.1. Labium (length/width): 1.4/1.1.
OL, 10.0; OW, 7.1. Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 4.3 + 4.0 + – + 2.7 = 11.0; I, 7.3 + 8.6 + 5.7 + 2.8 =
24.4; II, 7.0 + 8.3 + 5.4 + 2.8 = 23.5; III, 6.3 + 7.4 + 6.0 + 2.8 = 22.5; IV, 7.7 + 9.1 +
8.1 + 3.3 = 28.2.
♀ (range, mean ± SD): TL, 16.7–23.6, 20.4 ± 3.3; PL, 8.9–11.4, 10.1 ± 1.2; PW, 6.4–
8.6, 7.4 ± 0.9; N = 5.
Natural history: Several specimens have been collected in low depressions covered
with vegetation of Chenopods and Samphire. Mature females collected from December
to May. The holotype was dug from a burrow with a thick bathtub plug-like door (Fig.
20).
Distribution: New South Wales, Queensland, and South Australia (Fig. 22).
41
HOGGICOSA SNELLI (MCKAY, 1975) COMB. NOV.
(FIGS 4F, G, 6B–D, 21A–E, 22)
Lycosa snelli McKay, 1975: 313–316, fig. 1A–G; Main, 1976: 141, fig. 32D; Brignoli,
1983: 450; McKay, 1985: 83.
Types: Holotype. ♀ from Western Australia: Towera Station, north of Lyndon River,
23°11′S, 115°07′E, i.1952, A. Snell (WAM 69/797).
Paratypes. Western Australia: 2 juv., Barradale, 18 km south, 22°50′S, 114°57′E (QM
W4021); 2♂, 1 ♀, Barrow Island, 20°48′S, 115°24′E (WAM 74/498-9, 71/1716); 1 ♀,
Carnarvon, 14.5 km north, on NW Highway, 24°50′S, 113°47′E (WAM 69/1035); 2
juv., Lyndon Station, 23°38′S, 115°15′E (WAM 69/798-9); 1 ♀, 2 juv., Lyndon Station,
via Carnarvon, 23°38′S, 115°15′E (WAM 69/803-5); 12 juv., Manberry, 7 miles from,
towards Wandagee, 23°56′S, 114°10′E (WAM 37/117-28, published as 72/117-28 in
McKay (1973); 1 juv., Mardie Station, 21°13′S, 115°58′E (WAM 71/1718); 1 juv.,
Marilla Station, 22°58′S, 114°28′E (QM W4022); 1 ♀, 1 juv., North Western Highway,
760 mile peg, near Marrilla Station Turnoff, 23°05′S, 114°32′E (WAM 70/163, 70/164);
1 ♀, Yannarie River, 23°15′S, 115°12′E (WAM71/1717); 1 ♀, 3 juv., Yannarie River,
near Barradale, 22°50′S, 114°57′E (QM W4023).
Other material examined: Forty-five males, ten females, and six juveniles from 25
records (Appendix 3).
Diagnosis: Males and females can be easily distinguished from all other Hoggicosa by
the presence of a black line posterior to the epigastric furrow on the ventral opisthosoma
(Fig. 4F). The male palp is most similar to that of H. bicolor but can be distinguished by
the ventral process of the tegular apophysis, which is much larger and connected to the
anterior edge (Fig. 6B vs. 6A).
Description: Male: Based on WAM T65133, Woodleigh Station, 26°11′45′S,
114°25′24′E, WA. Dorsal shield of prosoma orange-brown, darker in eye quadrangle,
with a faint radial pattern; covered with black and white setae. Sternum pale orange and
labium brown with scattered white setae. Chelicerae dark brown with white setae. Legs
orange-brown, with tibia, metatarsus, and tarsus somewhat darker, especially legs I and
42
II. Opisthosoma dorsally cream with two small black patches on anterior half. Cover of
white setae with longer black setae scattered. Opisthosoma laterally cream. Venter
cream with characteristic black stripe below epigastric furrow, covered in white setae
(Fig. 4F). Terminal apophysis of pedipalp large, strongly curved apically (Fig. 21A).
Pars pendula transparent and connected to embolus near embolus base (Fig. 21B).
Subterminal apophysis large, easily visible next to the terminal apophysis. Tegular
apophysis with angular ventral process located apically with straight ridge to the apical
point (Fig. 6B).
Female: Based on WAM T47612, Shothole Canyon, Cape Range National Park,
22°02′41′S, 114°20′14′E, WA. Dorsal shield of prosoma orange, black around eye
quadrangle, no radial pattern with cover of white-grey setae. Sternum, labium, and
chelicerae as male. Legs yellowish-orange, with patella, tibia, metatarsus, and tarsus
somewhat more orange. Opisthosoma entirely cream with white setae, except for
characteristic bar of black setae to posterior of epigastric furrow (Fig. 4F). Epigyne with
anterior pockets not much greater in width than posterior transverse part (Fig. 21C).
Internal epigyne with spermatheca base as long as wide and nearly as wide as anterior
pockets (Fig. 21D).
Variation: McKay (1975) described the males of H. snelli from Barrow Island, off the
north-west coast of Western Australia. As there appear to be slight differences between
the tegular apophysis of mainland and island specimens (Fig. 6B vs. 6C), both
variations are figured here. In addition, the palp of a male found in the Kimberley
region of Western Australia also shows variation in the tegular apophysis (Fig. 6D) and
palea (Fig. 21E). These specimens are similar in all other morphological aspects,
including the characteristic epigastric stripe, and we consider them conspecific. A
female from Munda Station was found to have an enlarged epigastric stripe (Fig. 4G).
Measurements: ♂ WAM T65133 (♀ WAM T47612): TL, 19.9 (17.8); PL, 10.5 (10.0);
PW, 7.5 (6.6). Eyes: AME, 0.54 (0.50); ALE, 0.31 (0.27); PME, 1.35 (1.18); PLE, 1.23
(1.09). Sternum (length/width): 5.1/3.8 (4.3/3.1). Labium (length/width): 1.6/1.3
(1.6/1.4). OL, 9.4 (7.8); OW, 5.4 (5.0). Legs, lengths of segments (femur + patella/tibia
+ metatarsus + tarsus = total length): pedipalp, 5.2 + 5.6 + – + 3.8 = 14.6; I, 9.4 + 11.0 +
8.2 + 4.4 = 33.0; II, 8.8 + 10.4 + 8.1 + 4.1 = 31.4; III, 7.6 + 9.0 + 7.9 + 4.2 = 28.7; IV,
10.0 + 11.9 + 10.1 + 4.4 = 36.4 (pedipalp, 4.3 + 4.3 + – + 2.8 = 11.4; I, 7.3 + 8.8 + 5.3 +
43
3.1 = 24.5; II, 6.6 + 8.6 + 5.4 + 2.8 = 23.4; III, 6.0 + 7.4 + 5.7 + 2.8 = 21.9; IV, 7.4 +
10.0 + 7.7 + 3.4 = 28.5).
♂ (♀) (range, mean ± SD): TL, 12.5–21.6, 18.0 ± 1.8; PL, 7.5–11.3, 9.9 ± 0.8; PW, 5.5–
8.1, 7.0 ± 0.7; N = 25 (TL, 18.6–24.1, 20.7 ± 1.7; PL, 10.0–11.6, 10.8 ± 0.6; PW, 6.7–
8.5, 7.6 ± 0.6; N = 9).
Natural history: Hoggicosa snelli have been found on bare gravel slopes or red clayey
loams with one record from a red dune. Specimens have been recorded in association
with Mulga (Acacia aneura), Snakewood (A. xiphophylla), and Spinifex (Triodia)
vegetation or bare areas. Mature females were found all year round, but are particularly
common from January to April. Males have been collected from August to February.
Hoggicosa snelli differs in its burrowing behaviour in that it uses a pebble or debris to
block its burrow entrance. McKay (1975) described that each morning the pebble is
replaced in the same position, which leads to the build up of a visible circular ring of
silk on the pebble.
Distribution: Northern Western Australia (Fig. 22).
44
HOGGICOSA STORRI (MCKAY, 1973) COMB. NOV.
(FIGS 1D, E, 5G, H, 23A–D, 25)
Lycosa storri McKay, 1973: 389–394, figs 1H–J, 3A–E; Main, 1976: 48, 141, 149, 231,
pl. B8; Brignoli, 1983: 450; McKay, 1985: 83.
Types: Holotype: ♀ from Western Australia: Yellowdine, 38 miles south, 31°51′S,
119°39′E, 6.xi.1970, W. H. Butler (WAM 70/240). Epigynum missing.
Paratypes: Western Australia: 1 juv., Albion Downs, 24 miles south-west, 27°17′S,
120°01′E (WAM 71/875); 1 juv., Billeranga, 29°19′S, 115°52′E (WAM 68/501); 1 juv.,
Grants Patch, Broad Arrow near Kalgoorlie, 30°27′S, 121°20′E (WAM 70/22); 2 juv.,
Burnabinmah Station, 28°47′S, 117°22′E (WAM 68/823, 68/828); 1 ♀, Clinker Hill,
30°53′S, 121°46′E (WAM 68/504); 1 ♀, Corrigin, 32°20′S, 118°52′E (WAM 71/874); 1
juv., Dulbelling, 32°02′S, 117°15′E (WAM 68/825); 2 juv., Hyden, The Humps,
32°19′S, 118°58′E (WAM 69/884, 71/456); 1 ♀, Karonie, 4 miles northeast, 30°56′S,
122°35′E (WAM 68/505); 1 juv., Kellerberrin, 31°38′S, 117°43′E (WAM 38/1298); 1
♀, 1 juv., Koorda, 30°50′S, 117°29′E (WAM 70/245, 39/2169); 2 ♀, 2 juv., Lake
Moore, near south end, 30°12′S, 117°25′E (WAM 71/174, 71/175-6, 71/197); 1 juv.,
Leonara, 15 miles east, 28°53′S, 121°35′E (WAM 70/206); 1 ♀, Marloo Station,
28°19′S, 116°11′E (WAM 69/835); 1 ♀, 1 juv., Merredin, 31°29′S, 118°16′E (WAM
69/888, 68/502); 1 juv., Moorine Rock, 31°18′S, 119°08′E (WAM 68/500); 1 ♀, 2 juv.,
Mt Gibson, 29°36′S, 117°24′E (WAM 71/877, 71/876); 1 juv., Mullewa, 1.5 miles east,
28°32′S, 115°31′E (WAM 68/829); 1 ♂, 2 ♀ Muralgarra, 28°32′S, 117°03′E (WAM
39/2564, 39/2565, 39/2566); 1 ♀, 31 juv., Narembeen Camp Site, 32°04′S, 118°23′E
(WAM 69/962-94); 1 ♀, Noongar, 31°20′S, 118°58′E (WAM 39/2472); 1 juv., Nukarni,
31°18′S, 118°12′E (WAM 47/963); 5 juv., Paynes Find, 29°15′S, 117°41′E (WAM
70/53, 70/202-3, 70/54, 69/454); 1 juv., Quairading, 32°01′S, 117°24′E (WAM 69/885);
1 juv., Randells, 13 miles west on railway, 31°00′S, 121°59′E (WAM 68/827); 1 juv.,
Walebing, 3 miles north, 30°39′S, 116°13′E (WAM 68/498); 1 juv., Walyahmoning
Rock, 1 mile south-west, 30°38′S, 118°45′E (WAM 70/57, published as WAM 70/51 in
McKay (1973); 1 ♀, Warburton Ranges, 26°06′S, 126°39′E (WAM 71/878); 1 juv.,
Wialki at Arnolds Water Reserve, 30°25′S, 118°03′E (WAM 68/826); 1 ♀, Williams,
33°02′S, 116°53′E (WAM 68/824); 1 juv., Ravensthorpe, 33°35′S, 120°03′E (WAM
69/886); 1 ♀, Cocklebiddy, 70 miles north, 32°03′S, 124°54′E (WAM 69/890).
45
Other material examined: Ninety-four males, 23 females, and 29 juveniles from 152
records (Appendix 3).
Diagnosis: Females and immature males can be readily distinguished from all other
Hoggicosa species by the distinct leg coloration and abdominal pattern (Fig. 1D). This
pattern consists of light femora, tarsi, and metatarsi, with black patellae and tibiae, with
a pale stripe along either side of the abdomen from the spinnerets. The male palp is
most similar to that of H. brennani, but can be distinguished by the shape of the ventral
process on the tegular apophysis. In H. storri the ventral process lacks the flange found
in H. brennani (Fig. 5C, D vs. 5G) and is located closer to the apical tip.
Description: Male: Based on male from type locality, WAM T53406, Yellowdine,
31°51′S, 119°39′E, WA. Dorsal shield of prosoma orange-brown, darker in eye
quadrangle, covered with white setae. Sternum and labium brown with scattered black
setae. Chelicerae dark brown with white setae. Legs all greyish-brown, except for paler
ventral femur. Projections on apical end of coxae I (see remarks). Opisthosoma all
greyblack with black setae except for creamish-yellow streak running from spinnerets
two-thirds along either side. Terminal apophysis of pedipalp large, strongly curved
apically (Fig. 23A). Pars pendula transparent and connected just below embolus tip
(Fig. 23B). Subterminal apophysis large and easily visible next to terminal apophysis.
Tegular apophysis with angular ventral process located centrally or near apex. Curved
ridge connecting ventral process and apical point (Fig. 5G).
Female: Based on WAM 68/503, Wubin, 30°07′S, 116°38′E, WA. Dorsal shield of
prosoma orange-brown with cover of white setae. Sternum, labium, and chelicerae as
male. Legs; femur, metatarsus, and tarsus yellowish-cream with tibia and patella black
(Fig. 1D). Small projections on apical end of coxae I (see remarks). Opisthosoma black,
with pale side streak as male. Epigyne with small anterior pockets, much greater in
width than posterior transverse part (Fig. 23C). Internal epigyne with strongly
sclerotised anterior pockets and head of spermatheca elongate (Fig. 23D).
46
Variation: In some males a small black longitudinal stripe is present at the anterior end
of the dorsal abdomen. The length of the ridge between the ventral process and apical
point of the tegular apophysis can vary (Fig. 5G vs. 5H). Some females have a faint pale
longitudinal stripe at the anterior end of the dorsal abdomen.
Remarks: The epigynum of the holotype is missing and so a representative female is
used here for redescription. Several of the male specimens, including those from the
type locality, were found to have prominent protuberances extending from the tip of
coxae I and II near the sternum. Following further examination, some females were
found to have similar, but reduced, bulges. No other morphological differences were
found between those with and without coxal points and as the distributions overlap we
currently consider them conspecific.
Measurements: ♂ WAM T53406 (♀ WAM 68/503): TL, 17.6 (17.0); PL, 9.7 (9.1); PW,
7.3 (7.3). Eyes: AME, 0.45 (0.50); ALE, 0.23 (0.32); PME, 1.09 (1.18); PLE, 0.73
(1.04). Sternum (length/width): 3.6/3.4 (4.0/3.3). Labium (length/width): 1.0/1.0
(1.4/1.4). OL, 7.8 (7.8); OW, 5.7 (5.8). Legs, lengths of segments (femur + patella/tibia
+ metatarsus + tarsus = total length): pedipalp, 4.3 + 4.0 + – + 3.4 = 11.7; I, 8.6 + 9.8 +
8.6 + 5.0 = 32.0; II, 8.3 + 9.6 + 8.8 + 4.4 = 31.1; III, 7.1 + 7.8 + 7.8 + 4.3 = 27.0; IV,
9.3 + 10.4 + 10.0 + 4.7 = 34.4 (pedipalp, 4.0 + 4.3 + – + 2.8 = 11.1; I, 7.4 + 9.0 + 6.0 +
3.1 = 25.5; II, 7.1 + 8.6 + 6.0 + 3.1 = 24.8; III, 6.4 + 7.4 + 6.4 + 3.3 = 23.5; IV, 7.8 +
9.3 + 8.6 + 3.6 = 29.3).
♂ (♀) (range, mean ± SD): TL, 12.9–20.1, 17.2 ± 1.6; PL, 7.1–10.3, 9.4 ± 0.6; PW, 6.4–
8.1, 7.2 ± 0.4; N = 35 (TL, 17.9–23.0, 19.9 ± 1.7; PL, 8.7–10.3, 9.6 ± 0.5; PW, 6.6–8.1,
7.3 ± 0.5; N = 14).
47
Natural history: Hoggicosa storri have been collected from clay, gritty loam, rocky,
red, and yellow soils. Specimens have been recorded in association with vegetation of
Mallee (Eucalyptus) and Mulga (Acacia aneura) and woodlands of Wandoo
(Eucalyptus wandoo), Salmon Gum (E. salmonophloia), York Gum (E. loxophleba),
Gimlet (E. salubris), and E. striaticalyx, as well as open shrubland. Adult females have
been collected all year round, whereas adult males have been predominately collected
from October to March. Hoggicosa storri excavates burrows without doors.
Distribution: Western Australia (Fig. 25).
48
HOGGICOSA WOLODYMYRI SP. NOV.
(FIGS 4H, I, 5F, 7D, 24A–D, 25)
Types: Holotype. ♂ from South Australia: Taylorville Station, 34°06′S, 139°58′E, 2–
4.x.1999, Strathalbyn Field Nats. (SAM NN16408).
Paratype. ♀ with same data as holotype. (SAM NN16409).
Other material examined: One-hundred and twenty-three males, 27 females, and four
juveniles from 87 records (Appendix 3).
Etymology: The specific epithet is a patronym in honour of the senior author‟s late
grandfather Wolodymyr Kowal, who after immigrating to Australia fell in love with the
outback landscapes where this species is found.
Diagnosis: Hoggicosa wolodymyri can be distinguished from all other Hoggicosa by its
small body size and orange-yellow colour. The male palp is most similar to that of H.
bicolor, but can be distinguished by the tegular apophysis, which has a ridge between
the ventral process and the tip much longer than that of H. bicolor (compare Fig. 5F vs.
6A). The female epigyne is similar in shape to H. bicolor but is smaller in size and
females can be easily distinguished on body colour.
Description: Male: Based on holotype. Dorsal shield of prosoma orange-brown, darker
in eye quadrangle, with faint radial pattern; covered with black setae. Sternum orangeyellow, labium dark orange-brown, both with scattered black setae. Chelicerae dark
brown with white setae. Legs orange-yellow. Opisthosoma dorsally orange-yellow with
mottled black and grey patches; grey-black setae. Dark orange median longitudinal
band at anterior end (Fig. 4H). Opisthosoma laterally and ventrally pale orange-yellow,
some black dots on venter. Terminal apophysis of pedipalp large and strongly curved
apically (Fig. 24A, B). Pars pendula transparent and joins embolus at embolus tip (Figs
7D, 24B). Subterminal apophysis present, but located under terminal apophysis and
difficult to see (Fig. 7D). Tegular apophysis with small process, pointed ventrally and
located away from apical point. Straight ridge between ventral process and apical point
(Fig. 5F).
49
Female: Based on paratype. Dorsal shield of prosoma pale orange, darker in eye
quadrangle, with faint radial pattern; covered with black setae. Sternum, labium,
chelicerae, and legs as male. Opisthosoma dorsally and laterally as male (Fig. 4I).
Venter without black patches. Epigyne with small and simple anterior pockets, only
slightly greater in width than posterior transverse part (Fig. 24C). Internal epigyne with
thin sclerotized channels of median septum clearly visible as well as thin and elongate
spermatheca stalks (Fig. 24D).
Variation: Male specimens from WA are slightly smaller and pale yellow in colour,
with less colouration (dark patches) on the abdomen. Some males lack black patches on
the ventral opisthosoma.
Measurements: ♂ holotype (♀ paratype): TL, 15.5 (14.2); PL, 8.0 (6.8); PW, 6.0 (5.4).
Eyes: AME, 0.38 (0.38); ALE, 0.23 (0.27); PME, 0.81 (0.88); PLE, 0.77 (0.73).
Sternum (length/width): 3.4/2.7 (2.9/2.5). Labium (length/width): 0.9/1.1 (1.0/1.1). OL,
7.5 (7.4); OW, 4.6 (5.0). Legs, lengths of segments (femur + patella/tibia + metatarsus +
tarsus = total length): pedipalp, 4.1 + 3.8 + – + – = 7.9; I, 9.4 + 10.0 + 8.5 + 5.0 = 32.9;
II, 8.8 + 10.0 + 8.2 + 4.6 = 31.6; III, 8.2 + 9.4 + 8.8 + 4.6 = 31.0; IV, 10.2 + 11.2 + 11.5
+ 5.4 = 38.3 (pedipalp, 3.1 + 3.4 + – + 2.6 = 9.1; I, 6.6 + 7.5 + 4.8 + 3.0 = 21.9; II, 6.7 +
7.1 + 4.8 + 2.8 = 21.4; III, 5.9 + 6.5 + 5.0 + 2.8 = 20.2; IV, 7.4 + 8.4 + 6.9 + 3.1 =
25.8).
♂ (♀) (range, mean ± SD): TL, 11.6–14.8, 13.3 ± 1.0; PL, 6.4–7.8, 6.9 ± 0.4; PW, 5.0–
6.0, 5.5 ± 0.3; N = 14 (TL, 14.4–16.9, 15.5 ± 1.0; PL, 6.9–8.5, 7.4 ± 0.7; PW, 5.3–6.4,
5.8 ± 0.5; N = 6).
Natural history: Specimens have been collected from sand dunes, sand plains, interdune
swales, and clayey soils associated with open Mallee (Eucalyptus) with mixed
understorey or Mulga (Acacia aneura) and Spinifex (Triodia) vegetation. Males and
females have been collected predominately from September to December, although a
couple of males have been found in March and June. Records indicate H. wolodymyri
constructs a doorless burrow.
50
Distribution: New South Wales, Northern Territory, South Australia, and Western
Australia (Fig. 25).
ACKNOWLEDGEMENTS
We thank the following people at the WAM for useful comments and discussions: Mark
Harvey, Julianne Waldock, Jung-Sun Yoo (now National Institute for Biological
Resources, South Korea), and Karen Edward (now University of Western Australia).
We extend thanks to Erich Volschenk for assistance with phylogenetic analyses and
Mike Rix for help with SEMs. We greatly appreciate loans of material from David Hirst
(SAM), Graham Milledge (AM), and Robert Raven and Owen Seaman (QM).
Specimens were kindly sent to us by Maggie Hodge (Geolycosa) and Paolo Tongiorgi
(Lycosa tarantula), both initially for the study by Murphy et al., 2006. Scanning
electron micrographs were carried out using facilities at the Centre for Microscopy,
Characterization and Analysis, The University of Western Australia (UWA), which are
supported by University, State, and Federal Government funding. Financial support to
V. W. Framenau was initially (2002–2005) provided by an Australian Biological
Resources Study (ABRS) grant to Mark Harvey (WAM) and Andy Austin (The
University of Adelaide) for a revision of the Australian Lycosidae and later (2005–
2008) by an ABRS grant to Volker Framenau and Nikolaj Scharff (University of
Copenhagen, Denmark) for a revision of the Australian orb-weaving spiders of the
subfamily Araneinae. We thank David Hirst (Fig. 1F), Peter Hudson (Fig. 20) and Mark
Harvey (Fig. 9) for permission to use their photographs. We thank Karl Brennan
(Western Australian Department of Environment and Conservation), Bob Black
(UWA), and Barbara York Main (UWA) for comments on draft manuscripts.
51
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58
Table 1. Morphological character matrix. Character and character state descriptions in Appendix B.
Character
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19
Arctosa cinerea
0 1 0 0 2 1 0 0 1 0 0 0 1 1 1 1 0 0 Dingosa serrata
1 2 1 0 2 2 0 0 0 0 0 1 0 D. simsoni
1 2 1 0 2 2 0 0 0 0 0 1 0 Geolycosa hubbelli 1 0 1 0 1 2 1 3 0 0 1 1 1 0 0 0 G. missouriensis
1 0 1 0 0 0 1 3 0 0 1 1 1 0 0 0 ‘Grey Wolf Spider' 1 0 1 0 2 2 0 0 1 1 0 0 0 1 1 0 1 1 1
Hoggicosa alfi
1 1 2 0 2 1 0 3 1 1 1 0 1 0 1 1 0 1 0
H. bicolor
1 0 2 1 1 1 1 3 1 1 1 1 0 1 1 0 0 1 1
H. brennani
1 0 2 0 2 1 0 1 1 1 1 0 0 0 1 0 0 1 1
H. castanea
1 1 2 1 2 1 0 3 1 1 1 0 0 0 1 0 0 1 0
H. duracki
1 0 2 0 1 0 0 0 1 1 1 0 1 0 1 1 1 1 0
H. forresti
1 1 2 1 2 2 0 3 1 1 1 0 1 0 1 0 0 1 0
H. snelli
1 0 2 0 0 0 0 1 1 1 1 1 1 1 1 0 0 1 1
H. storri
1 0 2 1 0 0 0 3 1 1 1 1 1 0 1 0 0 1 1
H. wolodymyri
1 1 2 0 2 2 0 0 1 1 1 0 0 1 1 0 0 1 0
Hogna crispipes
0 1 2 0 2 1 0 0 1 0 2 0 1 1 1 0 0 1 1
H. immansueta
0 1 1 0 2 2 0 1 1 0 0 1 0 0 2 0 1 1 1
H. kuyani
0 1 2 0 2 2 0 0 1 0 2 0 1 1 1 0 0 1 1
Knoelle clara
0 1 2 0 2 2 0 1 1 2 1 0 1 2 1 1 1 1
Lycosa godeffroyi
0 2 2 0 2 2 0 3 1 0 0 1 1 0 1 0 1 1 0
L. leuckarti
0 2 2 0 2 2 0 2 1 0 0 0 1 1 1 0 1 1 0
L. praegrandis
1 1 2 0 2 2 0 1 1 0 0 0 1 ? 1 0 0 ? ?
L. tarantula
1 1 2 0 2 2 0 1 1 0 0 0 1 ? 1 0 0 ? ?
Mainosa longipes
1 1 1 0 2 1 1 3 0 1 0 1 1 0 0 1 1
Venator spenceri
0 1 1 0 2 2 0 1 1 0 0 1 0 0 2 0 1 1 1
Symbols: (-) = not applicable, (?) = missing data.
20
0
0
0
0
0
0
1
0
0
1
1
0
0
0
0
0
0
0
0
0
0
0
0
0
0
21
1
0
0
0
0
0
1
0
1
2
2
1
0
1
2
0
0
0
0
0
1
1
1
0
0
22
0
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
0
0
1
1
23
1
0
1
0
0
1
1
1
1
1
1
1
1
1
1
0
0
0
1
1
1
0
0
0
0
24
0
0
0
0
0
1
1
1
1
1
1
1
1
1
0
0
0
0
0
0
0
0
0
0
25
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
0
0
0
0
1
1
1
1
1
0
26
0
0
0
0
0
1
0
1
1
1
1
1
1
0
0
0
0
0
0
0
-
27
0
1
1
1
1
0
0
0
0
0
0
0
0
0
0
0
0
0
0
1
-
Table 2. Distribution of Hoggicosa in Australia with biogeographic regions within
states (after Thackway & Cresswell, 1997).
Species
Australian Distribution
Hoggicosa alfi sp. nov.
New South Wales, Queensland (ML), South Australia (CHC,
EYB, GAW, MDD, SSD, STP), Western Australia (AW,
CAR, COO, CR, GAS, GS, GSD, GVD, LSD, MUR, NUL,
PIL, TAN, YAL)
New South Wales, Northern Territory (DMR, MAC),
Queensland (MGD, MII, ML), South Australia (EYB, MDD,
SSD, STP), Western Australia (AW, CAR, COO, CR, FIN,
GAS, GAW, GD, GS, GVD, LSD, MAL, MUR, PIL, TAN,
YAL)
New South Wales (CP, DRP, MDD, NSS), Queensland
(BBS, NAN), South Australia (EYB, KAN, NCP, STP)
H. bicolor (Hogg, 1905)
H. brennani sp. nov.
H. castanea (Hogg, 1905)
H. duracki (McKay, 1975)
New South Wales (BHC, CP), Northern Territory (MAC),
Queensland (ML), South Australia (CHC, CR, EYB, FLB,
GAW, MDD, SSD, STP), Victoria (VVP), Western Australia
(AW, CAR, COO, ESP, GAS, GS, GSD, GVD, MAL,
MUR, NSS, NUL, PIL, SWA, WAR, YAL)
Western Australia (PIL, VB)
H. forresti (McKay, 1973)
Western Australia (AW, COO, GAS, GVD, HAM, MAL,
MUR, NUL, SWA), South Australia (EYB, FLB, MDD)
H. natashae sp. nov. *
New South Wales (BHC), Queensland (CHC), South
Australia (GAW, SSD)
H. storri (McKay, 1973)
Western Australia (AW, COO, CR, ESP, GAS, GS, JF, LSD,
MAL, MUR, NUL, SWA, YAL)
H. snelli (McKay, 1975)
Northern Western Australia (CAR, GAS, GSD, NK, PIL,
TAN)
H. wolodymyri sp. nov.
New South Wales (CP), Northern Territory (GSD), South
Australia (CR, EYB, FIN, FLB, GAW, MDD, NUL, RIV,
STP), Western Australia (GVD, MUR)
Abbreviations of biogeographic regions: AW = Avon Wheatbelt, BBS = Brigalow Belt South, BHC =
Broken Hill Complex, CAR = Carnarvon, CHC = Channel Country, COO = Coolgardie, CP = Cobar
Peneplain, CR = Central Ranges, DMR = Davenport Murchison Ranges, DRP = Darling Riverine Plains,
ESP = Esperance Plains, EYB = Eyre Yorke Block, FIN = Finke, FLB = Flinders Lofty Block, GAS =
Gascoyne, GAW = Gawler, GD = Gibson Desert, GS = Geraldton Sandplains, GSD = Great Sandy
Desert, GVD = Great Victoria Desert, HAM = Hampton, JF = Jarrah Forest, KAN = Kanmantoo, LSD =
Little Sandy Desert, MAC = MacDonnell Ranges, MAL = Mallee, MDD = Murray Darling Depression,
MGD = Mitchell Grass Downs, MII = Mount Isa Inlier, ML = Mulga Lands, MUR = Murchison, NAN =
Nandewar, NCP = Naracoorte Coastal Plain, NK = Northern Kimberley, NSS = New South Wales South
Western Slopes, NUL = Nullarbor, PIL = Pilbara, RIV = Riverina, SSD = Simpson Strzelecki Dunefields,
STP = Stony Plains, SWA = Swan Coastal Plain, TAN = Tanami, VB = Victoria Bonaparte, VVC =
Victorian Volcanic Plains, WAR = Warren, YAL = Yalgoo. (Interim Biogeographic Regionalisation for
Australia, version 6.1, after Thackway & Cresswell, 1997). * = only females known.
59
Figure 1. Hoggicosa species, habitus photos (A–H) and male diagnostic character (I).
A, Hoggicosa bicolor (Hogg) penultimate ♂ from Western Australia (WA), not
registered. B, H. bicolor (Hogg) adult ♂ from Lorna Glen Station, WA, WAM T70329.
C, Hoggicosa forresti (McKay, 1973) adult ♂ from Lorna Glen Station, WA, WAM
T65610. D, Hoggicosa storri (McKay) penultimate ♂ from WA, not registered. E, H.
storri (McKay) adult ♂ from Lorna Glen Station, WA, WAM T70277. F, Hoggicosa
natashae sp. nov. holotype ♀ from Lake Gilles, SA, SAM NN14785, Photo courtesy of
D. Hirst. G, Hoggicosa alfi sp. nov. ♂ from type locality, Lorna Glen Station, WA, not
registered. H, H. alfi sp. nov. ♀ from type locality, WAM T70334. I, Hoggicosa
castanea (Hogg) lateral view of male cymbium tip with diagnostic macrosetae bent
dorsally, from Gluepot Station, SA, SAM NN19314. Scale bars = 5 mm.
60
Figure 2. Strict consensus tree showing the relationships amongst Hoggicosa species
and other Lycosinae (length = 104, consistency index = 35, retention index = 53).
Characters are indicated by squares: character number above and character state below
square with shaded squares for nonhomoplasious characters. Bremer support and
relative Bremer support (0–100) values for each branch are indicated. Inset of colour
dimorphism (character 4, bold) under fast optimization (ACCTRAN) and slow
optimization (DELTRAN).
61
Figure 3. Hoggicosa castanea (Hogg) carapace. A, lateral view. B, frontal view. Scale
bars = 1 mm.
62
Figure 4. Hoggicosa species, abdomen (A–G) and habitus (H–I). A–C, ♀ Hoggicosa
castanea (Hogg). A, dorsal; B, ventral, from Fisherman Point, Lincoln National Park,
South Australia (SA), SAM NN15185; C, dorsal, from north of Lake Goorly, Western
Australia (WA), WAM T47784. D–E, Hoggicosa brennani sp. nov. ♂ holotype from
Taylorville Station, SA, SAM NN17017. D, dorsal; E, ventral. F–G, Hoggicosa snelli
(McKay), ventral. ♂ from Kennedy Range National Park, WA, WAM T65149. G, ♀
from Munda Station, WA, WAM T53870. H–I, Hoggicosa wolodymyri sp. nov. from
Taylorville Station, SA. H, ♂ holotype, SAM NN16408. I, ♀ paratype, SAM NN16409.
Scale bars = 5 mm.
63
Figure 5. ♂ Hoggicosa species, male palp, tegular apophyses. A–B, Hoggicosa
castanea (Hogg). A, north of Bower, South Australia (SA), WAM T64050; B, palpal
variation from east of Mount Barren, Western Australia (WA), WAM T53507. C–D,
Hoggicosa brennani sp. nov. holotype from Taylorville Station, SA, SAM NN17017;
D, tegular apophysis ventral spur enlarged. E, Hoggicosa forresti (McKay) from North
Baandee Nature Reserve, WA, WAM T47762. F, Hoggicosa wolodymyri sp. nov. from
Queen Victoria Springs Nature Reserve, WA, WAM T52527. G–H, Hoggicosa storri
(McKay). G, south of the type locality Yellowdine, WA, WAM T53406; H, palpal
variation from Yuinmery, WA, WAM T62781. All scale bars = 0.2 mm except for D =
0.1 mm
64
Figure 6. ♂ Hoggicosa species, male palp, tegular apophyses. A, Hoggicosa bicolor
(Hogg) from Mt Vernon Station, Western Australia (WA), WAM T62336. B–D,
Hoggicosa snelli (McKay). B, mainland male from Woodleigh Station, WA, WAM
T65133; C, palpal variation from Barrow Island, WA, WAM T57697; D, palpal
variation from Drysdale River Station, Kimberley, WA, WAM T56397. E–F,
Hoggicosa alfi sp. nov. E, paratype from Lorna Glen Station, WA, WAM T53919; F,
palpal variation from Nanga Station, WA, WAM T65565. G–H, Hoggicosa duracki
(McKay) from Hope Downs Station, WA, WAM T65119. H, tegular apophysis ventral
spur enlarged. Scale bars = 0.2 mm.
65
Figure 7. ♂ Hoggicosa species, male palp, palea region. A, Hoggicosa castanea (Hogg)
from East Mt Barren, Western Australia (WA), WAM T53507. B, Hoggicosa duracki
(McKay) from Hope Downs Station, WA, WAM T65119. C, Hoggicosa forresti
(McKay) from Helena-Aurora Ranges, WA, WAM T47763. D, Hoggicosa wolodymyri
sp. nov. from Queen Victoria Springs Nature Reserve, WA, WAM T52527. Scale bars
= 0.1 mm. Note: twisting of terminal and subterminal apophysis is a result of scanning
electron microscopy drying process.
66
Figure 8. Hoggicosa castanea (Hogg). A–B, palp, ♂ from Gluepot Station, South
Australia (SA), SAM NN19314. A, ventral; B, palea. C–D, epigynum, ♀ from
Fisherman Point, Lincoln National Park, SA, SAM NN15185. C, ventral; D, dorsal.
Scale bars = 0.5 mm.
67
Figure 9. Hoggicosa castanea burrow from Stirling Range caravan park, Western
Australia, WAM T58378. A, door closed. B, door open. Photos courtesy of M. Harvey.
Scale bars = 10 mm.
Figure 10. Distribution records of Hoggicosa castanea (Hogg).
68
Figure 11. Hoggicosa alfi sp. nov. A–B, palp, ♂ paratype from Lorna Glen Station,
Western Australia (WA), WAM T53919. A, ventral; B, palea. C–D, epigynum, ♀
paratype, from Lorna Glen Station, WA, WAM T77406. C, ventral; D, dorsal. E,
epigynum, dorsal, ♀ variation from Nanga Station, WA, WAM T62772. Scale bars =
0.5 mm.
69
Figure 12. Distribution records of Hoggicosa alfi sp. nov.
70
Figure 13. Hoggicosa bicolor (Hogg) from Mt Vernon Station, Western Australia,
WAM T62336. A–B, ♂, palp. A, ventral; B, palea. C–D, ♀, epigynum. C, ventral; D,
dorsal. Scale bars = 0.5 mm.
71
Figure 14. Distribution records of Hoggicosa bicolor (Hogg).
72
Figure 15. Hoggicosa brennani sp. nov. from Taylorville Station, South Australia. A–
B, ♂ holotype, palp, SAM NN17017. A, ventral; B, palea. C–D, ♀ paratype, epigynum,
SAM NN17029. C, ventral; D, dorsal. Scale bars = 0.5 mm.
73
Figure 16. Hoggicosa duracki (McKay). A–D, paratypes from Argyle Downs
Homestead, Western Australia (WA), WAM 74/495-6. A–B, ♂ palp. A, ventral; B,
palea. C–D, ♀, epigynum. C, ventral; D, dorsal. E, epigynum, ventral, ♀ holotype from
Argyle Downs, WA, WAM 74/494. Scale bars = 0.5 mm.
74
Figure 17. Hoggicosa forresti (McKay) from North Baandee Nature Reserve, Western
Australia, WAM T47762. A–B, ♂, palp. A, ventral; B, palea; C–D, ♀, epigynum. C,
ventral; D, dorsal. Scale bars = 0.5 mm.
75
Figure 18. Distribution records of Hoggicosa brennani sp. nov. (black circles),
Hoggicosa duracki (McKay) (grey circles), and Hoggicosa forresti (McKay) (white
circles).
76
Figure 19. Hoggicosa natashae sp. nov. A–B, epigynum, ♀ holotype from Lake
Gilles, South Australia (SA), SAM NN14785. A, ventral; B, dorsal. C–D, epigynum
variation, ♀ from Cooper Creek, SA, SAM NN020. C, ventral; D, dorsal.
Figure 20. Hoggicosa natashae sp. nov. burrow entrance of holotype from Lake Gilles,
South Australia, SAM NN14785. Photo courtesy of P. Hudson. Diameter of coin = 28
mm.
77
Figure 21. Hoggicosa snelli (McKay). A–B, palp, ♂ from Woodleigh Station, Western
Australia (WA), WAM T65133. A, ventral; B, palea. C–D, epigynum, ♀ from Shothole
Canyon, Cape Range National Park, WA, WAM T47612. C, ventral; D, dorsal. E, palp,
♂ palea variation from Drysdale River Station, Kimberley, WA, WAM T56397. Scale
bars = 0.5 mm.
78
Figure 22. Distribution records of Hoggicosa natashae sp. nov. (grey circles) and
Hoggicosa snelli (McKay) (white circles).
79
Figure 23. Hoggicosa storri (McKay). A–B, palp, ♂ from Stoneville, Western
Australia (WA), WAM T47794. A, ventral; B, palea. C–D, epigynum, ♀ from Wubin,
WA, WAM 68/503. C, ventral; D, dorsal. Scale bars = 0.5 mm.
80
Figure 24. Hoggicosa wolodymyri sp. nov. from Taylorville Station, South Australia.
A–B, ♂ holotype, palp, SAM NN16408. A, ventral; B, palea. C–D, ♀ paratype,
epigynum, SAM NN16409. C, ventral; D, dorsal. Scale bars = 0.5 mm.
81
Figure 25. Distribution records of Hoggicosa storri (McKay) (white circles) and
Hoggicosa wolodymyri sp. nov. (grey circles).
82
H. wolodymyri sp. nov.
H. storri (McKay, 1973)
H. duracki (McKay, 1975)
H. forresti (McKay, 1973)
H. snelli (McKay, 1975)
H. castanea (Hogg, 1905)
H. bicolor (Hogg, 1905)
H. brennani sp. nov.
Hoggicosa alfi sp. nov.
"Grey Wolf Spider"
G. missouriensis (Banks, 1895)
Geolycosa hubbelli Wallace, 1942
D. simsoni (Simon, 1898)
Dingosa serrata (L. Koch, 1877)
Species
Arctosa cinerea (Fabricius, 1777)
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂♀
♂
♀
♂
♀
♂♀
♂♀
♂
♀
♂
♀
♂
♀
83
Location
Isar River near Wallgau, Germany
Lech River near Forchach, Austria
Yanchep, Western Australia
Inglewood, Perth, Western Australia
Yokrakine Rock, Western Australia
Boorabin, Western Australia
Archbold Biological Station, Florida, United States of America
* (Wallace, 1942)
Holmes County State Park, Mississippi, United States of America
Holmes County State Park, Mississippi, United States of America
Broken Hill, New South Wales
Runnymede Flora Reserve, Victoria
Lorna Glen Station, Western Australia
Lorna Glen Station, Western Australia
Mt Vernon Station, Western Australia
Taylorville Station, South Australia
Taylorville Station, South Australia
Gluepot Station, South Australia
Fisherman Point, Lincoln National Park, South Australia
Argyle Downs Homestead, W
North Baandee Nature Reserve, Western Australia
Woodleigh Station, Western Australia
Shothole Canyon, Cape Range National Park, Western Australia
Stoneville, Western Australia
Wubin, Western Australia
Taylorville Station, South Australia
Taylorville Station, South Australia
WAM
WAM
WAM
WAM
WAM
WAM
WAM
SAM
SAM
SAM
SAM
WAM
WAM
WAM
WAM
WAM
WAM
SAM
SAM
Deposition
WAM
WAM
WAM
WAM
WAM
WAM
WAM
Species used for phylogenetic analysis with specimen location, place deposited and registration number.
* = characters scored from secondary sources.
APPENDIX 1
T56118
T56117
T62654
T56072
T53919
T77406
T62336
NN17017
NN17029
NN19314
NN15185
74/495-7
T47762
T65133
T47612
T47794
68/503
NN16408
NN16409
Registration
T56247
T56246
T58321
T68496
71.1422
T51253
T56572
V. spenceri Hogg, 1900
Mainosa longipes (L. Koch, 1878)
L. tarantula (Linnaeus, 1758)
L. praegrandis C. L. Koch, 1836
L. leuckarti (Thorell, 1870)
Lycosa godeffroyi L. Koch, 1865
Hogna immansueta (Simon, 1909)
H. kuyani Framenau, Gotch & Austin,
2007
Knoelle clara (L. Koch, 1877)
Hogna crispipes L. Koch, 1877
♂
♀
♂♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
♂
♀
84
Deepdale, Western Australia
South Lake, Western Australia
Red Bluff, Red Bluff Caravan Park, Western Australia
`Sieda`, East of Grass Patch,Western Australia
Laverton, Western Australia
Drysdale River Station, Western Australia
Kapalga, Northern Territory
Maylands, Perth, Western Australia
Eneabba, Western Australia
Burekup, Western Australia
Gardner Reserve Road, Western Australia
* (Zyuzin & Logunov, 2000)
Amissa, Greece
* (Álvares, 2006)
San Rossore, Pisa, Italy
Francois Peron National Park, Western Australia
Nerren Nerren Station, Western Australia
Kanyaka Creek, Wilson, South Australia
Adelaide, South Australia
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
WAM
T56055
T48038
94/1940
T51488
T64071
90/566
T65662
T75884
T58331
T53586
T55296
T56241
T58372
T65006
T65005
T53852
T53675
APPENDIX 2
Character descriptions
1. Carapace, profile in lateral view: cephalic region not elevated, profile horizontal
(0) (Framenau et al., 2006: fig. 23); cephalic region elevated, profile strongly sloping
away from eyes (1) (Fig. 3A).
2. Carapace, radial colour pattern, female: absent (0) (Fig. 1A); weak or indistinct
(1) (Fig. 1H); strong pattern of black and white lines „Union-Jack-colour pattern‟ (2).
The „Union-Jackcolour pattern‟ is seen in Lycosa leuckartii (Main, 1976: figs 26, 27).
3. Anterior eye row, curvature in frontal view: straight (0); slightly procurved (1)
(Framenau, 2006a: fig. 4); strongly procurved (2) (Fig. 3B). Eye row curvature is
determined by drawing a line through the middle of the anterior median eyes. If the
line passed through the middle of the anterior lateral eyes it was scored as straight. If
the line passed through the upper half of the anterior lateral eyes it was considered
slightly procurved and strongly procurved if the line did not pass through the anterior
lateral eyes.
4. Leg colouration, alternating dark and light segments, in females but not adult
males: absent (0) (Fig. 1G, H); present (1) (Fig. 1A, B).
5. Abdomen, dorsal colour, female: unicoloured (0) (Fig. 1D); dual coloured (1) (Fig.
1F); multicoloured (2) (Fig. 4A).
6. Abdomen, cardiac (heart) or chevron mark, female: absent (0) (Fig. 1D); present,
light colour compared to surrounding (1) (Fig. 1A); present, dark colour compared to
surrounding (2) (Fig. 1C). If multiple colours surrounded the cardiac mark, the
predominate colour was used.
7. Abdomen, lateral colour pattern, female: pale (0) (fig. 4F); black (1) (Framenau,
2006a, fig. 1).
8. Abdomen, ventral colour pattern, female: uniform light (0); light with dark pattern
(1) (Fig. 1E, F); dark with light pattern (2); uniform dark (3) (Fig. 4B). If the black
pattern reached all the way to the spinnerets and covered most of the ventral abdomen
it was considered uniform dark.
9. Cymbium tip, macrosetae: absent (0) (Framenau, 2006a: fig. 6); present (1) (Fig.
1I).
10. Cymbium tip, number of macrosetae: One to ten macrosetae (0) (Framenau et al.,
2006: fig. 20); 10–30 macrosetae (1) (Fig. 1I); >
fig. 2).
85
11. Cymbium tip, macrosetae direction: straight (0) (Álvares, 2006: fig. 13); curved
dorsally (1) (Framenau et al., 2006: fig. 21); curved ventrally (2) (Fig. 1I).
12. Tegular apophysis, position of ventral process: distance between ventral process
tip and tegular apophysis tip greater than half distance of tegular apophysis (0) (Fig.
5A); distance between ventral process tip and tegular apophysis tip less than half
distance of tegular apophysis (1) (Fig. 6A). The distance of the tegular apophysis was
taken as the length of the line from the apical point through the ventral process to the
edge of the strongly sclerotized tegular apophysis (Fig. 5A).
13. Tegular apophysis, connection of ventral process to apical edge: absent (0) (Fig.
5A); present (1) (Fig. 6B). The apical edge of the tegular apophysis is defined in
relation to the palp.
14. Tegular apophysis, connection of ventral process to apical point, ridge shape:
curved (0) (Fig. 5A); straight (1) (Fig. 6A).
15. Tegular apophysis, number of ventral processes: none (0) (Framenau & Baehr,
2007: fig. 2C); one (1) (Fig. 1A); two (2) (Framenau, 2006b: fig. 6).
16. Terminal apophysis, direction: curved apically (0) (Fig. 8B); straight, pointing
retrolaterally (1) (Fig. 11B).
17. Terminal apophysis, shape of tip: pointed, sharp tip (0) (Fig. 8B); truncated, broad
tip (1) (Fig. 16B).
18. Subterminal apophysis: absent (0) (Framenau & Baehr, 2007: fig. 6A); present (1)
(Fig. 11B).
19. Subterminal apophysis, visibility in ventral view: Beneath terminal apophysis
and difficult to see (0) (Figs 7A, 8B); Next to terminal apophysis and easily visible (1)
(Fig. 13B).
20. Pars pendula, thickness: thin, transparent (0) (Fig. 13B); thick and obvious,
opaque (1) (Fig. 8B).
21. Pars pendula, connection to embolus: Joins well below embolus tip (0) (Fig.
13B); Joins just below embolus tip (1) (Fig. 11B); along whole embolus (2) (Fig. 7A,
B). If the pars pendula was only found at the base of the embolus (Fig. 21B) or the
length of embolus without the pars pendula was close to the length of the terminal
apophysis (Fig. 13B), it was scored as 0. If the pars pendula joined at the embolus tip
it was scored as 2 and those that had a pars pendula intermediate to these cases were
scored as 1.
22. Epigyne, inverted T-shaped median septum: absent (0) (Zyuzin & Logunov,
2000: fig. 2); present (1) (Fig. 8C).
86
23. Epigyne, median septum, widening anteriorly: absent (0) (Zyuzin & Logunov,
2000: fig. 2); present (1) (Fig. 8C).
24. Epigyne, distance between anterior pockets: equal or shorter than width of
posterior transverse part (0) (Framenau, 2006b: fig. 9); greater than width of posterior
transverse part (1) (Fig. 8C).
25. Burrow, female and immatures: absent (0); present (1).
26. Burrow, trapdoor: absent (0) (Framenau, 2006a: fig. 2); present (door or rock) (1)
(Fig. 9A, B).
27. Burrow, palisade: absent (0) (Fig. 9B); present (1) (Framenau, 2006a: fig. 2).
87
APPENDIX 3
List of material examined by species then state.
Hoggicosa castanea
NSW: 2 ♂, Birdwood Station, Lower Murray-Darling Region, 33º29'54''S, 142º44'30''E (AM KS71096);
1 ♀, Broken Hill, 31º57'S, 141º27'E (SAM NN17226); 1 ♀, Broken Hill, Springs Creek, Barrier Hwy,
120km E, 31º43'S, 142º41'E (SAM NN17227); 1 ♂, Glen Tilt Station, Lower Murray-Darling region,
31º41'59''S, 143º35'32''E (AM KS66996); Gundabooka National Park, Yanda Creek, near Ben Lomond,,
30º31'145''S, 145º48'E (SAM NN18280); 1 ♀, Gundabooka National Park, Yanda Creek, near Ben
Lomond,, 30º31'S, 145º48'E (SAM NN18283); 10 ♂, 1 ♀, no exact locality (AM KS91620, KS91594,
KS92508, KS91602, KS91605); 1 ♂, Nymagee, 6 mi S, 32º04'S, 146º19'E (AM KS5728); 45 ♂, Orange
Grove Station, Lower Murray-Darling region, 33º36'15''S, 143º34'39''E (AM KS66841); 1 ♂, Prill Park
Station, Lower Murray-Darling region, 34º40'20''S, 142º41'33''E (AM KS66966); 1 ♀, Rabbit Camp (no
exact location), no exact locality (WAM 69/36); 1 ♂, 2 ♀, Round Hill, Euabalong, 32º57'S, 146º9'E (AM
KS86505, KS82567, KS69276); 3 ♂, Round Plain Station, Lower Murray-Darling region, 33º43'18''S,
143º37'40''E (AM KS66838); 1 ♂, Woolcunda Station, Lower Murray-Darling region, 32º51'25''S,
141º21'05''E (AM KS67437); NT: Hermannsburg, 23º56'S, 132º46'E (SAM NN16555); Qld: 1 ♂,
`Gumbardo`, 26º04'38''S, 144º45'20''E (QM S63293); 1 ♀, Ambathala, 1mile E of No 3 bore on old road,
25º58'S, 145º20'E (QM S70660); SA: 1 ♂, no exact locality (QM S22456); 1 ♀, 31º53'45''S, 137º32'43''E
(SAM NN13782); 1 ♀, ALGE campsite, no exact locality (SAM no reg.); 1 ♀, Amyton Cementary,
32º37'S, 138º20'E (SAM NN14720); 1 ♀, Bairds Bay, 4.1km ESE, 33º9'30''S, 134º24'22''E (SAM no
reg.); 1 ♀, Billeroo Well, S of Lake Frome, 31º12'S, 139º55'E (SAM NN13776); 3 ♂, Bower, N of,
34º00'31''S, 139º21'24''E (WAM T64050); 1 ♀, Brookfield Conservation Park, 34º20'S, 139º31'E (SAM
NN13806); 1 ♀, Cadell, 34º02'S, 139º46'E (SAM NN13808); 1 ♀, Calperum Station, Frogamerry,
33º55'04''S, 140º24'42''E (SAM NN13807); 1 ♀, Chambers Gorge turnoff, 8km W, 30º58'S, 139º16'E
(SAM NN13759); 2 ♀, Claire, N of, 33º50'S, 138º36'E (WAM 69/802, 69/800); 1 ♀, Coffin Bay,
34º40'S, 135º19'E (SAM NN15186); 1 ♀, Coffin Bay National Park, Yangie Bay camping area, 34º38'S,
135º22'E (SAM NN15188); 1 ♀, Dalhousie Springs, 1km N of spring, 26º28'S, 135º29'E (NMV K8162);
1 ♂, Danggali Conservation Park, Tomahawk Dam, 3km N, 33º19'39''S, 140º42'50''E (SAM NN17074); 1
♀, Emu-Cook Junction, 26mi S, no exact locality (WAM 69/807); 1 ♀, Erudina Woolshed, near, 31º29'S,
139º23'E (SAM NN13802); 2 ♀, Euro Bluff, NW of Pt Augusta, 32º21'S, 139º21'E (SAM NN13781,
NN13765); 1 ♀, Eyre Peninsula, 32º32'18''S, 136º34'31''E (SAM NN13770); 2 ♂, Eyre Peninsula (no
exact location), 33º39'S, 137º11'E (SAM NN13773-4); 1 ♀, Flinders Ranges, between Hawker and
Wilpena, 31º50'S, 138º35'E (WAM 69/921); 1 ♀, Gawler Ranges, no exact locality, 32º44'S, 136º47'E
(SAM NN13764); 1 ♂, Gluepot Station, Gluepot Homestead, 11.5km W, 33º45'08''S, 139º59'51''E (SAM
NN19439); 2 ♂, Gluepot Station, Gluepot Homestead, 4.7km N, 33º43'23''S, 140º07'26''E (SAM
NN18801, NN18800); 1 ♀, Gluepot Station, Gluepot Homestead, 7.2km WNW, 33º44'29''S, 140º02'54''E
(SAM NN19498); 2 ♂, Gluepot Station, Gluepot Homestead, 7km N, 33º42'01''S, 140º07'24''E (SAM
NN18881-2); 1 ♂, Gluepot Station, Gluepot Homestead, 9.6km W-WNW, 33º44'51''S, 140º01'07''E
(SAM NN19314); 1 ♀, Inila Rock Waters, 31º47'S, 133º46'E (SAM NN16236); 1 ♀, Innamincka,
27º44'S, 140º44'E (SAM NN436); 1 ♀, Kappawanta Basin, 33º40'S, 135º22'E (SAM NN15187); 1 ♀, 1
juv., Lake Callabonna, 29º40'S, 140º01'E (WAM 71/243-4); 3 ♀, Lake Gilles, 32º43'S, 136º47'E (SAM
NN13787, NN13792, NN13791); 1 ♀, Lake Pitikanta, 28º21'S, 138º18'E (SAM NN15193); 1 ♂, Lake
Torrens to Andamooka, no exact locality (QM S21351); 1 ♀, Lincoln National Park, Fisherman Point,
34º45'S, 135º59'E (SAM NN15185); 2 ♀, Lincoln National Park, near Spalding Cave, 34º46'S, 135º58'E
(SAM NN15183-4); 1 ♀, Lucky Bay, 33º42'S, 137º02'E (SAM NN13786); 2 ♀, Middleback, 32º56'S,
137º23'E (SAM NN17004, NN16996); 1 ♀, Minnipa, Agricultural Research Centre, 3km NNW, 32º51'S,
135º9'E (SAM NN13798); 1 ♀, Mt Sturt, 3km S, 32º45'S, 135º24'E (SAM NN13761); 2 ♀, Mt Whyalla,
32º49'S, 137º26'E (SAM NN13793, NN13794); 1 ♀, Muckera Rockhole, 30º02'S, 130º03'E (SAM
NN17006); 1 ♂, 1 ♀, 1 juv., Murninnie Beach, 33º20'S, 137º25'E (SAM NN13797, NN13795); 1 ♀,
Musgrave Park, No.25 Bore, Mt. Caroline, 25miles N, 26º20'S, 130º49'E (SAM NN15243); 3 ♀, no
locality given (SAM NN021); 1 ♀, North Well, nr Kingoonya, 30º50'S, 135º18'E (SAM NN13777); 1 ♀,
Orroroo, 32º44'S, 138º36'E (SAM NN13805); 1 ♀, OTC Station, E of, N of Ceduna, 32º07'S, 133º40'E
(SAM NN13760); 1 ♂, Peake Station, Edith Spring, 4.8km NE, 28º26'10''S, 136º07'41''E (SAM
NN15781); 1 ♂, Peake Station, Four Hills Trig, 6.8km NNW, 28º27'04''S, 136º27'46''E (SAM NN15787);
1 ♂, Peake Station, Mussel WH, 1.5km NE, 28º27'12''S, 136º23'26''E (SAM NN15802); 1 ♀,
Pinkawillinie Conservation Park, 33º03'S, 135º50'E (SAM NN17061); 1 ♀, Pinkawillinie Conservation
Park, 33º07'S, 136º00'E (SAM NN13799); 1 ♀, Pt Gawler, 34º38'S, 138º28'E (SAM NN13785); 1 ♂, 2
♀, Redcliffe plant site, 33º04'S, 137º34'E (SAM NN13784, NN13788, NN13790); 2 ♂, 1 ♀, Roxby
88
Downs, 30º33'S, 136º54'E (SAM NN16172, NN13803, NN13804); 1 ♂, Roxby Downs, Olympic Dam
site, 30º27'S, 136º54'E (SAM NN13758); 1 ♀, 1 juv., Salt Creek nr Iron Knob, 32º46'S, 137º05'E (SAM
NN13762); 2 ♀, Scrubby Peak, 32º31'S, 135º19'E (SAM NN13800, NN13767); 1 ♀, She-Oak Log,
34º30'S, 138º49'E (SAM NN13789); 1 ♀, Simpson Desert, 26º07'S, 138º37'E (NMV K8177); 1 ♀, South
Gap Station, nr edge Lake Torrens, 31º36'S, 137º32'E (SAM NN13757); 1 ♂, South west of SA, no exact
locality (SAM NN13779); 2 ♀, Spider Lake, 35º13'S, 136º55'E (SAM NN15191-2); 1 ♂, Survey Locks
Well, via Woomera, 31º9'S, 136º48'E (SAM NN13783); 1 ♀, Tarcoola Turnoff, Glendambo area,
30º57'S, 135º43'E (SAM NN17010); Tregalana Station, Whyalla, 20km N, 32º50'S, 137º37'E (SAM no
reg.); 1 ♀, Tregalana Station, Whyalla, 20km N, 32º52'S, 137º33'E (SAM NN13780); 2 ♂, Uno Range,
32º43'S, 136º45'E (SAM NN13771-2); 3 ♀, Wauraltee, 34º35'S, 137º33'E (SAM NN026, NN027,
NN028); 3 ♀, Whyalla Airport, 33º03'S, 137º30'E (SAM NN13796, NN13778, NN13775); WhyteYarcowie, 33º13'S, 138º53'E (SAM NN14721); 1 ♂, Willow Springs Station, Willow Springs
Homestead, 13.5km NNE, 31º21'31''S, 138º50'17''E (SAM NN16196); 1 ♀, Woolshed Flat, 34º07'S,
138º38'E (SAM NN018); 1 ♀, Wynbring Rocks, 30º33'S, 133º32'E (SAM NN13754); 1 ♀, Yardea
Station, Moonarie Homestead, 29km S, 32º22'S, 135º31'E (SAM NN13763); 1 ♀, Yumbarra
Conservation Park, Yumbarra Rockhole Track, 31º46'S, 133º29'E (SAM NN13755); VIC: 1 ♂, Altona
North, 37º52'S, 144º51'E (AM KS20520); 1 ♀, Little Desert, 36º33'S, 141º50'E (NMV K8253); WA: 1
♀, Albion Downs, 24 miles SW, 27º29'S, 120º10'E (WAM 71/1686); 1 ♂, Benjiwarn, 27º47'55''S,
122º40'55''E (WAM T48023); 2 ♂, Bidgemia Station, Gasgoyne Jn, 25º12'34''S, 115º30'50''E (WAM
T65128); 1 ♂, Boolathana Station, 24º24'47''S, 113º40'30''E (WAM T65121); 1 ♂, Boolathana Station,
24º24'48''S, 113º42'24''E (WAM T65122); 1 ♂, Boolathana Station, 24º24'38''S, 113º39'47''E (WAM
T65123); 2 ♀, Boorabin, 31º14'S, 120º19'E (WAM T48021, T48024); 1 ♂, Boulder, 30º47'S, 121º29'E
(AM KS86506); 2 ♀, Buningonia Spring, 31º26'20''S, 123º32'10''E (WAM T48022); 1 ♀, Burnerbinmah
Station, Nangel Paddock, S of Wadda Wadda Well, 28º42'56''S, 117º12'17''E (WAM T52346); 2 ♂, Bush
Bay, 25º07'30''S, 113º49'22''E (WAM T65129); 1 ♀, Carnarvon, 24º53'S, 113º40'E (WAM T63319); 1 ♂,
Commonwealth Rd, West (SE. of Kulin), 32º44'13''S, 118º16'16''E (WAM T62796); 1 ♂, Durokoppin
Nature Reserve, 31º30'S, 117º44'E (WAM T62789); 1 ♂, East Mt Barren, 33º55'S, 120º01'E (WAM
T53507); 1 ♂, Edel Land, 26º31'44''S, 113º29'56''E (WAM T47780); 1 ♂, Eneabba, R.G.C. Mineral
Sands, 29º50'S, 115º15'E (WAM T62793); 2 ♀, 1 juv., Fitzgerald River Inlet, 34º08'S, 119º24'E (WAM
71/769-770, 70/187); 1 ♂, 1 ♀, Fitzgerald River Reserve, 34º04'S, 119º25'E (WAM 71/199-200); 1 ♂,
Fitzgerald River, near; 29km S of Highway 1, 34º08'S, 119º24'E (WAM T55335); 2 ♀, Forrest, 30º44'S,
127º41'E (WAM 69/45169/837); 1 ♂, Francois Peron National Park, 25º58'34''S, 113º34'15''E (WAM
T65569); 1 ♂, Francois Peron National Park, 25º52'31''S, 113º32'59''E (WAM T65556); 1 ♀, Golden
Ridge, 30º51'S, 121º39'E (WAM 28/347); 1 ♀, Great Victoria Desert, Googs Track, E of, SE of Mt
Finke,, 31º08'S, 134º10'E (WAM T63318); 2 ♀, 1 juv., Greenhead, Airstrip 2mi E, no exact locality
(QM S70664-5); 1 ♀, Group 147, via Northcliffe, 34º37'S, 116º08'E (WAM 37/2822); 1 ♂, Hamelin
Homestead, 26º25'S, 114º11'E (WAM T53475); 1 ♂, Howatharra Nature Reserve, 28º32'51''S,
114º39'41''E (WAM T62783); 1 ♂, Irrunytju Rockhole, 26º07'S, 128º58'E (WAM T53379); 1 ♂,
Jibbarding Nature Reserve, 30º00'32''S, 116º49'19''E (WAM T62771); 1 ♂, Kalgoorlie, 50km NE, Black
Swan Nickel Mine, 30º23'07''S, 121º38'59''E (WAM T53250); 1 ♂, Kalgoorlie, 50km NE, Black Swan
Nickel Mine, 30º23'56''S, 121º41'06''E (WAM T56961); 1 ♂, Kalgoorlie, 50km NE, Black Swan Nickel
Mine, 30º24'02''S, 121º40'59''E (WAM T56941); 1 ♂, Kalgoorlie, 5mi N, 30º40'S, 121º27'E (WAM
T53818); 1 ♂, Kambalda, ca. 15km SW, 31º12'58''S, 121º27'23''E (WAM T56553); 1 ♂, Koolanooka
Dam Road, SE of Morawa, 29º14'40''S, 116º06'06''E (WAM T62777); 1 ♀, Lake Colville, 29º30'S,
126º40'E (WAM 89/293-5); 1 ♀, Lake King, 33º05'S, 119º36'E (WAM T53734); 1 ♂, Lake Lefroy, road
to NE reference site, 31º14'S, 121º50'E (WAM T41651); 1 ♂, Lake Lefroy, SW, 31º17'01''S, 121º38'13''E
(WAM T53840); 1 ♀, Lake Lefroy, SW, 31º17'03''S, 121º38'15''E (WAM T45937); 2 ♂, Lake Moore,
35-40 km WNW of Beacon, 30º20'01''S, 117º29'14''E (WAM T51462); 2 ♂, Lorna Glen Station,
26º17'50''S, 121º33'08''E (WAM T64816, T66451); 3 ♂, Lorna Glen Station, 26º16'14''S, 121º29'52''E
(WAM T66443); 2 ♂, Lorna Glen Station, 26º18'13''S, 121º33'46''E (WAM T66449); 1 ♂, Lorna Glen
Station, 26º18'11''S, 121º28'31''E (WAM T66847); 4 ♂, Lorna Glen Station, 26º04'30''S, 121º27'08''E
(WAM T66473, T64843); 1 ♂, Lorna Glen Station, 26º16'26''S, 121º33'34''E (WAM T66453); 1 ♂,
Lorna Glen Station, 26º12'10''S, 121º22'32''E (WAM T64792); 1 ♂, Lorna Glen Station, 26º01'56''S,
121º33'36''E (WAM T64829); 1 ♂, Mardathuna station, 24º30'41''S, 114º38'14''E (WAM T65125); 1 ♀,
McDermid Rock, 32º01'S, 120º44'E (WAM T47785); 1 ♀, Mesa A, 32.7km WSW of Pannnawonica,
21º42'56''S, 116º01'03''E (WAM T77612); 1 ♂, Minniberri, Norrish's property, 3 km W. of Kodj Kodjin
on Minniberri Rd,, 31º15'S, 117º52'E (WAM T62794); 2 ♂, Moore Rd, south (SW. of Mullewa),
28º43'20''S, 115º19'46''E (WAM T62782); 1 ♂, Morawa-Perenjori road, 29º13'56''S, 116º04'05''E (WAM
T65115); 1 ♀, Mt Gibson, 29º35'20''S, 117º12'05''E (WAM T70324); 1 ♂, 1 ♀, Mt Gibson, 29º36'S,
117º24'E (QM S70658-9); 2 ♀, Mt Holland, 20km N, 31º56'S, 119º37'E (WAM T53733, T53694); 1 ♀,
Munda Station, 20º30'21''S, 118º03'36''E (WAM T47610); 1 ♂, Murchison settlement, camp just N,
26º52'35''S, 115º57'9''E (WAM T51477); 1 ♂, Nanga Station, 26º29'23''S, 114º03'24''E (WAM T65557);
89
3 ♂, Nanga Station, 26º28'40''S, 114º04'34''E (WAM T65120); 1 ♂, Naretha, 31º00'S, 124º49'E (WAM
T53626); 1 ♀, Newman, 23º22'S, 119º44'E (WAM 71/1735); 1 ♀, Nullarbor Plain, ca. 18km NE of Haig,
30º56'59''S, 126º15'50''E (WAM T56243); 1 ♂, Oakajee Nature Reserve, 28º34'11''S, 114º38'30''E (WAM
T65117); 1 ♂, Ora Bunda, 30º32'30''S, 121º01'10''E (WAM T62765); 1 ♂, PWD Camp, Murchison
River, 27º42'S, 114º9'E (WAM 69/782); 1 ♀, Queen Victoria Springs Nature Reserve, 30º14'S, 123º41'E
(WAM T53064); 2 ♂, 1 ♀, Quobba Station, Cape Cuvier, 24º14'41''S, 113º33'08''E (WAM T65150,
T63279); 2 ♂, Ravensthorpe, 20km S, 33º46'S, 120º03'E (WAM T62792); 1 ♀, Rawlinna, 70mile E,
30º20'S, 126º03'E (WAM 71/413); 1 ♀, Red Bluff, Red Bluff Caravan Park, 27º44'37''S, 114º08'49''E
(WAM T58302); 1 ♂, Salt River, 45 km ENE of Quairading, 31º53'31''S, 117º49'46''E (WAM T51471); 1
♀, Sanderson Road, N of Lake Goorly, 29º57'29''S, 117º01'05''E (WAM T47784); 1 ♀, State Forest,
32º57'04''S, 115º43'03''E (WAM T53815); 1 ♂, 1 ♀, Stirling Range caravan park, 34º18'55''S,
118º11'14''E (WAM T58378, T62795); 2 ♂, Tutanning, 32º32'S, 117º19'E (WAM T62790, T62791); 2 ♂,
Urawa Nature Reserve, North, 28º24'02''S, 115º34'34''E (WAM T62327); 1 ♀, Wandana Reserve,
28º19'S, 115º9'E (WAM T47783); 1 ♂, Weelhamby Lake, 29º11'22''S, 116º28'25''E (WAM T62780); 1
♂, Weelhamby Lake, West, 29º11'02''S, 116º27'32''E (WAM T48090); 1 ♀, Wiluna, 26º35'S, 120º14'E
(WAM 71/1687); 4 ♂, Woodleigh Station, 26º11'31''S, 114º30'33''E (WAM T65124); 1 ♂, Yuinmary,
28º33'15''S, 119º05'30''E (WAM T48007); 6 ♂, Yuinmery, 28º31'55''S, 119º11'35''E (WAM T56593).
Paratypes of H. forresti: 1 ♀, Morawa, 29º13'S, 116º00'E (WAM 70/172); 1 ♀, Mt Magnet, 323mile
peg, 28º03'S, 117º50'E (WAM 69/46); 1 ♀, Kulin, 32º40'S, 118º9'E (WAM T53819; 33/1607); 1 ♀,
Coonana, 12 miles NW, 30º54'S, 123º01'E (WAM 69/35); 1 ♀, Laverton, Police Station, 28º38'S,
122º24'E (WAM 26/716, published as WAM 26/717 in McKay, 1973); 1 ♀, Marloo Station, 28º19'S,
116º11'E (WAM 69/42).
Hoggicosa alfi
NSW: 1 ♂, Beleuah Station, 90 km NE of Bourke, 29º21'24''S, 146º13'13''E (AM KS37163); 5 ♂, Sturt
National Park, 13.7 km E intersection Middle Road & Camerons Corner Road, 29º02'40''S, 141º18'26''E
(AM KS71045); QLD: 1 ♀, Naretha, 26º35'S, 143º57'E (WAM T55624); SA: 1 ♀, Ampeinna Hills, 10.2
km E, 27º05'04''S, 131º13'45''E (SAM NN11165); 1 ♀, Ampeinna Hills, 10.5 km E, 27º05'13''S,
131º13'15''E (SAM NN11166); 1 ♀, Ampeinna Hills, 11.6 km E, 27º04'52''S, 131º14'03''E (SAM
NN11167); 1 ♂, Anna Creek Station, Mungutana Dam, 7 km NNW, 29º16'13''S, 135º38'53''E (SAM
NN15801); 1 ♀, Approdinna Attora Knolls, Lake Tamblyn camp, 26º02'30''S, 137º36'13''E (SAM
NN15929); 1 ♀, Arckaringa Station, Nasa Bore, 4.6 km NE, 27º46'41''S, 135º12'42''E (SAM NN15826);
2 ♂, Arcoona Station, May Hill, 5.1 km W, 31º17'16''S, 136º34'59''E (SAM NN15777-8); 1 ♂, Calperum
Station, Yabbie Tanks, 2.25 km NE, 33º36'S, 140º34'E (SAM NN16388); 4 ♂, Cheesman Peak, 12.2 km
NW, 27º20'13''S, 130º14'15''E (SAM NN11099-102); 1 ♂, Cheesman Peak, 4.5 km NE, 27º22'26''S,
130º21'44''E (SAM NN11108); 1 ♂, Cheesman Peak, 4.7 km NNE, 27º22'01''S, 130º21'06''E (SAM
NN11127); 2 ♂, Cheesman Peak, 9.3 km NNW, 27º19'46''S, 130º17'36''E (SAM NN11103-4); 12 ♂,
Clifton Hills Outstation (E of), 26º30'S, 139º29'E (SAM NN16001-12); 9 ♂, Clifton Hills Outstation, 4.1
km NE, 26º30'40''S, 139º28'42''E (SAM NN15332-8, NN15388, NN15400); 11 ♂, Clifton Hills
Outstation, 4.25 km NW, 26º31'07''S, 139º26'04''E (SAM NN15360-70); 7 ♂, Clifton Hills Outstation,
5.25 km E, 26º32'25''S, 139º30'17''E (SAM NN15339, NN15355-8, NN15398-9); 26 ♂, Clifton Hills
Outstation, 5.7 km NE, 26º30'37''S, 139º29'33''E (SAM NN15340-54, NN15371-81); 6 ♂, 2 ♀, Clifton
Hills Ruin, 26º31'S, 139º26'E (SAM NN16013-6, NN16021, NN16022, NN16024, NN16025); 1 ♂,
Coomandook, 2 km S, 35º29'03''S, 139º41'10''E (SAM NN16332); 2 ♂, 1 ♀, 3 juv., Coongie, 27º12'S,
140º10'E (SAM NN16087-8, NN16150); 1 ♀, Cowell, 33º19'29''S, 137º05'36''E (SAM no reg.); 10 ♂,
Dalarinna Hill, 8.5 km E, 29º43'13''S, 138º40'18''E (SAM NN15790-9); 1 ♂, Dalarinna Hill., 10 km SE,
29º45'27''S, 138º40'04''E (SAM NN15775-6); 2 ♀, Danggali Conservation Park, Tomahawk Dam, 3 km
N, 33º19'39''S, 140º42'50''E (SAM NN17069, NN17075); 1 ♀, Emu, 51 km W, 28º32'S, 131º43'E (SAM
NN16109); 1 ♂, Galga, 19 km N, 34º30'06''S, 139º55'18''E (SAM NN16306); 1 ♀, Gluepot Station,
Gluepot Homestead, 8.5 km W-WNW, 33º44'49''S, 140º01'56''E (SAM NN18699); 1 ♀, 1 juv., Head of
Bight, 31º29'S, 131º9'E (SAM NN16158); 1 ♂, Ketchalby Rockhole, 9.6 km S, 32º37'28''S, 135º01'56''E
(SAM no reg.); 1 ♂, 1 juv., Koonchera Waterhole, 10.5 km SSE, 26º45'42''S, 139º31'48''E (SAM
NN15397); 1 ♂, Koonchera Waterhole, 4 km SSE, 26º42'46''S, 139º30'42''E (SAM NN15389); 2 ♂,
Kunytjanu, 25 km N, 26º29'16''S, 129º10'25''E (SAM NN11122-3); 4 ♂, Mabel Creek Homestead, 25 km
SSW, 29º10'20''S, 134º14'30''E (SAM NN15253, NN15254-5, NN15258); 1 ♂, Mabel Creek Homestead,
28 km SSW, 29º11'40''S, 134º15'E (SAM NN15260); 1 ♂, Mabel Creek Homestead, 28 km SW, 29º10'S,
134º11'30''E (SAM NN15252); 2 ♂, Mabel Creek Homestead, 30 km SW, 29º9'40''S, 134º06'30''E (SAM
NN15256-7); 1 ♂, Mabel Creek Station, Lake Phillipson, 10 km N, 29º21'30''S, 134º28'E (SAM
NN15259); 1 ♂, Maralinga, 12 km SSW, 30º16'00''S, 131º33'10''E (SAM NN15249); 1 ♂, Memory Bore
Camp, 26º42'S, 135º32'E (SAM NN15786); 2 ♂, Mootatunga, 4 km S, 34º59'16''S, 140º50'16''E (SAM
NN16304-5); 3 ♂, Mt Hoare, no exact locality (SAM no reg.); 8 ♂, 3 ♀, Mt Hoare, 6 km W, 27º03'23''S,
129º38'20''E (SAM no reg.); 1 ♂, 1 juv., Mt Lindsay, 3.1 km WNW, 27º01'9''S, 129º51'01''E (SAM
90
NN11128); 1 ♂, 2 ♀, Mt Lindsay, 48.9 km SE, 27º18'50''S, 130º15'54''E (SAM NN11124-6); 2 ♂, Mt
Lindsay, 6.6 km WNW, 27º03'39''S, 129º49'26''E (SAM NN11129-30); 2 ♂, Muckera Rockhole, 52 km
N, 29º33'33''S, 130º08'19''E (SAM NN15248, NN16100); 1 ♀, Munyaroo Conservation Park, 17 km SSE
Moonabbie, 33º23'44''S, 137º21'17''E (SAM no reg.); 1 ♂, New Alton Downs Homestead, 19.7 km SE,
26º35'27''S, 139º08'01''E (SAM NN15359); 1 ♂, 1 ♀, no exact locality (SAM NN1629, no reg.); 1 ♂, Pile
Hill., 6.3 km SW, 29º08'11''S, 138º24'9''E (SAM NN15783); 3 ♂, Pinkawillinie, 33º03'20''S, 135º46'57''E
(SAM no reg.); 2 ♂, Relief Bore, Tallaringa Conservation Park, 68.5 km W, 28º13'S, 133º22'E (SAM
NN15246-7); 1 ♀, Serpentine Lakes, 28º30'S, 129º00'E (SAM NN16127); 1 ♀, Simpson Desert, Knolls
Track, 26º07'S, 137º37'E (WAM T53488); 1 ♂, Simpson Desert, Purni Bore, Colson Track, 69.8 km E,
26º15'36''S, 136º47'39''E (SAM NN15932); 1 ♂, Simpson Desert, Purni Bore, French Line, 29.4 km
ENE, 26º13'48''S, 136º23'00''E (SAM NN15931); 1 ♂, Simpson Desert, Purni Bore, Rig Rd, 30.3 km E,
26º15'41''S, 136º23'51''E (SAM NN15930); 1 ♂, Simpson Desert, Purni Bore, Rig Rd, 44.7 km E,
26º19'16''S, 136º32'30''E (SAM NN15927); 1 ♀, South Gap Station, Beda Hill (near), 31º51'S, 137º37'E
(SAM NN16179); 1 ♂, Tallaringa Well, Tallaringa Conservation Park, 2.7 km W, 29º01'S, 133º16'E
(SAM NN15245); 6 ♂, Taylorville Station, 15 Mile Dam, 34º02'12''S, 140º11'04''E (SAM NN17040-1,
NN17013-6); 1 ♂, Taylorville Station, Casuarina Dam, 33º53'10''S, 140º18'32''E (SAM NN17038); 2 ♂,
Taylorville Station, Middle Dam, 1.5 km SW, 33º54'37''S, 140º12'20''E (SAM NN17031-2); 1 ♂,
Todmorden Homestead, 18.4 km NNE, 26º58'58''S, 134º48'36''E (SAM NN15926); 3 ♂, 2 ♀, 1 juv.,
Warburton River, Yelpawaralinna Waterhole, 27º07'30''S, 138º42'30''E (SAM NN15996, NN15997-8,
NN15999, NN16049); 3 ♂, Warburton River, Yelpawaralinna Waterhole, 1.8 km ESE, 27º05'19''S,
138º41'01''E (SAM NN15394-6); 6 ♂, Warburton River, Yelpawaralinna Waterhole, 7.6 km NNW,
27º06'22''S, 138º41'49''E (SAM NN15382-7); 2 ♀, Wyola Lake, 29º9'S, 130º14'E (SAM NN16103,
NN13672); WA: 1 ♂, 1 ♀, no exact locality (WAM T77405, T77406); 3 ♂, Badjaling, 1.5km N, 31º59'S,
117º30'E (WAM T53790); 7 ♂, Boolathana Station, 24º24'49''S, 113º44'41''E (WAM T65567); 1 ♀,
Boorabie, Nullabor Plain, 29º03'S, 128º26'E (WAM T65116); 3 ♂, Bungalbin Hill, Aurora Range,
30º16'11''S, 119º43'30''E (WAM T62809); 1 ♂, Buningonia Spring, 3.5 km SW, 31º26'S, 123º32'E
(WAM T51394); 1 ♀, Carnarvon, 50 miles N, 24º10'S, 113º40'E (WAM T53873); 1 ♀, East Nugadong
Nature Res., 30º12'S, 116º57'E (WAM T63247); 1 ♀, Edel Land, 26º08'45''S, 113º26'15''E (WAM
T62314); 1 ♂, Goongarrie Station, 30º06'04''S, 121º9'18''E (WAM T46063); 1 ♂, Goongarrie Station,
29º53'59''S, 121º10'35''E (WAM T46062); 1 ♂, Goongarrie Station, 29º58'04''S, 121º04'54''E (WAM
T46058); 1 ♂, Goongarrie Station, 29º56'48''S, 121º07'00''E (WAM T46057); 1 ♂, Goongarrie Station,
29º50'13''S, 120º57'36''E (WAM T46061); 2 ♂, Kennedy Range National Park, 24º34'14''S, 114º57'12''E
(WAM T65560); 2 ♂, 1 ♀, Kennedy Range National Park, 24º30'01''S, 115º01'07''E (WAM T65559); 1
♀, 3 juv., Koorda, 30º49'S, 117º29'E (SAM NN16594); 1 ♀, Lake Mackay, 22º26'47''S, 128º27'33''E
(WAM T84373); 3 ♂, Laverton, 39 km E, 28º28'S, 122º50'E (WAM T55586, T65571, T65572); 1 ♂,
Little Sandy Desert, 18.2 km NNE. Of Kulonoski East Well, 24º31'45''S, 120º17'44''E (WAM T66896); 1
♂, Lorna Glen Station, 26º13'35''S, 121º31'08''E (WAM T55131); 2 ♂, Lorna Glen Station, 26º15'55''S,
121º16'53''E (WAM T70326); 1 ♂, 1 ♀, Lorna Glen Station, 26º15'58''S, 121º06'40''E (WAM T70333,
T70334); 11 ♂, Lorna Glen Station, 26º16'53''S, 121º21'27''E (WAM T53917, T64664); 9 ♂, 1 ♀, Lorna
Glen Station, 26º12'04''S, 121º18'14''E (WAM T53919, T64621); 3 ♂, Lorna Glen Station, 26º14'07''S,
121º16'53''E (WAM T53918, T64926); 3 ♂, Lorna Glen Station, 26º17'06''S, 121º22'9''E (WAM T53921,
T64924); 1 ♂, Lorna Glen Station, 26º09'28''S, 121º33'50''E (WAM T64729); 2 ♂, Lorna Glen Station,
26º00'05''S, 121º33'48''E (WAM T66403); 12 ♂, 1 ♀, 2 juv., Mardathuna Station, 24º25'43''S,
114º30'00''E (WAM T65568, T62808); 1 ♂, 1 juv., Mardathuna Station, 24º24'23''S, 114º26'42''E (WAM
T65570); 1 ♀, Monkey Mia, Shark Bay, Faure Island, 15 km SE, 25º52'30''S, 113º53'12''E (SAM
NN14132); 1 ♂, 1 ♀, Moore Rd, south (SW. of Mullewa), 28º43'20''S, 115º19'46''E (WAM T62807); 3
♂, Morgan Range, 25º53'30''S, 128º25'38''E (WAM T79150); 1 ♀, 3 juv., Mt Elvire Station, 29º33'36''S,
119º36'08''E (WAM T63249); 9 ♂, 1 juv., Nanga Station, 26º32'47''S, 113º57'47''E (WAM T65566); 1 ♂,
1 ♀, Nanga Station, 26º32'47''S, 113º57'47''E (WAM T47778, T62772); 3 ♂, Nanga Station, 26º31'21''S,
114º00'08''E (WAM T65564); 14 ♂, Nanga station, 26º35'32''S, 113º53'22''E (WAM T65118); 2 ♂,
Nanga Station, 26º29'23''S, 114º03'24''E (WAM T65565); 2 ♂, Nerren Nerren Station, 27º00'22''S,
114º32'29''E (WAM T65563); 4 ♂, Nerren Nerren Station, 27º03'28''S, 114º30'25''E (WAM T65561); 4
♂, Nerren Nerren Station, 27º03'00''S, 114º34'32''E (WAM T65562); 1 ♂, Nerren Nerren Station,
27º03'24''S, 114º34'23''E (WAM T65558); 29 ♂, Point Salvation, 7 – 8 km WNW, 28º12'S, 123º36'E
(WAM T62373 T62810 T62374 T65573 T65574 T65575 T65576 T65577 T65585); 1 ♀, Queen Victoria
Spring Nature Reserve, Streich Mound, 30º28'S, 123º41'E (WAM T63281); 1 ♂, Queen Victoria Spring,
1 km NE of, 30º28'S, 123º41'E (WAM T63246); 13 ♂, Queen Victoria Springs Nature Reserve, 30º14'S,
123º41'E (WAM T49114, T49134, T52355, T52540, T52569, T52675, T52682, T52700, T53135); 1 ♀,
Rudall River, 22º28'S, 122º29'E (WAM 71/1582); 1 ♂, Tanami, 90 km SE of Sturt Creek, 19º35'20''S,
128º52'13''E (WAM T70981); 10 ♂, Walter James Range, 24º37'45''S, 128º45'22''E (WAM
T79143,T79144); 3 ♂, Walter James Range, 24º41'37''S, 128º45'47''E (WAM T79139); 2 ♂, Walter
James Range, 24º46'57''S, 128º46'48''E (WAM T79140); 2 ♂, Walter James Range, 24º39'16''S,
91
128º45'21''E (WAM T79137); 5 ♂, Walter James Range, 24º42'27''S, 128º45'38''E (WAM T79142); 8 ♂,
Walter James Range, 24º48'03''S, 128º47'50''E (WAM T79141); 5 ♂, Walter James Range, 24º33'35''S,
128º42'36''E (WAM T79138); 1 ♀, Wandana Reserve, 28º19'S, 115º9'E (WAM T62770); 1 ♀, 3 juv.,
Well 43, Canning Stock Route, 21º12'S, 125º59'E (WAM 73/140-3); 23 ♂, Yamarna Station, 28º13'30''S,
123º35'30''E (WAM T65586, T65587, T65588); 3 ♂, Yundamindra, 29º24'00''S, 122º28'05''E (WAM
T47776); 1 ♂, Zuytdorp, 27º15'50''S, 114º04'14''E (WAM T63248). Paratypes of H. forresti: 1 ♀, Mt
Magnet, 323 mile peg, 28º03'S, 117º50'E (WAM 69/791); 1 ♀, Paynes Find area, 323 mile peg, 29º15'S,
117º41'E (WAM 70/186).
Hoggicosa bicolor
NT: 1 ♂, 2 ♀, Alice Springs, 23º42'S, 133º52'E (SAM NN17243, AM KS71064, NTMAG, no reg.); 1 ♀,
Alice Springs Desert Park, 23º42'S, 133º52'E (AM KS69273); 1 ♀, 1 juv., Alice Springs, 8 km W,
23º42'S, 133º53'E (AM KS40990); 1 ♀, Bitter Springs (near), 23º33'S, 134º27'E (SAM NN13671); 1 juv.,
Charlotte Waters, 25º55'S, 134º54'E (NMV K8201); 1 ♀, Hermannsburg, 23º56'S, 132º46'E (SAM
NN17220); 1 ♀, Idacowra Station, nr Finke River, 23º55'S, 132º43'E (SAM NN17219); 1 ♂, Kings Creek
Station, 24º26'21''S, 131º49'15''E (SAM NN16570); 1 juv., Palm Creek, 24º03'S, 132º40'E (NMV
K8202); 1 ♀, Rabbit Flat Roadhouse, 24 km W, 20º11'S, 129º45'E (NTMAG no reg.); 1 ♀, Tennant
Creek, 19º39'S, 134º11'E (SAM NN17221); 6 ♀, 10 juv., Tennant Creek, 19º39'S, 134º11'E (QM
S21353); 2 ♀, Trephina Gorge turnoff, near Alice Springs, 23º32'S, 134º24'E (QM S21358); 1 ♂, Uluru,
25º20'S, 131º02'E (SAM NN16560); 2 ♀, 1 juv., Uluru, 25º21'S, 131º02'E (QM S21357); 2 ♀,
Wauchope, 20º39'S, 134º13'E (QM S21364); 1 ♀, Yulara, 25º15'S, 122º58'E (AM KS69260); Qld: 1 ♀,
Beaudesert, 21º32'S, 141º06'E (QM S70647); 1 ♂, Byrock, 24 km NW, 26º03'S, 143º08'E (AM
KS82556); 2 ♂, 5 ♀, 5 juv., Camooweal, 19º56'S, 138º07'E (QM S21362); 1 ♂, 2 ♀, 3 juv., Lake Julius
turnoff, 20 km E Mt Isa, 20º44'S, 139º29'E (QM S21363); SA: 1 ♂, Amata, 35 km SE, 26º16'37''S,
131º27'38''E (SAM NN11118); 1 ♀, Bookaloo, E of, 31º54'9''S, 137º28'06''E (SAM NN13684); 1 ♀,
Candosa, no exact locality (SAM no reg.); 3 ♂, Cheesman Peak, 4.7 km NNE, 27º22'01''S, 130º21'06''E
(SAM NN11105-7); 1 ♀, 2 juv., Coober Pedy, 10 miles E, 29º01'S, 134º55'E (WAM 70/214-6); 1 ♀,
Cook, 145 km N, 29º29'S, 130º10'E (SAM NN13677); 1 ♂, Donald Well Hill, 0.7 km WNW, 26º12'17''S,
132º19'42''E (SAM NN11117); 1 ♂, East Arckaringa Homestead, 27º54'30''S, 134º50'20''E (SAM
NN16151); 1 ♂, Everard Ranges, 27º10'S, 132º25'E (SAM NN21381); 1 ♂, Everard Ranges, 2.6 km
WNW Etelerinna Hill, 27º08'S, 132º24'E (SAM no reg.); 1 ♀, Gawler Ranges, 32º43'39''S, 136º47'16''E
(SAM NN13680); 1 ♂, Hambidge, 33º23'S, 135º57'E (SAM NN17001); 1 ♂, Hamilton Homestead, 13.4
km SSE, 26º49'20''S, 135º08'11''E (SAM NN15920); 1 ♀, Hamilton Station, Bitchera WH, 6.1 km
WNW, 26º33'37''S, 134º28'25''E (SAM NN15622); 1 ♂, Hamilton Station, Bitchera WH, 10.9 km WNW,
26º31'25''S, 134º26'31''E (SAM NN15529); 1 ♂, Indulkana Creek, 26º55'S, 133º47'E (SAM NN21382); 1
♂, Ketchalby Rockhole, 9.6 km S, 32º37'28''S, 135º01'56''E (SAM no reg.); 3 ♂, Kunytjanu, 26 km S,
26º24'18''S, 129º07'47''E (SAM NN11119-21); 2 ♂, Kunytjanu, 8 km NW, 26º36'55''S, 129º18'51''E
(SAM NN11109-10); 1 ♀, Lake Gairdner (near), 32º17'S, 135º55'51''E (SAM NN13679); 1 ♂, Lambina
Homestead, 12.6 km NNE, 26º48'01''S, 134º05'26''E (SAM NN15921); 1 ♂, Lambina Homestead, 47.1
km N, 26º29'14''S, 134º02'30''E (SAM NN15922); 1 ♂, Ludgate Well, 4 km WSW, 26º25'30''S,
134º51'15''E (SAM NN15523); 3 ♂, Mabel Creek Homestead, 28 km SW, 29º10'S, 134º11'E (SAM
NN16036-8); 1 ♀, Makiri, 27º04'S, 131º09'E (SAM NN13675); 1 ♂, Marla, 34º20'S, 139º31'E (SAM
NN13822); 1 ♂, Maryinna Hill, 11.5 km SSE, 27º03'34''S, 131º16'00''E (SAM NN21443); 1 ♂, Mimili,
26.3 km ENE, 26º54'47''S, 132º57'03''E (SAM NN11089); 1 ♂, Mimili, 26 km ENE, 26º54'50''S,
132º56'54''E (SAM NN11088); 1 ♂, 1 ♀, Mimili, 31.5 km ENE, 26º53'45''S, 132º59'58''E (SAM
NN11060, NN11090); 1 ♂, Mt Lindsay, 27º01'30''S, 129º52'32''E (SAM NN11087); 1 ♀, Mt Lindsay
(Wataru), 27º01'32''S, 129º52'36''E (SAM NN11061); 1 ♀, 1 juv., Mt Lindsay (Wataru), 27º01'30''S,
129º52'32''E (SAM NN11062); 8 ♂, 1 ♀, Mt Lindsay, 48.9 km SE, 27º18'50''S, 130º15'54''E (SAM
NN11059, NN11091-3, NN11094-8); 1 ♂, Mt Sarah Homestead, 11.7 km SSW, 27º01'32''S, 135º13'10''E
(SAM NN15923); 1 ♂, Ngarutjara Homeland, 10 km NNE Mt Woodroffe, 26º18'S, 131º44'E (SAM
NN11086); 1 ♂, North Arckaringa Creek, 27º42'50''S, 134º49'10''E (SAM NN16073); 1 ♀, Pinkawillinie
Conservation Park, 33º06'52''S, 135º59'50''E (SAM NN13681); 1 ♀, Pinkawillinie Conservation Park,
33º07'S, 136º00'E (SAM NN13678); 1 ♂, Relief Bore, Tallaringa Conservation Park, 65.6 km W,
28º12'S, 133º23'E (SAM NN14662); 2 ♂, Sentinal Hill, 1.4 km SW, 26º05'35''S, 132º26'37''E (SAM
NN11113-4); 1 ♂, Sentinal Hill, 10.4 km SW, 26º08'19''S, 132º22'01''E (SAM NN11116); 1 ♂, Sentinal
Hill, 10.5 km S, 26º10'34''S, 132º27'22''E (SAM NN11112); 1 ♂, Sentinal Hill, 14 km SE, 26º10'18''S,
132º32'52''E (SAM NN11115); 1 ♀, Sentinel Hill, nr & SW of, 26º05'S, 132º26'E (SAM NN11063); 1 ♀,
Serpentine Lake, E side, 28º30'20''S, 129º02'30''E (SAM NN13674); 2 ♂, Simpson Desert, Purini Bore,
Rig Rd, 43.7 km E, 26º19'17''S, 136º31'53''E (SAM NN15925, NN15928); 3 ♂, Tallaringa boundary at
Mabel Creek Station, 28º59'S, 133º49'E (SAM NN16143-5); 1 ♀, Tallaringa Well, 50 km W, 28º55'S,
132º50'E (SAM NN13673); 1 ♂, Todmorden Homestead, 12.6 km ENE, 27º07'01''S, 134º52'43''E (SAM
NN15924); 1 ♂, Todmorden Homestead, 17.4 km ESE, 27º11'04''S, 134º55'25''E (SAM NN15940); 1 ♀,
92
Uno Range, 32º43'S, 136º41'E (SAM NN13682); 1 ♀, Vokes Hill, 28º33'S, 130º34'E (SAM NN13676); 1
♂, Womikata Bore, 6 km WSW, 26º06'33''S, 132º05'57''E (SAM NN11111); 1 ♀, Woomera, 31º9'S,
136º48'E (SAM NN13683); WA: 1 ♀, Amy Giles Rocks, 25º53'26''S, 128º31'35''E (WAM T79145); 1 ♂,
Bencubbin Kellerberrin rd., 31º24'37''S, 117º45'06''E (WAM T63274); 1 ♂, Bidgemia Station, Gasgoyne
Junction, 25º10'31''S, 115º29'17''E (WAM T65171); 4 ♂, Boolathana Station, 24º24'49''S, 113º44'41''E
(WAM T65170, T65168); 2 ♂, Boolathana Station, 24º24'48''S, 113º42'24''E (WAM T65169); 2 ♂,
Brockman, 16.5 km SW of Mount Brockman, 22º34'19''S, 117º11'34''E (WAM T78135); 1 ♂, Brockman,
19 km SW of Mount Brockman, 22º36'01''S, 117º11'21''E (WAM T78136); 1 ♂, Brockman, 3.5 km W. of
Mount Brockman, 22º27'52''S, 117º16'07''E (WAM T78134); 1 ♀, 1 juv., Burnabinmah Station, 28º47'S,
117º22'E (WAM 71/880-1); 1 ♀, Canning Stock Route, Well 10-1, 24º51'S, 121º39'E (NMV K8169); 1
♀, Canning Stock Route, Well 31, no exact locality (WAM T55303); 1 ♂, Cape Cuvier, Quobba Station,
24º13'24''S, 113º30'13''E (WAM T65555); 1 ♂, Chook Lake, 29º53'32''S, 123º35'44''E (SAM NN21380);
1 ♀, Coolcalalaya Station, vicinity of Murchison, 27º31'S, 115º03'E (WAM T53502); 2 ♀, Diamond Well
Station, 26º27'39''S, 119º27'01''E (WAM T46097); 3 ♂, 2 juv., Durokoppin Nature Reserve, 31º30'S,
117º44'E (WAM T51355, T55579, T62484); 2 ♂, 1 juv., East Yorkrakine Reserve, 31º28'S, 117º41'E
(WAM T55580, T63277); 3 ♂, Francois Peron National Park, 25º50'20''S, 113º36'23''E (WAM T63253);
1 ♀, Gibson Desert, Huntoil Road, 24º06'S, 125º51'E (WAM T47718); 1 ♂, Gill Pinnacle, Schwerin
Mural Crescent, 24º53'S, 128º47'E (SAM NN16589); 2 ♂, Goongarrie Station, 29º58'12''S, 120º59'17''E
(WAM T46069); 1 ♂, Goongarrie Station, 29º58'48''S, 121º07'00''E (WAM T46066); 1 ♂, Goongarrie
Station, 29º55'16''S, 121º08'52''E (WAM T46072); 1 ♂, Goongarrie Station, 29º58'04''S, 121º04'54''E
(WAM T46067); 2 ♂, Goongarrie Station, 29º55'24''S, 121º08'27''E (WAM T46071); 1 ♂, Goongarrie
Station, 30º02'32''S, 120º52'53''E (WAM T46070); 1 ♂, Goongarrie Station, 29º58'06''S, 122º01'30''E
(WAM T46068); 1 ♀, Grasspatch, 'Sieda', Fitzgerald Locality 41, 33º14'S, 121º43'E (WAM T47719); 1
♀, Hamersley Range, 10 miles S, on Mt Tom Price Road, 22º21'S, 117º19'E (WAM 69/1045); 1 ♂, 1 ♀,
Hope Downs Station, 22º30'S, 119º05'E (WAM T45560); 1 ♂, Hope Downs Station, 22º30'S, 119º14'E
(WAM T45559); 1 ♀, Jiggalong Mission, vicinity of, 23º22'S, 120º47'E (WAM 71/1438); 4 ♂, Jundee,
11.7 km N of Jundee homestead, 26º14'57''S, 120º40'19''E (WAM T70263); 1 ♀, Jundee, 14.1 km ESE of
Lake Violet Homestead, 26º35'59''S, 120º47'24''E (WAM T70262); 1 ♂, 1 ♀, Jundee, 8.5 km SSE of
Jundee homestead, 26º25'16''S, 120º40'45''E (WAM T70264, T70265); 10 ♂, Laverton, 39 km E, 28º28'S,
122º50'E (WAM T65579, T62768, T62769, T55585, T55574, T55592, T65578); 1 ♂, Leonora, 370 km
E, Warburton Road, 28º36'S, 124º47'E (WAM T63276); 1 ♂, Little Sandy Desert, 17.5 km SE of
Burranbar Pool, 23º55'23''S, 120º31'51''E (WAM T47724); 1 ♂, Little Sandy Desert, 20.8 km NNE. Of
Kulonoski East Well, 24º30'33''S, 120º18'31''E (WAM T66895); 1 ♂, Little Sandy Desert, Cooma Well,
24º04'46''S, 120º20'15''E (WAM T47723); 3 ♂, Lorna Glen Station, 26º11'32''S, 121º11'40''E (WAM
T70327, T70328, T70329); 2 ♂, Lorna Glen Station, 26º11'59''S, 121º15'59''E (WAM T70276, T70280);
4 ♂, Lorna Glen Station, 26º12'04''S, 121º18'13''E (WAM T53920, T70278, T70279); 1 ♂, Lorna Glen
Station, 26º15'58''S, 121º06'40''E (WAM T70332); 1 ♂, Lorna Glen Station, 26º13'35''S, 121º31'08''E
(WAM T70330); 1 ♂, Lorna Glen Station, 26º12'04''S, 121º18'14''E (WAM T70273); 1 ♂, Lorna Glen
Station, 26º15'55''S, 121º16'53''E (WAM T70325); 1 ♂, Lorna Glen Station, 26º17'50''S, 121º33'08''E
(WAM T70275); 3 ♂, Lorna Glen Station, 26º16'53''S, 121º21'27''E (WAM T53911, T70274); 1 ♂,
Lorna Glen Station, 26º14'07''S, 121º16'53''E (WAM T64925); 1 ♂, Lorna Glen Station, 26º16'57''S,
121º06'44''E (WAM T70331); 1 ♂, Lorna Glen Station, 26º04'30''S, 121º27'08''E (WAM T64768); 1 ♂,
Lorna Glen Station, 26º04'09''S, 121º26'54''E (WAM T64761); 1 ♂, Lorna Glen Station, 26º07'48''S,
121º31'02''E (WAM T53913); 2 ♂, Mardathuna Station, 24º25'43''S, 114º30'00''E (WAM T65163); 3 ♂, 1
♀, Mardathuna Station, 24º24'23''S, 114º26'42''E (WAM T47715, T65164); 1 ♂, Mardathuna Station,
24º26'36''S, 114º30'42''E (WAM T63272); 1 ♂, Mardathuna Station, 24º30'41''S, 114º38'14''E (WAM
T65127); 6 ♂, Meedo Station, 25º40'49''S, 114º37'20''E (WAM T65158, T65161); 2 ♂, Meedo Station,
25º42'42''S, 114º35'58''E (WAM T65162); 1 ♀, Meedo Station, 25º37'23''S, 114º41'40''E (WAM
T47717); 1 ♂, Meekatharra, 86 km N, 25º56'05''S, 118º50'36''E (WAM T52094); 1 ♂, Morgan Range,
25º55'58''S, 128º26'57''E (WAM T79147); 1 ♂, Morgan Range, 25º56'08''S, 128º26'16''E (WAM
T79149); 1 ♂, Mt Brockman, 22º25'08''S, 117º24'32''E (WAM T63271); 1 ♂, Mt Brockman, 22º18'39''S,
117º15'35''E (WAM T63273); 1 ♀, Mt Brockman, Nammuldi Mine (Hamersley Iron), 22º24'41''S,
117º26'03''E (WAM T47720); 1 ♂, Mt Fraser, 25º38'S, 118º23'E (WAM T62334); 1 ♂, Mt Gibson
Station, 29º47'9''S, 117º20'04''E (WAM T46044); 1 ♀, Mt Gibson turnoff, 2 miles E (Paynes Find),
29º37'S, 117º07'E (WAM 68/792); 3 ♂, Mt Keith mine, 13.8 km E. of Lake Way homestead, 26º57'43''S,
120º35'44''E (WAM T74638); 1 ♂, Mt Keith mine, 14.2 km ENE. of Mt Keith homestead, 27º14'35''S,
120º38'59''E (WAM T74650); 1 ♂, Mt Keith mine, 14.2 km E. of Mount Keith homestead, 27º38'56''S,
120º38'56''E (WAM T74629); 2 ♂, 1 ♀, Mt Keith mine, 14.3 km ENE. of Mount Keith homestead,
27º14'35''S, 120º38'59''E (WAM T74607, T74612, T74614); 16 ♂, Mt Keith mine, 14.4 km ESE. of
Lake Way homestead, 26º58'53''S, 120º36'24''E (WAM T74280, T74630, T74633); 2 ♂, Mt Keith mine,
14.8 km E. of Lake Way homestead, 26º58'9''S, 120º36'53''E (WAM T74648); 12 ♂, Mt Keith mine, 15.5
km E. of Lake Way homestead, 26º57'41''S, 120º37'22''E (WAM T74634, T74642); 1 ♂, Mt Keith mine,
93
15.6 km E. of Mount Keith homestead, 26º57'41''S, 120º37'25''E (WAM T74279); 1 ♂, Mt Keith mine,
17.8 km ESE. of Lake Way homestead, 26º58'54''S, 120º38'33''E (WAM T74637); 4 ♂, 1 ♀, Mt Keith
mine, 18.6 km SE. of Lake Way homestead, 27º03'29''S, 120º36'22''E (WAM T74631, T74651); 1 ♀, Mt
Keith mine, 18.7 km SE. of Lake Way homestead, 27º03'29''S, 120º36'22''E (WAM T74613); 5 ♂, Mt
Keith mine, 22.4 km E. of Mount Keith homestead, 27º14'19''S, 120º43'58''E (WAM T74283, T74290,
T74641); 3 ♂, 1 ♀, Mt Keith mine, 22.5 km E. of Mount Keith homestead, 27º14'18''S, 120º44'01''E
(WAM T74288, T74293, T74295, T74652); 5 ♂, Mt Keith mine, 22.5 km ESE. of Lake Way homestead,
26º58'53''S, 120º36'24''E (WAM T74645); 1 ♂, Mt Keith mine, 22.5 km SE. of Lake Way homestead,
27º06'17''S, 120º36'21''E (WAM T74610); 1 ♂, Mt Keith mine, 24.6 km E. of Mount Keith homestead,
27º15'11''S, 120º45'30''E (WAM T74289, T74628); 15 ♂, Mt Keith mine, 26.1 km ENE. of Mount Keith
homestead, 27º13'22''S, 120º46'03''E (WAM T74287, T74291, T74292, T74294, T74602, T74609,
T74611, T74636); 5 ♂, Mt Keith mine, 26.2 km ENE. of Mount Keith homestead, 27º13'21''S,
120º46'06''E (WAM T74282, T74284, T74286, T74605, T74606); 2 ♂, Mt Keith mine, 28.9 km ENE. of
Mount Keith homestead, 27º11'22''S, 120º47'08''E (WAM T74604, T74608); 2 ♂, Mt Keith mine, 29 km
ENE. of Mount Keith homestead, 27º11'22''S, 120º47'12''E (WAM T74285, T74603); 2 ♂, Mt Keith
mine, 9.3 km ESE. of Lake Way homestead, 26º57'57''S, 120º33'31''E (WAM T74635, T74646); 2 ♂, Mt
Keith mine, 9.5 km ESE. of Lake Way homestead, 26º58'25''S, 120º33'29''E (WAM T74277, T74278); 8
♂, Mt Keith mine, 9.6 km ESE. of Lake Way homestead, 26º58'25''S, 120º33'29''E (WAM T74632,
T74640); 2 ♂, Mt Keith mine, 9 km E. of Lake Way homestead, 26º56'22''S, 120º33'29''E (WAM
T74649); 1 ♀, 2 juv., Mt Magnet, 323 mile peg, 28º03'S, 117º50'E (WAM 68/822, 69/843, 69/1037); 1 ♀,
Mt Vernon, 24º13'S, 118º14'E (WAM T47710); 1 ♂, 1 ♀, Mt Vernon Station, 53.4 km SE, 24º30'S,
118º30'E (WAM T62336); 2 ♂, Nanga Station, 26º29'23''S, 114º03'24''E (WAM T63265, T65167); 4 ♂,
3 ♀, Nerren Nerren Station, 27º03'00''S, 114º34'32''E (WAM 94/1939, T51221, T51222, T63269,
T63270, T63275, T65165); 4 ♂, Nerren Nerren Station, 27º03'24''S, 114º35'21''E (WAM T63268,
T65166); 1 ♂, Nerren Nerren Station, 27º00'21''S, 114º32'29''E (WAM T51223); 1 ♂, Nerren Nerren
Station, 27º00'22''S, 114º32'29''E (WAM T63255); 1 ♂, Nerren Nerren Station, 27º07'24''S, 114º35'21''E
(WAM T51224); 1 ♂, Nerren Nerren Station, 27º03'28''S, 114º36'25''E (WAM T47725); 1 ♂, Nerren
Nerren Station, 27º03'00''S, 114º34'32''E (WAM); Nerren Nerren Station, 27º03'28''S, 114º36'25''E
(WAM 94/1942); 1 ♂, Nerren Nerren Station, 27º08'S, 114º38'E (WAM T62724); 2 ♂, Newman, 15 km
N by W of, 23º13'S, 119º29'E (ANIC no reg.); 1 ♀, 3 juv., Paraburdoo, 100 miles SSW of edge of 4 East
ore body, 24º52'S, 117º40'E (QM W7174); 1 ♂, 1 ♀, Point Salvation, 7 – 8 km WNW, 28º12'S, 123º36'E
(WAM T47709, T65583); 1 ♀, Tallering Peak, 28º06'S, 115º38'E (WAM T54398); 1 ♀, 1 juv., Tanami,
90 km W of Tanami, 19º52'48''S, 128º46'12''E (WAM T70988, T70992); 2 ♀, Tuckanarra, 4.5 km N,
27º08'S, 118º08'E (WAM T47722); 1 ♂, Wanjarri, 53.6 km N of Leinster, 27º26'38''S, 120º47'56''E
(WAM T76483); 1 ♀, Warburton Mission, 26º08'S, 126º35'E (WAM 69/836); 2 ♀, Warburton Ranges,
26º06'S, 126º39'E (WAM 68/511, 71/1434); 1 ♂, Western Australia, no exact locality (WAM T70178); 1
♂, Wharburton, 26º08'S, 126º35'E (WAM 73/179); 7 ♂, 1 ♀, Woodleigh Station, 26º11'44''S,
114º32'14''E (WAM T47713, T65160); 9 ♂, Woodleigh Station, 26º11'45''S, 114º25'24''E (WAM
T65151, T65152); 1 ♂, 1 ♀, Woodleigh Station, 26º13'01''S, 114º35'59''E (WAM T47714, T63254,
T63266, T65155, T65156); 7 ♂, 1 ♀, Woodleigh Station, 26º12'30''S, 114º34'35''E (WAM T47716,
T63267, T65157); 2 ♂, Woodleigh Station, 26º11'31''S, 114º30'33''E (WAM T65153, T65154); 9 ♂, 1 ♀,
1 juv., Woodline, 31º50'S, 122º19'E (WAM T47711, T51561); 1 ♀, Wubin, 30º07'S, 116º36'E (WAM
33/1613); 18 ♂, Yamarna Station, 28º13'30''S, 123º35'30''E (WAM T65580, T65581, T65582, T65584); 3
♂, 1 ♀, Yamarna Station, B-area, 28º13'30''S, 123º35'30''E (WAM 99/188, T47765); 1 ♀, Yandi Station,
27º45'S, 114º48'E (WAM 38/915); 1 ♀, Yandicoogina, 22º47'S, 119º18'E (WAM T47721).
Hoggicosa brennani
NSW: 1 ♀, Bungeema, via Rand, 35º36'S, 146º35'E (AM KS86508); 1 ♀, Combara Siding, Coonamble
Line, 31º08'S, 148º22'E (AM KS86512); 2 ♂, Condobolin, 17.6 km N, 32º57'S, 147º08'E (AM KS7873,
KS7847); 1 ♀, Condobolin, 17 km N, 32º56'S, 147º06'E (AM KS5084); 2 ♂, Gulthul Station, 30 km N of
Euston, 34º11'S, 142º57'E (AM KS57304); 4 ♂, Gulthul Station, near Euston, 34º17'S, 142º53'E (AM
KS57290); 1 ♀, Hermidale, 31º33'S, 146º44'E (AM KS86511); 1 ♀, Lake Cargelligo 19.6 km S, 33º28'S,
146º20'E (AM KS50290); 1 ♂, Lake Cargelligo, 17.6 km S, 33º28'S, 146º20'E (AM KS50291); 4 ♂,
Mallee Cliffs National Park, near Euston, 34º10'45''S, 142º40'15''E (AM KS57292); 1 ♂, Mallee Cliffs
National Park, near Euston, 34º10'S, 142º40'E (AM KS54488); 2 ♀, Merrygoen, 31º50'S, 149º14'E (AM
KS86509); 1 ♀, no exact locality (AM KS84844); 1 ♂, Nymagee, 9 km S, 32º04'S, 146º19'E (AM
KS5726); 1 ♂, Rankins Springs, 33º51'S, 146º16'E (AM KS84047); 1 ♂, Round Hill Nature Reserve,
32º59'20''S, 146º05'06''E (QM S53118); 1 ♀, South Yathon National Park, 32º35'S, 145º24'E (NMV
K8176); 1 ♂, 1 ♀, Yara, 32º51'54''S, 146º11'21''E (AM no reg.); 1 ♂, 1 ♀, Yathong Nature Reserve,
32º35'58''S, 145º32'28''E (AM KS79039, no reg.); Qld: 3 ♀, 3 juv., `Jaffra`, near Texas, 28º51'S,
151º10'E (AM KS8270 KS86507); 1 ♂, 1 ♀, Altonvale and Moombah Station, 40 km W Westmar,
94
27º53'S, 149º23'E (QM S70650); 1 ♂, Inglewood, 28º25'S, 151º04'E (QM S70651); 2 ♀, Morven,
26º25'S, 147º07'E (QM S52226); 1 ♀, Weengallon, 28º22'S, 149º03'E (QM S70648); SA: , no exact
locality (SAM NN18149); 1 ♀, Dudley Conservation Park, Penneshaw PO, 14 km SW, 35º48'S,
137º52'E (SAM NN16463); 2 ♂, Calperum, 33º32'39''S, 140º20'38''E (SAM NN16416-7); 4 ♂, Calperum
Station, Murphys Branchline Tank, 2.25 km SE, 33º37'S, 140º29'E (SAM NN16377-8, NN16379,
NN16382); 2 ♂, Calperum Station, Yabbie Tanks, 4.25 km ESE, 33º36'S, 140º34'E (SAM NN16390-1);
1 ♂, Cape du Couedic, Kangaroo Island, 36º01'S, 136º44'E (SAM NN15264); 1 ♂, Cape Willoughby
Lighthouse, Cape Hart Conservation Park, 4.2 km SW, 35º51'25''S, 138º05'15''E (SAM NN16464); 1 ♂,
Coorong area, 3.3 km W Sth Taunta Homestead, 36º06'55''S, 139º50'55''E (SAM no reg.); 1 ♂, Coorong
area, 4.5 km W Sth Taunta Homestead, 36º07'10''S, 139º50'07''E (SAM no reg.); 1 ♀, 1 juv., Dudley
Conservation Park, 35º48'S, 137º52'E (SAM NN15190); 1 ♂, Dudley Conservation Park, Penneshaw PO,
16 km SE, 35º51'24''S, 137º58'20''E (SAM NN16465); 1 ♂, Edillilie area, 34º25'S, 135º43'E (SAM
NN16245); 3 ♂, Flashjack Dam, 2.3 km N, 33º54'10''S, 140º31'10''E (SAM NN16265-7); 1 ♂, Flashjack
Dam, 7 km SW, 33º56'10''S, 140º27'40''E (SAM NN16264); Frogamerry Dam, 4 km NE, 33º51'20''S,
140º32'10''E (SAM NN16268-9); 1 ♀, Gluepot Station, Gluepot Homestead, 1.9 km N-NNW,
33º44'51''S, 140º07'07''E (SAM NN19093); 1 ♀, Gluepot Station, Gluepot Homestead, 12.7 km W,
33º45'28''S, 139º59'07''E (SAM NN18703); 1 ♀, Gluepot Station, Gluepot Homestead, 9.6 km W-WNW,
33º44'51''S, 140º01'07''E (SAM NN19315); 1 ♂, Hideaway Hut, 10.5 km SW, 33º45'50''S, 140º25'50''E
(SAM NN16263); 1 ♂, Kangaroo Flat, 2 km NW, 35º43'48''S, 139º42'28''E (SAM NN16323); 1 ♂, Karte,
2km SW, 35º04'26''S, 140º40'58''E (SAM NN16313); 1 ♂, Kiawarra, 1.7 km SSE, 35º55'42''S,
137º17'00''E (SAM NN16459); 1 ♂, Marree, 29º39'S, 138º04'E (QM S21352); 1 ♂, Monarto South, 5 km
NE, 35º05'50''S, 139º9'41''E (SAM NN16311); 1 ♀, no exact locality (SAM no reg.); 1 ♂, Paringa, 11 km
NW, 34º08'34''S, 140º54'21''E (SAM NN16312); 1 ♀, Ravine des Casoars, Cape Borda, 35º47'S,
136º34'E (SAM NN15189); 1 ♂, Seal Bay, 5 km N, 35º56'54''S, 137º19'04''E (SAM NN16462); 2 ♂,
Taylorville Station, 20 Mile Dam, 3.5 km W, 34º02'12''S, 140º11'04''E (SAM NN17011-2); 2 ♀,
Taylorville Station, Casuarina Dam, 33º53'10''S, 140º18'32''E (SAM NN17029, NN17049); 1 ♂,
Taylorville Station, Middle Dam, 1.5 km SW, 33º53'10''S, 140º18'32''E (SAM NN17017); Taylorville
Station, Turkey Nest Dam, 4 km SE, 33º56'26''S, 140º9'20''E (SAM NN17046); 1 ♂, The Needles, 1 km
N, 35º49'44''S, 139º22'40''E (SAM NN16314); 2 ♂, Warrinya, 2.3 km SSW, 35º56'14''S, 137º16'51''E
(SAM NN16460-1).
Hoggicosa duracki
WA: 3 ♂, Hope Downs Station, 20º54'S, 118º40'E (WAM T65119); 2 ♂, Karratha Station, 2 km NW,
20º52'34''S, 116º38'50''E (WAM no reg.).
Hoggicosa forresti
SA: 1 ♂, „Parcoola‟, SW of, 33º40'S, 139º59'E (WAM T53489); 1 ♂, Border Village, 31º38'S, 129º00'E
(WAM T56655); 1 ♂, Border Village, 103 km E, 31º38'S, 129º57'E (WAM T62798); 1 ♂, Border
Village, 8 km E, 31º38'S, 129º05'20''E (SAM NN13817); 1 ♂, Border Village, 8 km SE, 31º39'40''S,
129º05'E (SAM NN13816); 1 ♀, Brookfield Conservation Park, 34º22'S, 139º30'E (SAM NN13821); 2
♀, Brookfield Conservation Park, 34º20'S, 139º31'E (SAM NN14133-4); 1 ♀, Clare, N. of (98 Miles N.
of Adelaide), 33º50'S, 138º36'E (WAM 68/863); 1 ♀, Cook, 80 km NW, 29º58'S, 130º01'E (SAM
NN13756); 1 ♀, Eyre Peninsula (no exact location), 33º39'S, 137º11'E (WAM 69/808); 1 ♂, Hambidge,
33º23'S, 135º57'E (SAM NN17007); 2 ♂, 3 ♀, Kimba, S, 33º11'S, 136º33'E (SAM NN13828-9,
NN14135-7); 1 ♂, Kimba, S of, 33º11'S, 136º33'E (QM S70656); 1 ♀, Lake Gilles, 33º05'14''S,
136º36'00''E (SAM NN13818); 1 ♀, Muckera Rockhole, 30º02'S, 130º03'E (SAM NN16994); 1 ♂, 2 ♀,
Poochera, 50 km E, 32º43'S, 135º20'E (SAM NN13825-7); 2 ♀, Weelbubly, Eucla area, 31º37'S,
128º35'E (SAM NN13823); Wirrulla, conservation park NE, 32º23'30''S, 134º48'45''E (SAM no reg.); 1
♀, Yumbarra Conservation Park, Yumbarra Rockhole Track, 31º46'S, 133º29'E (SAM NN13819); WA: 3
♀, Balladonia, 32º27'S, 123º51'E (SAM NN17240-2); 1 ♂, 2 juv., Bungalbin Hill, 30º18'S, 119º43'E
(WAM T47781); 2 ♀, 2 juv., Buningonia Spring, 31º28'10''S, 123º30'00''E (WAM T47773, T47782); 1
♂, Buningonia Spring, 31º26'S, 123º33'E (WAM T53690); 1 ♂, Buningonia Spring (Well), ca. 3 km
NNE of, 31º26'S, 123º33'E (WAM T51400); 1 ♀, Burnabinmah Station, 28º46'35''S, 117º32'50''E (WAM
T55281); 1 ♂, Chook Lake, 29º33'51''S, 123º36'20''E (SAM no reg.); 1 ♀, Cottesloe, 31º59'53''S,
115º45'34''E (WAM 22/5); 1 ♀, Cunderdin Road, 30º38'03''S, 118º29'03''E (WAM T47786); 1 ♀,
Diemal, 1 km W, 29º40'S, 119º18'E (WAM T47770); 1 ♂, Dragon Rocks Nature Reserve, PingaringVarley Road, 32º45'35''S, 119º00'07''E (WAM T47792); 1 ♂, Durokoppin Field Station, 8 km E, Ryans
Property, 31º24'S, 117º46'E (WAM T47399); 1 ♂, Durokoppin Reserve, 31º30'S, 117º44'E (WAM
T62799); 1 ♂, Eucla Motel, 39.5 km WSW, 31º47'S, 128º29'E (WAM T55509); 1 ♂, Exclamation Lake
area, 32º48'S, 121º24'E (WAM T45864); 1 ♂, Gardner Reserve Road, 31º46'45''S, 117º28'22''E (WAM
T62801); 1 ♂, Goongarrie Station, 29º50'15''S, 120º57'36''E (WAM T46060); 1 ♂, Goongarrie Station,
29º58'06''S, 121º01'30''E (WAM T46059); 2 ♂, Grass Patch, 'Sieda', 33º13'56''S, 121º46'00''E (WAM
95
T53581, T70269); 2 ♂, Grass Patch, 'Sieda', Fitzgerald Locality 41, 33º14'S, 121º43'E (WAM T53486,
T62466); 1 ♂, Grass Patch, 'Sieda', Fitzgerald Locality 41, 33º13'56''S, 121º46'00''E (WAM T62797); 3
♂, Helena-Aurora Ranges, 30º24'S, 119º38'E (WAM T47763, T47764, T47767); 1 ♂, Kalgarrin National
Park, S, 32º30'05''S, 118º33'39''E (WAM T48019); 1 ♀, Kalgoorlie, 30º45'S, 121º27'E (WAM T47768); 1
♂, Kalgoorlie, 50 km NE, Black Swan Nickel Mine, 30º23'57''S, 121º40'42''E (WAM T56888); 1 ♂,
Kellerberrin, 10 km NW, McClelands property, 31º34'S, 117º45'E (WAM T46094); 1 ♀, Lake Cronin,
32º24'S, 119º45'E (WAM T47772); 1 ♂, Lake Cronin, 32º22'S, 119º49'E (WAM T47777); 1 ♀, Lake
Cronin, 32º23'00''S, 119º45'10''E (WAM T47779); 1 ♂, Lake Cronin, 32º22'15''S, 119º49'30''E (WAM
T47771); 1 ♂, Lake Goorly, 29º49'50''S, 116º57'19''E (WAM T47791); 1 ♂, Lake Gulson Nature
Reserve, 32º45'59''S, 119º24'12''E (WAM T48083); 1 ♂, Lake Magenta Nature Reserve, 33º40'37''S,
119º04'52''E (WAM T63278); 1 ♂, Lake Mollerin Station, 30º31'47''S, 117º34'45''E (WAM T47789); 4
♂, 1 juv., Laverton, 39 km E, 28º28'S, 122º50'E (WAM T55571, T55587, T62380); 1 ♂, Lorna Glen
Station, 26º15'24''S, 121º29'52''E (WAM T65610); 2 ♂, Minniberri, Norrish's property, 3 km W. of Kodj
Kodjin on Minniberri Road, 31º15'S, 117º52'E (WAM T62800); 1 ♀, Moorine Rock, 8 miles W, 31º18'S,
119º00'E (WAM 70/44b); 1 ♀, Mt Kokeby, 32º13'S, 116º58'E (WAM T63280); 1 ♂, Mt Ragged, NE of,
33º13'17''S, 123º38'47''E (WAM T46098); 1 ♂, Mullamullang Cave area, 31º45'S, 127º14'E (AM
exKS50234); 1 ♂, 1 ♀, Mundrabilla Homestead, Tampanna Cave, campsite nearby, ca. 30km N of Eyre
Highway, 31º42'S, 127º40'E (WAM 91/919-20); 1 ♂, Mungarine Nature Reserve North, Beacon,
30º19'51''S, 117º45'12''E (WAM T47787); 1 ♂, Newdegate, 20 km NE, 32º50'S, 119º20'E (WAM
T58343); 1 ♂, 1 ♀, North Baandee Nature Reserve, 31º38'S, 117º43'E (WAM T47762); 1 ♀, Nullarbor
Camp 5, ca. 90 km N of Loongana, 30º07'18''S, 126º53'01''E (WAM T47766); 1 ♂, Point Salvation, 7 – 8
km WNW, 28º12'S, 123º36'E (WAM T62387); 1 ♂, Roe Plain, 32º04'23''S, 126º30'38''E (WAM
T56395); 1 ♂, Shire Reserve, 11 km E of Latham, 29º44'10''S, 116º33'43''E (WAM T47790); 1 ♂,
Tardun, 28º42'S, 115º42'E (WAM T62451); 1 ♂, Vermin Proof Fence West, E Beacon, 30º14'14''S,
118º18'9''E (WAM T47793); 1 ♂, 1 juv., Warrachuppin North Road, 31º00'06''S, 118º41'31''E (WAM
T47788); 1 ♀, Westonia, 31º18'S, 118º41'E (WAM T70267); 1 ♀, Wialki, Arnold's farm, 30º29'S,
118º07'E (WAM 69/39); 3 ♂, 1 ♀, Woodline, 31º55'S, 122º24'E (QM S70646, S70655, S70657, WAM
T47774); 1 ♀, Wubin, 30º06'S, 116º37'E (WAM T56591); 1 ♂, Yundamindra, 29º15'S, 122º06'E (WAM
T47775); 1 ♂, Zanthus, 4 km W, 30º48'S, 124º00'E (WAM T47769).
Hoggicosa natashae
NSW: 1 ♀, Fowlers Gap Research Station, 75 km N of Broken Hill, 31º05'S, 141º44'E (AM KS64942);
SA: 1 ♀, Cooper Creek, 28º23'S, 137º41'E (SAM NN020); 1 ♀, Lake Gilles, 32º43'S, 136º47'E (SAM
NN13801); 2 ♀, Lake Gilles, 32º41'20''S, 136º55'20''E (SAM NN14785, NN14786); 2 ♀, 1 juv., Wilson,
4 km S, 28º08'S, 141º53'E (QM S21417).
Hoggicosa snelli
WA: 2 ♂, Barrow Island, 20º47'S, 115º24'E (WAM T57698, T57697); 1 ♂, Bidgemia Station, Gasgoyne
Junction, 25º05'17''S, 115º22'48''E (WAM T65147); 2 ♂, Drysdale River Station, 15º42'S, 126º23'E
(WAM T56397); 1 ♀, Gascoyne Junction, 25º03'S, 115º12'E (WAM T51556); 8 ♂, Kennedy Range
National Park, 24º33'04''S, 114º57'32''E (WAM T62805, T65149); 4 ♂, Mardathuna Station, 24º26'36''S,
114º30'42''E (WAM T62804); 4 ♂, Mardathuna Station, 24º30'41''S, 114º38'14''E (WAM T65126,
T65148); 4 juv., Marilla Station, 22º58'S, 114º28'E (QM W4022); 1 ♂, Meedo Station, 25º40'49''S,
114º37'20''E (WAM T65159); 2 ♂, Meedo Station, 25º39'13''S, 114º37'38''E (WAM T65130); 6 ♂, 1 ♀,
Meedo Station, 25º37'23''S, 114º41'40''E (WAM T65132); 1 ♂, Meedo Station, 25º37'31''S, 114º42'19''E
(WAM T65131); 2 ♀, 1 juv., Mt Gibson, camp near, 29º35'S, 117º11'E (WAM T53871); 1 ♀, Munda
Station, 20º30'S, 118º03'E (WAM T53870); 3 ♀, 1 juv., Paraburdoo, 4 km W of '4 East' ord body,
23º12'S, 117º40'E (QM W7173); 1 ♀, Shothole Canyon, Cape Range National Park, 22º02'41''S,
114º20'14''E (WAM T47612); 1 ♂, Tanami, 90 km W of Tanami, 19º52'00''S, 128º50'46''E (WAM
T70975); 1 ♂, Tanami, 92 km W of Tanami, 19º53'59''S, 128º49'37''E (WAM T70978); 1 ♂, Telfer,
21º43'S, 122º14'E (WAM T62806); 11 ♂, Woodleigh Station, 26º11'45''S, 114º25'24''E (WAM T65133,
T65134, T65146);
Hoggicosa storri
WA: 1 ♂, Ajana Back Road, 27º59'57''S, 114º37'55''E (WAM T63252); 1 ♀, Boddington, SW of,
Worsley Alumina, Overland Conveyor Belt (conveyor #1), line stand 580, 32º58'S, 116º25'E (WAM
T71701); 1 ♂, Booanya, 32º45'S, 123º36'E (NMV K8251); 1 ♀, Bullfinch, 50 km N of, 30º20'S, 119º07'E
(WAM T53616); 1 ♀, Bullock Holes Tribes Reserve, eastern boundary, 30º31'S, 121º51'E (WAM
T62764); 1 ♂, Bungalbin Hill, 30º17'S, 119º43'E (WAM T48005); 1 ♀, Burnabinmah Station,
28º46'35''S, 117º32'50''E (WAM T55282); 6 ♂, 1 ♀, Caiguna, ca. 21 km E, ca. 1.1 km S Eyre Hwy,
96
32º10'52''S, 125º40'49''E (WAM T47733, T47734, T47737, T47736, T47735, T47738); 1 ♀, Coolgardie,
103 miles W, 30º57'S, 119º25'E (WAM 69/887); 1 ♀, Coolgardie, 20 km W, 30º57'S, 119º55'E (WAM
T51235); 1 ♀, Diemal, 1 km W, 29º40'S, 119º18'E (WAM T47798); 1 ♂, Dongolocking Nature Reserve,
33º04'38''S, 117º41'44''E (WAM T62776); 2 ♂, Earoo Park, 8 km ENE, 29º31'S, 118º24'E (WAM
T47796, T47794); 1 ♀, Eucla Motel, 39 km WSW, 31º04'S, 128º29'E (WAM T55505); 1 ♂, 1 juv.,
Goongarrie Station, 30º05'50''S, 121º10'24''E (WAM T46064);1 ♂, Goongarrie Station, 30º02'39''S,
120º55'16''E (WAM T48015); 1 ♂, Goongarrie Station, 30º01'54''S, 120º54'57''E (WAM T46065); 1 ♂,
Grass Patch Wheat Bin, 33º14'S, 121º43'E (WAM T48014); 1 ♂, Grass Patch, 'Seida', 33º13'56''S,
121º46'00''E (WAM T70270); 2 ♂, 1 ♀, Grass Patch, 'Sieda', Fitzgerald Locality 41, 33º14'S, 121º43'E
(WAM T48013, T62477, T47712); 1 ♀, Jibbering Well, 29º53'S, 116º49'E (WAM 71/873); 1 ♀, John
Forrest National Park, 31º53'S, 116º05'E (WAM T48016); 1 ♂, Jundee, 8.5 km SSE of Jundee
homestead, 26º25'16''S, 120º40'45''E (WAM T70266); 2 ♂, Kalgoorlie, 50 km NE, Black Swan Nickel
Mine, 30º23'54''S, 121º40'53''E (WAM T53921); 2 ♂, 1 ♀, Kalgoorlie, 50 km NE, Black Swan Nickel
Mine, 30º23'07''S, 121º38'59''E (WAM T53251, T53252); 2 ♂, 1 ♀, Kalgoorlie, 50 km NE, Black Swan
Nickel Mine, 30º23'05''S, 121º38'41''E (WAM T53212, T53268); 1 ♂, Kalgoorlie, 50 km NE, Black
Swan Nickel Mine, 30º23'56''S, 121º41'06''E (WAM T56962); 1 ♀, Kalgoorlie, 50 km NE, Black Swan
Nickel Mine, 30º23'57''S, 121º40'42''E (WAM T56887); 1 ♂, 1 ♀, Kalgoorlie, 50 km NE, Black Swan
Nickel Mine, 30º24'02''S, 121º40'59''E (WAM T56943, T56940); 1 ♂, Kalgoorlie, 50 km NE, Black
Swan Nickel Mine, 30º23'25''S, 121º38'51''E (WAM T56831); 2 ♂, Kalgoorlie, 50 km NE, Black Swan
Nickel Mine, 30º23'22''S, 121º39'03''E (WAM T53203); 3 ♂, Kalgoorlie, 50 km NE, Black Swan Nickel
Mine, 30º23'29''S, 121º39'10''E (WAM T53319); 1 ♂, Kambalda, ca. 15 km SW, 31º12'58''S,
121º27'23''E (WAM T56551); 1 ♀, Koorda, 30º49'S, 117º29'E (SAM NN17314); 1 ♂, Kundip,
Ravensthorpe, 33º40'56''S, 120º11'57''E (WAM T69836); 1 ♂, Kundip, Ravensthorpe, 33º40'28''S,
120º11'49''E (WAM T69835); 1 ♂, Kundip, Ravensthorpe, 33º40'04''S, 120º12'07''E (WAM T69834); 1
♂, Kundip, Ravensthorpe, 33º40'50''S, 120º11'37''E (WAM T69831); 1 ♀, Lake Cronin, 33º22'57''S,
119º45'06''E (WAM T74411); 1 ♀, Lake Cronin, 32º23'S, 119º45'E (WAM T48003); 1 ♀, Lake Gilmore,
55 km S Norseman, 32º37'S, 121º36'E (SAM NN17313); 1 ♂, Lake Goorly, 29º49'50''S, 116º57'19''E
(WAM T62786); 2 ♂, Lake Magenta Nature Reserve, 33º40'37''S, 119º04'52''E (WAM T62778); 1 ♂,
Leinster, 75 km N of, 27º26'S, 120º22'E (WAM T66979); 1 ♂, Little Sandy Desert, 10.8 km NNE of
Kulonoski East Well, 24º35'23''S, 120º15'41''E (WAM T62773); 1 ♂, 1 ♀, Lord Nelson, 10.15 km SSW
of Black Hill, 28º9'26''S, 119º30'56''E (WAM T63356, T63347); 2 ♂, Lord Nelson, 10.3 km SSW of
Black Hill, 28º9'23''S, 119º30'27''E (WAM T63351, T63353); 1 ♂, Lord Nelson, 10.4 km SSW of Black
Hill, 28º9'43''S, 119º31'31''E (WAM T63349); 4 ♂, Lord Nelson, 11.4 km SSW of Black Hill,
28º10'06''S, 119º30'45''E (WAM T63352, T63350, T63348, T63355); 1 ♀, Lorna Glen Station,
26º09'55''S, 121º06'00''E (WAM T70281); 1 ♂, Lorna Glen Station, 26º11'59''S, 121º15'59''E (WAM
T70277); 1 ♀, Lorna Glen Station, 26º01'56''S, 121º33'36''E (WAM T65374); 2 ♂, Lorna Glen Station,
26º02'39''S, 121º26'48''E (WAM T66467); 1 ♂, Lorna Glen Station, 26º06'46''S, 121º30'15''E (WAM
T64773); 2 ♂, Lorna Glen Station, 26º17'50''S, 121º33'08''E (WAM T64720, T66400); 1 ♂, Lorna Glen
Station, 26º16'27''S, 121º33'35''E (WAM T64857); 1 ♂, Lorna Glen Station, 26º02'39''S, 121º26'48''E
(WAM T64754); 2 ♂, Lorna Glen Station, 26º18'13''S, 121º33'46''E (WAM T64927, T66848); 2 ♂,
Lorna Glen Station, 26º15'46''S, 121º30'40''E (WAM T66398); 4 ♂, Lorna Glen Station, 26º12'10''S,
121º22'32''E (WAM T64629, T53915, T66978); 4 ♂, Lorna Glen Station, 26º18'11''S, 121º28'31''E
(WAM T53916, T66442, T53912); 2 ♂, Lorna Glen Station, 26º07'49''S, 121º31'02''E (WAM T66410); 1
♂, Lorna Glen Station, 26º00'05''S, 121º33'48''E (WAM T53914); 1 ♀, Maya, E, 29º52'S, 116º30'E
(WAM T53617); 1 ♀, Merredin, 31º29'S, 118º17'E (WAM T44325); 1 ♀, Mollerin, 30º24'S, 117º31'E
(WAM T47800); 1 ♀, Morgan Range, 25º55'52''S, 128º56'59''E (WAM T79146); 1 ♂, Mt Dean, N,
33º13'14''S, 123º38'48''E (WAM T62802); 1 ♂, Mt Gibson Station, 29º36'24''S, 117º24'38''E (WAM
T46037); 1 ♂, Mt Gibson Station, 29º36'11''S, 117º24'20''E (WAM T46039); 1 ♂, Mt Gibson Station,
29º36'18''S, 117º24'30''E (WAM T46038); 2 ♂, Mt Gibson Station, 29º45'29''S, 117º19'07''E (WAM
T46042); 1 ♂, Mt Gibson Station, 29º40'52''S, 117º28'02''E (WAM T48046); 4 ♂, 2 juv., Mt Gibson
Station, 29º36'37''S, 117º24'36''E (WAM T46040); 1 ♂, Mt Gibson Station, 29º41'53''S, 117º24'21''E
(WAM T46043); 1 ♂, Mt Jackson, 30º15'S, 119º15'E (WAM T48025); 1 ♂, Mt Keith mine, 10 km NE.
of Mount Keith homestead, 27º12'29''S, 120º34'24''E (WAM T74660); 1 ♂, Mt Keith mine, 14.8 km E. of
Lake Way homestead, 26º58'9''S, 120º36'53''E (WAM T74657); 1 ♂, Mt Keith mine, 14 km ESE. of Lake
Way homestead, 26º58'9''S, 120º36'53''E (WAM T74654); 1 ♂, Mt Keith mine, 18.7 km E. of Mount
Keith homestead, 27º14'54''S, 120º41'48''E (WAM T74655); 1 ♂, Mt Keith mine, 21.6 km E. of Lake
Way homestead, 26º58'53''S, 120º40'57''E (WAM T74656); 4 ♂, Mt Keith mine, 22.5 km SE. of Lake
Way Homestead, 27º06'17''S, 120º36'21''E (WAM T72734, T74658, T74661, T74659); 1 ♂, Mullewa
Airstrip, 28º28'37''S, 115º30'20''E (WAM T63251); 1 ♀, Mundaring, 31º53'S, 116º10'E (WAM T48001);
1 ♀, Narrogin, Lyon Banks, 32º56'S, 117º11'E (WAM 36/5044); 1 ♀, Nimary, ca. 40 km NE Wiluna,
26º20'S, 120º38'E (WAM T48017); 1 ♂, no exact locality (WAM T63250); 1 ♂, 1 ♀, no locality on label,
(WAM T48009); 1 ♀, no locality on label, (WAM 69/889); 1 ♀, Pickering Brook, 31º59'S, 116º11'E
97
(WAM 99/192); 1 ♀, Scaddan, 33º27'S, 121º44'E (WAM 30/921); 1 ♂, Stirling Range Caravan Park,
34º18'55''S, 118º11'14''E (WAM T62803); 1 ♀, Stoneville, 30º52'S, 116º10'E (WAM T47797); 1 ♀,
Walk-Walkin, around, via Koorda, 30º49'S, 117º19'E (WAM 40/1100); 2 ♀, Walliston, 31º59'S, 116º04'E
(WAM T48012, T47799); 1 ♀, Walyahmoning Rock, 2 miles SW, 30º39'S, 118º44'E (WAM 74/1467); 1
♂, Wandana Reserve, 28º19'S, 115º9'E (WAM T47795); 1 ♂, Wanjarri, 50.3 km N of Leinster,
27º28'47''S, 120º49'27''E (WAM T76481); 1 ♀, Warburton Ranges Mission, 26º08'S, 126º35'E (WAM
74/1465); 1 ♀, Western Australia, no exact locality (NMV K8252); 1 ♀, Westonia, 15 km NW, 31º11'S,
118º46'E (WAM T66893); 1 ♂, 1 ♀, Wiluna, 26º34'13''S, 120º00'43''E (SAM NN16660-1); 1 ♀, 1 juv.,
Woodline, 31º57'S, 122º24'E (WAM T48002); 1 ♂, Wooraloo, no exact locality (WAM no reg.); 1 ♂,
Worsley Alumina, Overland Conveyor Belt, start of Conveyor (tail end), SW of Boddington, 32º48'S,
116º28'E (WAM T58323); 1 ♀, Wubin, 32 miles NE, Great Northern Highway, 30º07'S, 116º38'E (WAM
68/503); 1 ♀, Wydgee Homestead, 17 km at 125deg, 28º56'S, 117º58'E (WAM T53749); 1 ♀, Yarloop,
32º58'S, 115º54'E (WAM 24/604); 1 ♂, Yellowdine, 38 miles S, 31º51'S, 119º39'E (WAM T53406); 1 ♂,
Yuinmery, 28º31'55''S, 119º11'35''E (WAM T62775); 1 ♂, Yuinmery, 28º33'25''S, 119º05'30''E (WAM
T48006); 1 ♂, Yuinmery, 28º32'00''S, 119º05'45''E (WAM T62781); 9 ♂, Yundamindra, 29º15'S,
122º06'E (WAM T48008, T56589, 90/568-9, T48010, T48004, T48011).
Hoggicosa wolodymyri
NSW: 1 ♀, 16km W of Euabalong West, 33º03'S, 146º24'E (AM KS44770); 1 ♂, Pulletop, 33º58'46''S,
146º03'28''E (QM S53673); 1 ♂, Round Hill, near Euabalong, 32º58'S, 146º9'E (AM KS8307); 6 ♂,
Warrakoo Station, Lower Murray Darling region, 33º56'44''S, 141º08'13''E (AM KS72675); 1 ♂,
Warrakoo Station, Lower Murray-Darling region, 33º51'16''S, 141º07'06''E (AM KS66843); 1 ♂, Yara,
32º56'48''S, 146º11'32''E (AM exVWF19129); NT: 1 ♂, Uluru National Park, ~6 km S of ranger station,
25º24'03''S, 130º59'18''E (AM KS63728); SA: 1 ♂, Adelaide & Pearson Island, between, no exact
locality (SAM NN16231); 2 ♂, Balah, 7 km SE, 33º46'40''S, 139º49'00''E (SAM NN16282-3); 1 ♀, 1
juv., Bindyi Research Station, Koonamore, 32º07'S, 139º21'E (SAM NN15295); 2 ♂, 2 juv., Brooks
Bore, 0.8 km W, 32º59'20''S, 140º54'30''E (SAM NN16285-6); 1 ♂, Bullock Dam, 7.6 km NNE,
33º21'20''S, 139º43'40''E (SAM NN16284); 2 ♂, Calperum Station, Murphys Branchline Tank, 2.25 km
SE, 33º37'S, 140º29'E (SAM NN16380-1); 1 ♂, Calperum Station, Yabbie Tanks, 2.25 km NE, 33º36'S,
140º34'E (SAM NN16387); 3 ♂, Calperum Station, Yabbie Tanks, 4.25 km ESE, 33º36'S, 140º34'E
(SAM NN16392-4); 2 ♂, Catalogue Dam, 2.7 km N, 33º46'20''S, 140º43'40''E (SAM NN16280-1); 1 ♂,
Corrobinnie Hill, 1.2 km SSE, 32º59'33''S, 135º44'39''E (SAM no reg.); 1 ♀, Danggali Conservation
Park, Tomahawk Dam, 8 km S, 33º24'46''S, 140º43'E (SAM NN17072); 1 ♂, Emu, 4 km NW, 28º38'S,
132º10'E (SAM NN15271); 2 ♂, Flashjack Dam, 2.3 km N, 33º54'10''S, 140º31'10''E (SAM NN16271-2);
5 ♂, Flashjack Dam, 7 km SW, 33º56'10''S, 140º27'40''E (SAM NN16275-9); 1 ♂, Frogamerry Dam, 4
km NE, 33º51'20''S, 140º32'10''E (SAM NN16270); 1 ♀, Gluepot Station, Gluepot Homestead, 1.5 km EENE, 33º45'50''S, 140º08'15''E (SAM NN19055); 1 ♀, Gluepot Station, Gluepot Homestead, 11.3 km W,
33º45'16''S, 139º59'58''E (SAM NN18702); 1 ♂, Gluepot Station, Gluepot Homestead, 4.7 km N,
33º43'23''S, 140º07'26''E (SAM NN18802); 1 ♂, Gluepot Station, Gluepot Homestead, 6.8 km N,
33º42'9''S, 140º07'16''E (SAM NN18748); 1 ♂, 2 ♀, Gluepot Station, Gluepot Homestead, 8.5 km WWNW, 33º44'49''S, 140º01'56''E (SAM NN18416, NN18698, NN18732); 1 ♀, Gluepot Station, Gypsum
Dam, 33º46'19''S, 140º04'07''E (SAM NN18410); 1 ♂, Great Victoria Desert, 27º52'S, 130º22'E (SAM
NN15270); 5 ♂, Hamilton Homestead, 13.2 km S, 26º50'03''S, 135º04'01''E (SAM NN15943-7); 1 ♂,
Hamilton Homestead, 24.4 km SSE, 26º54'22''S, 135º11'46''E (SAM NN15948); 1 ♂, Hamilton
Homestead, 6.8 km SE, 26º45'43''S, 135º07'08''E (SAM NN15949); 2 ♂, Hideaway Hut, 10.5 km SW,
33º45'50''S, 140º25'50''E (SAM NN16273-4); 1 ♂, Immarna Siding, 10.4 km S, 30º34'46''S, 132º12'27''E
(SAM NN15289); 2 ♂, Ketchalby Rockhole, 3.4 km W, 32º32'37''S, 134º58'59''E (SAM no reg.); 2 ♂,
Kunytjanu, 8 km NW, 26º36'45''S, 129º18'50''E (SAM NN11182-3); 1 ♀, Lake Gilles National Park,
33º03'S, 136º40'E (SAM NN15285); 1 ♂, Lambina Homestead, 43.7 km N, 26º31'00''S, 134º05'18''E
(SAM NN15942); 1 ♂, Mabel Creek Homestead, 30 km SW, 29º10'30''S, 134º06'30''E (SAM NN15290);
1 ♂, Monash, 34º14'S, 140º33'E (SAM NN14776); 1 ♂, Mootatunga, 4 km S, 34º59'16''S, 140º50'16''E
(SAM NN16322); 2 ♂, Mootatunga, 4 km S, 34º59'9''S, 140º50'9''E (SAM NN16320-1); 1 ♀, Mt Finke, 8
km E, 30º55'S, 134º00'E (SAM NN15280); 8 ♂, Mt Hoare, 3 km WSW, 27º03'51''S, 129º40'16''E (SAM
no reg.); 2 ♀, Mt Hoare, 6 km W, 27º03'23''S, 129º38'20''E (SAM no reg.); 3 ♂, Muckera Rockhole,
30º02'S, 130º03'E (SAM NN16999, NN17000, NN17002); 1 ♂, North east of OTC Station, Ceduna,
31º52'S, 133º49'E (SAM NN15284); 1 ♀, Oakbore Station, 33º42'07''S, 140º35'06''E (SAM no reg.); 3 ♀,
OTC Station, E of, Cenduna, 31º52'S, 133º49'E (SAM NN15281-3); 1 ♂, Paney Station shearer's
quarters, 32º44'20''S, 135º42'00''E (SAM no reg.); 1 ♂, Paney Station shearer's quarters, 2.6 km SW,
32º39'46''S, 135º37'9''E (SAM no reg.); 3 ♂, Pooginook Conservation Park, 34º05'S, 140º06'E (SAM
NN15291-3); 5 ♂, Tallaringa Conservation Park, Tallaringa Well, 10 km NE, 29º01'S, 133º25'E (SAM
NN15265-9); 1 ♂, Tallaringa Conservation Park, Tallaringa Well, 2.7 km W, 29º01'S, 133º16'E (SAM
NN15272); 1 ♂, 1 ♀, Taylorville Station, 34º06'S, 139º58'E (SAM NN16408, NN16409); 5 ♂,
98
Taylorville Station, 17 Mile Dam, 3.5 km W, 34º02'12''S, 140º11'04''E (SAM NN17033-7); 9 ♂,
Taylorville Station, 18 Mile Dam, 3.5 km W, 34º02'12''S, 140º11'04''E (SAM NN17020-8); 1 ♀,
Taylorville Station, Casuarina Dam, 33º53'10''S, 140º18'32''E (SAM NN17053); 1 ♀, Taylorville Station,
Casuarina Dam, 33º53'10''S, 140º18'32''E (SAM NN17030); 4 ♂, Taylorville Station, Crows Nest Dam,
4.5 km ENE, 33º58'S, 140º11'10''E (SAM NN17042-5); 1 ♂, Taylorville Station, Middle Dam, 1.5 km
SW, 33º54'37''S, 140º12'20''E (SAM no reg.); 2 ♂, Taylorville Station, Middle Dam, 1.5 km SW,
33º53'10''S, 140º18'32''E (SAM NN17018-9); 2 ♂, Taylorville Station, Mile Dam, 3.5 km W 10,
34º02'11''S, 140º11'03''E (SAM no reg.); 1 ♀, Taylorville Station, near Casuarina Dam, 33º53'10''S,
140º18'32''E (SAM no reg.); 1 ♀, Waikerie, nr Holiday House, 34º12'44''S, 140º00'30''E (SAM
NN15294); 1 ♂, Wendale, 2 km SE, 34º43'33''S, 140º18'14''E (SAM NN16319); 2 ♀, Wirrulla,
conservation park NE, 32º23'20''S, 134º48'45''E (SAM no reg.); 1 ♂, Yumbarra Conservation Park, Inila
Rockwaters, 1.5 km S, 31º47'42''S, 133º25'44''E (SAM NN15287); 1 ♂, Yumbarra Conservation Park,
Inila Rockwaters, 7 km W, 31º47'26''S, 133º20'58''E (SAM NN15288); 1 ♂, Yumbarra Conservation
Park, Inila Rockwaters, 7 km W, 31º48'14''S, 133º24'05''E (SAM NN15286); 4 ♀, 1 juv., Yumbarra
Conservation Park, Yumbarra camp, SW corner along dog fence, 31º39'S, 133º22'E (SAM NN15278-9,
NN15276-7); 3 ♂, Yumbarra Conservation Park, Yumbarra Rockhole track, 31º39'S, 133º22'E (SAM
NN15273-5); WA: 1 ♂, Goongarrie Station, 29º56'44''S, 121º07'14''E (WAM T55374); 1 ♂, Mulga
Rock, 29º53'27''S, 123º36'51''E (SAM NN22290); 8 ♂, Queen Victoria Springs Nature Reserve, 30º14'S,
123º41'E (WAM T49265, T49292, T52354, T52408, T52444, T52506, T52527).
99
Summary of Section I
In this first section I revised the taxonomy of the „bicolor group‟ of Australian wolf
spiders and provided strong phylogenetic evidence that they represent a distinct
Australian genus. According to the Rules of the International Code of Zoological
Nomenclature (International Commission of Zoological Nomenclature 1999),
Hoggicosa Roewer, 1960 represents the valid name for this genus. A systematic
analysis based on morphological characters supported the monophyly of Hoggicosa
based on a synapomorphy of the female genitalia. In addition, the combination of two
characters depicting the cymbium spines of males provided a second synapomorphy.
Prior to my study, spiders in this genus were incorrectly assigned to the putative
Mediterranean genus Lycosa. My work has resulted in transferring nearly a third of the
Australian species currently placed within Lycosa to Hoggicosa. As well as redescribing
and relimiting species boundaries for the six species named prior to my work, I have
also described four new Hoggicosa species. Future workers could use molecular data to
test independently the species boundaries and phylogenetic hypothesis proposed here.
Hoggicosa provide ideal model species for further ecological and evolutionary studies,
being large, widespread within the arid zone of Australia, often very common and
conspicuous, particularly the females of species with unusual sexual colour
dimorphism.
The fascinating colour dimorphism displayed between the sexes of four species of
Hoggicosa, with females more colourful than males, begs further investigation. Indeed,
spiders are ideal animals for the study of sperm competition and cryptic female choice
(Eberhard 2004). What selection pressure, either sexual or natural, has driven this
dimorphism remains unclear and the current lack of basic information on natural history
and mating system (i.e. multiple mating and sperm priority pattern) for most species is a
limiting factor for interpreting this unusual evolutionary phenomenon. Now that the
species within Hoggicosa are named and identifiable, this should allow the rapid
accumulation of natural history information and raise interest in the study of their
evolutionary history.
Along with their burrowing behaviour, which made them suitable for a detailed
population study, one of the initial reasons I chose to work on the „bicolor group‟ was
their large size. This meant that they would be easier to handle in ecological studies, but
100
also that their genitalia were easily visible under a light stereomicroscope. However, the
palps and epigynes of wolf spiders are morphologically conservative, which made the
identification of species more difficult than expected. The terminal apophysis, pars
pendula and tegular apophysis of the male pedipalp proved the most useful
discriminators for males. In contrast, body colour was a key distinguishing character for
females.
References
Eberhard, W. G. (2004) Why study spider sex: special traits of spiders facilitate studies
of sperm competition and cryptic female choice. Journal of Arachnology, 32,
545-556.
International Commission of Zoological Nomenclature. (1999) International Code of
Zoological Nomenclature. Fourth Edition, The International Trust for
Zoological Nomenclature 1999 (c/o The Natural History Museum, London).
101
SECTION II: ECOLOGY
SECTION II: ECOLOGY
General Introduction
Spinifex grasslands are a dominant habitat in Australia, covering over 25% of the
continent (Allan and Southgate 2002). Spinifex is a common name used to describe
over 64 species of perennial hummock grasses within the subtribe Triodiinae (Lazarides
1997). These species are characterized by a distinctive, drought-adapted leaf anatomy,
in which the leaves form thin blades or spines, that are often prickly and resinous
(Lazarides 1997). Their dry, resinous leaves and growth form produce large, air-filled
clumps or hummocks, that create an ideal fuel (Pianka 1989, Burrows et al. 1991).
Spinifex is therefore highly flammable, and large areas (> 10 000 km2) burn frequently
due to lightning strikes and human ignition (Allan and Southgate 2002, Turner et al.
2008). Fire plays an integral part in ecosystem processes, providing one of the main
sources of nutrient cycling, given the high aridity and slow decomposition rates (Griffin
and Friedel 1985, Stafford Smith and Morton 1990). Fire was an important tool for
aboriginal inhabitants and extensively used in the past (Jones 1969, Gould 1971;
Kimber 1983, Bird et al. 2004, 2005). Since the arrival of Europeans, aboriginal
occupation of arid Australia has changed and with it, the fire regime has been altered
(Bowman 1998, Burrows et al. 2006; Bird et al. 2008). For the western desert region
these changes occurred rapidly during the 1950s and 60s due to forced relocations to
clear land for missile and nuclear weapons testing (Bird et al. 2008).
This has led to great interest in how the flora and fauna of spinifex grasslands respond
to disturbance by fire. Many studies have examined the response of vegetation
(Burbidge 1943, Griffin and Friedel 1984 a, b, Westoby et al. 1988, Bogusiak et al.
1990, Griffin 1992, Rice and Westoby 1999) and vertebrate fauna (Masters 1993, 1996,
Southgate and Master 1996, Letnic 2003, Letnic et al. 2004, Letnic and Dickman 2005).
For small mammals, the current level of knowledge has reached a stage that allows the
development of detailed state and transition models (Letnic and Dickman in press).
However, only a handful of studies have examined the response of invertebrates to fire
in arid Australia (Smith and Morton 1990, Gunawardene and Majer 2005, Barrow et al.
2007), and only one has examined the response of spiders (Langlands et al. 2006). I set
out to examine the response of spiders to disturbance by fire in a spinifex grassland in
Western Australia. I was interested in the long-term pattern in the assemblage of spiders
as a whole.
102
Specifically, I had three main research questions:
1) Is there a successional pattern following disturbance by fire?
2) If so, which variables best explain this post-fire successional pattern?
3) To what extent the post-fire response of spiders can be predicted?
Given the limited time available for a Ph.D. project, I sought to address these questions
of long-term pattern (up to 20 years post-fire) using a chronosequence study. I recognise
that the chronosequence approach carries with it a number of limitations and
assumptions, and these caveats need to be acknowledged when interpreting results.
Each of the following chapters focuses on one of these questions.
In the second chapter of this thesis, I assess the changes in abundance, species richness,
evenness and species composition of spiders with post-fire age. Previous work
demonstrated changes within all these parameters following disturbance by fire for
assemblages of spiders in other habitats, including eucalypt and boreal forests (Huhta
1971, Riechert and Reeder 1972, Merrett 1976, Strehlow 1993, York 1999, Buddle et
al. 2000, 2006, Andersen and Mueller 2000, Moretti et al. 2002, Niwa and Peck 2002,
Abbott et al. 2003, Larrivée et al. 2005, Brennan et al. 2006, Langlands et al. 2006,
Gillette et al. 2008). Therefore, while I expected to find significant differences among
post-fire ages, I was particularly interested in the successional trajectory. Does the
assemblage return to a long-unburnt state (deterministic) or are post-fire changes largely
stochastic? To help describe the successional trajectory post-fire I follow the definitions
of Westman (1978). Westman defined resilience as “the ability of a natural ecosystem
to restore its structure following acute or chronic disturbance”. As one of the
characteristics of resilience he described the ability of an assemblage to resist change as
inertia (Westman 1978).
Having found successional changes following fire, in the third chapter of this thesis I
assessed the factors that might potentially explain these differences. The strong
influence of fire and rainfall on vertebrates in arid Australia is well established (Masters
1993, 1996, Southgate and Masters 1996, Letnic 2003, Letnic et al. 2004, Letnic and
Dickman 2005). Detecting fire effects on beetles in Australian savannas is contingent
on rainfall (Blanche et al. 2001), and previous work on spiders in the arid zone has
suggested rainfall as a key variable (Langlands et al. 2006). Therefore, recorded
detailed rainfall measurements by installing electronic tipping bucket rain gauges at or
near all sites. I also measured other explanatory factors that can influence spiders, such
103
as habitat structure, species composition of plants (floristics), soil and predators. In
addition, it was important to acknowledge that the spatial arrangement of sites in
relation to each other can influence the fauna. I was particularly interested in
quantifying the influence that each of these may have by examining the unique and
shared amounts of variation in the spiders explained by each type of variable.
Finally, given the insights gained from the previous two chapters, I tested if the post-fire
response of spiders could become more predictive, rather than simply identifying
repeating patterns. For this, I adopted an approach that has proven successful for
predicting the response of plants to fire, a species-traits approach. Examining the
response of traits, rather than species, ultimately leads to a greater mechanistic
understanding and results are potentially more easily applied to other locations and
species. Ideally, one might hope to collect a spider from any locality and from only its
physical and behavioural traits predict the species‟ change in abundance following
disturbance. I was interested in testing if the traits of species could predict their
response to fire. In the fourth chapter, I utilise three methods to test for links between
the traits of spiders and the environment (post-fire age) in which they were collected.
The use of these techniques has only recently become widely accessible, and the
strengths and weaknesses of each method are still being established. Additionally, the
use of a traits-based approach for fauna and disturbance by fire is highly novel.
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108
CHAPTER 2
Is the successional trajectory of an arid spider
assemblage following fire deterministic?
Peter R Langlands
Karl E C Brennan
Bruce Ward
Formatted for Austral Ecology
109
ABSTRACT
Fire is a common disturbance in many ecosystems, including arid Australia.
Understanding whether fauna respond in a deterministic manner towards a single
endpoint, or to multiple states, is of crucial importance for conservation management.
Why different taxa or assemblages display single or multiple end points is also
important to develop a synthetic theory of succession. To examine the post-fire changes
in assemblages of spiders, we established a chronosequence study in spinifex habitat of
central Western Australia. Ground-active spiders were pitfall-trapped over nine months
in sites representing experimental fires (0 and 0.5 years post-fire) and wildfires (3, 5, 8
and 20 years post-fire). There were significant non-linear changes in species richness,
evenness and composition of spiders with increasing post-fire age. For all three
measures, the assemblage appears highly deterministic, converging towards the long
unburnt state. Similarity in richness, evenness and species composition to the 20-yearold sites all increased with increasing time since fire (3 to 8 years). However,
experimentally burnt sites did not neatly fit this sequence. We consider two alternative
hypotheses to explain this second trajectory: inertia within the system or the rapid
migration and recolonization from nearby surrounding unburnt areas. Analyses
indicated that half of the 179 species had significant preferences for, or where restricted
to, particular post-fire ages. This suggests that adequate pyrodiversity, both in terms of
post-fire ages and/ or scale and intensity of fires, may be important for the conservation
of spiders in this habitat. However, due to the high number of singletons and low
indicator values, the significance of this result for conservation management remains
equivocal. Despite this, the high degree of determinism provides hope that managers
can develop a good predictive understanding of post-fire successional changes in spider
assemblages in arid Australia.
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INTRODUCTION
Fire is a conspicuous disturbance in many environments and of great importance to the
maintenance of biodiversity (Bradstock et al. 2002). This is particularly true in the vast
arid zone of Australia, where the vegetation is highly flammable and large swathes (>
10 000 km2) can be burnt due to lightning strikes and human ignition (Allan &
Southgate 2002; Turner et al. 2008). Over the last century, the fire regime of arid
Australia has been substantially altered (Edwards et al. 2008). Previously, frequent and
extensive use of fire by Aborigines (Gould 1971; Kimber 1983) created a fine mosaic of
post-fire ages (Burrows et al. 2006; Bird et al. 2008). The current patch mosaic burning
paradigm assumes that „pyrodiversity begets biodiversity‟, but this has received limited
critical assessment (Parr & Andersen 2006). Understanding the conservation
implications of a changed fire regime, from many small fires to few immense fires, is a
challenging task. An essential first step is examining the response of fauna and flora in
relation to the time since single fires.
Successional patterns with time since fire can display a continuum of responses
from a single, deterministic end-point, multiple stable end-points or purely stochastic
trajectories. Here, the framework of complex systems theory, and the analogy of a ball
and cup or basins within a three-dimensional surface are useful (Samuels & Drake
1997; Anand & Desrochers 2004). The ball represents the community, its location
represents its current state (e.g., species richness or composition) and the base of the
cup or basin is the attractor or stable end-point. Therefore, disturbances will move the
ball around the cup (species richness or composition changes), but if insufficient to
move the ball over the lip of the cup, it will eventually return to the base (original
richness or composition). The velocity of return is determined by the slope of the sides.
Westman‟s (1978) terminology of resilience and inertia can describe the behaviour of
the ball. The ball and cup analogy implies greater variation in community structure
immediately following disturbance, but over time the ball returns to a single end point
and community structure becomes more homogeneous. In the case of disturbance by
fire, increased variability immediately after fire could be caused by patchy fires, which
increase heterogeneity of post-fire habitats. Additionally, random colonization or lottery
effects following disturbance could increase variability. Uncovering why single or
multiple end-points occur is of critical interest in succession theory (Young et al. 2001;
Chase 2003).
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The response of vertebrates to fire in arid Australia has received considerable
attention. Reptiles follow a strongly deterministic pattern (Masters 1996; Letnic et al.
2004), while mammal succession seems more stochastic (Masters 1993; Southgate &
Masters 1996; Letnic 2003; Letnic et al. 2004). Invertebrate assemblages, however,
have received limited investigation (Friend 1995; Langlands et al. 2006). Considering
the high diversity and abundance of invertebrates, this should be an issue of concern to
fire ecologists. Over the last decade, awareness has grown substantially amongst nature
conservation agencies that there is a need to cater for the invertebrate component of
biodiversity. There is a critical lack, however, of scientific studies to guide decisions
about how best to manage fire other than vague notions of pyrodiversity. Identifying if
species have preferences for, or are restricted to, sites of particular post-fire ages is
important for assessing the potential for current fire regimes to cause local extinctions
(Driscoll & Henderson 2008).
Spiders are a diverse and ubiquitous predatory group, ideal for examining post-fire
responses. A review of Australian studies on invertebrates and fire found that spiders
were one group that showed consistent post-fire responses (Friend 1995). They are
sensitive to many features that change following disturbance by fire, particularly habitat
structure and complexity, along with litter depth and nutrient content (Duffey 1962;
Bultman & Uetz 1982; Riechert & Gillespie 1986; Uetz 1991). They can also influence
ecosystem functioning by preying on decomposers at lower trophic levels (Lawrence &
Wise 2000; 2004) and are favoured prey for many insectivorous marsupials (Fisher &
Dickman 1993; Bos & Carthew 2007). Indeed studies from forest ecosystems show
marked changes in spider assemblages following burning (e.g. Huhta 1971; Buddle et
al. 2006; Brennan et al. 2006), but we know very little about the response of spiders in
arid ecosystems (but see Langlands et al. 2006).
We sought to describe the post-fire changes of an assemblage of spiders in the
Australian arid zone. Are there differences among post-fire ages in abundance, species
richness, evenness and composition? If so, is the succession of spider assemblages
highly deterministic? We define deterministic succession as sites being more similar in
species composition to similar ages (e.g. following a chronological order) with
similarity to long unburnt sites increasing and multivariate dispersion decreasing over
time. In addition, within the „pyrodiversity promotes biodiversity paradigm‟, we were
interested in how many and which species were significant indicators for, or were
restricted to, particular post-fire ages.
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METHODS
Study area
The study was conducted in central Western Australia at the proposed Lorna Glen
(Matuwa) Conservation Park, located approximately 150 km NE of Wiluna (Fig. 1).
The former sheep and cattle station receives a median annual rainfall of 235 mm (range
86-654 mm) and experiences mean minimum and maximum monthly temperatures from
21-38 ˚C in summer and 5-21 ˚C in winter (Australian Bureau of Meteorology).
Lorna Glen contains a range of habitat types, with the most widespread of these
being the fire-prone hummock grasslands (Bullimore). This is a vegetation assemblage
dominated by hard spinifex Triodia basedowii E. Pritz, 1918, with an over storey of
marble gums (Eucalyptus gongylocarpa Blakely, 1936). There are also scattered mulga
(Acacia aneura Benth, 1855) and mallee (E. kingsmillii Maiden and Blakely, 1929 and
E. lucasii Blakely, 1934). Therefore, the vegetation is remarkably similar to that found
throughout much of the Great Victoria Desert. Although spinifex is highly flammable,
fires are unlikely to spread within stands less than 10-15 years old, unless preceded by
periods of high rainfall, which increases biomass and promotes growth of short-lived
soft grasses (Allan & Southgate 2002). Our study was restricted to this habitat type, as
improving knowledge of faunal responses to fire within the Bullimore is of critical
concern to land managers.
Study design
We conducted our study at the landscape scale, with 27 sites selected to represent the
majority of fire ages present at Lorna Glen (Fig. 1). Prior to 2000 Lorna Glen had a
recent history of fire suppression by pastoralists; however, infrequent and large-scale
(>100 km2) fires still occurred. We used Landsat satellite images from 1985 to 2005 to
establish the recent fire history of the study area. From these natural fire histories and
some experimental fires, we selected six treatments for post-fire ages: 0, 0.5, 3, 5, 8 and
20+ years since the last fire. The patch size in which each site was located was at least 9
ha and there were three to five sites per post-fire age (Fig. 1, Table 1). At each site, a 50
x 50 m (0.25 ha) quadrat was established a minimum of 150 m from the site boundary
(change in fire age) or road.
Many studies of the ecology of fires conducted at the landscape scale have
difficulties finding multiple fires of the same age within a study area that can act as true
replicates (Brennan et al. 2009). Our study design was similarly constrained by the
pyrodiversity present at Lorna Glen, with very few sites burnt multiple times since 1985
113
and no very recent burns (< 1-year-old). We were therefore unable to examine the
interplay of time since fire with fire frequency (multiple fires). Additionally, for some
post-fire ages (3, 5 and 8 years) multiple sites were located within a single fire scar
(Table 1). However, in these instances, sites were interspersed with other ages and
located as far apart as possible (the minimum distance between two sites within the
same fire scar was 1.9 km [sites 3-2 and 3-5] and was more often in the order of 5-10
km). To resolve the problem of a lack of very recent burns, we burnt seven patches of
habitat unburnt for at least 20 years. We burnt three patches in October 2005 and four
patches in April 2006 to examine two additional post-fire ages, 0 and 0.5 years
respectively. Each experimentally burnt patch had a single sampling site and was 9 ha
in size (300 x 300 m). For details of fire ignition procedure, weather conditions during
burning and temperatures of experimental fires see Appendix A (online supplementary
material).
Sampling and identification of spiders
At each site we installed five pitfall traps in each quadrat, one at each corner and one in
the centre. A few large traps are more efficient at sampling spiders than many smaller
traps (Brennan et al. 1999). Additionally, a few traps set for a longer period is more
efficient than many traps set for a shorter time (Riecken 1999). Traps consisted of a
sleeve (125 mm diameter PVC pipe) into which jars (2 L, 82 mm opening, 125 mm
diameter body, 200 mm deep) were inserted with a plastic collar filling the 21.5 mm
gap. One litre of preserving fluid was used (80% propylene glycol, 16% water and 4%
formalin) with the addition of three drops of detergent as surfactant (Pekar 2002).
Propylene glycol was used in preference to ethylene glycol as it is less hazardous to
human health (Hall 1991) and performs equally well (Weeks & McIntyre 1997). Roofs
of corrugated iron (200 mm square by 0.3 mm thick) covered each pitfall at a height of
3 cm, to minimise access by vertebrates and protect the contents from direct sunlight.
We opened the traps 30 April 2006 and exchanged them at three monthly intervals until
18 January 2007 (256- 258 days per trap). The PVC sleeves ensured minimum
disturbance when exchanging jars. We rinsed the trap contents with water in a 0.5 mm
sieve before storing them in 75% ethanol.
We sorted male spiders from each trap and recorded their abundance. We then
sorted these to family (Raven et al. 2002) and identified to species level. Taxonomic
nomenclature follows Platnick (2010), except for wolf spiders in the genus Hoggicosa
(see Langlands & Framenau 2010). It is very difficult to match males, females and
114
juveniles of the same species correctly, because taxonomic knowledge of the Australian
spider fauna is particularly poor compared to the northern hemisphere (Brennan et al.
2004). To avoid identification errors the results presented here are from males only,
with species boundaries verified by taxonomic experts (see acknowledgements). We
combined data for each pitfall trap and collection period to give one sample per site. All
specimens are deposited in the Western Australian Museum (registration numbers
T61480-T62081, T89622-T91450).
Statistical analyses
A permutational analysis of variance (Legendre & Anderson 1999; Anderson 2001)
tested for differences in abundance, species richness, evenness and species composition
of male spiders with the fixed factor AGE (levels 0, 0.5, 3, 5, 8 and 20 years). We used
unrestricted permutation of the raw data with type III sums of squares and 9999
permutations in PERMANOVA+ (Anderson et al. 2008, version 1.01). For univariate
analyses, a similarity matrix between all pairs of sites was calculated based on
Euclidean distance. To overcome the limited number of unique permutations for some
pair-wise comparisons (only 35 permutations for 0 vs 0.5), we used Monte Carlo pvalues. Anderson & Robinson (2003) demonstrate that the asymptotic permutation
distribution of the entire pseudo-F statistic can be calculated in such situations. As
abundance varied between sites, prior to analysis we rarefied species richness to the
minimum number of spiders collected from a site (85 males) using PRIMER (Clarke &
Gorley 2006, version 6.1.11). To compare evenness in the abundance of species
between post-fire ages we used the Berger-Parker index. The Berger-Parker index is the
inverse of the proportion of the most abundant species in a sample, and has low
sensitivity to sample size.
For species composition, the abundance of each species of spider was fourth root
transformed, to decrease the influence of abundant species, and the Bray-Curtis measure
of similarity calculated. We used non-metric multidimensional scaling (nMDS) to
visualise in two dimensions the similarity in species composition between sites. We
fitted ellipsoid hulls using Titterington‟s algorithm in the R package „cluster‟ (Maechler
et al. 2005), so all sites of a given age were on or within the boundary of an ellipse. To
uncover which species were most responsible for the observed similarity of the
experimentally burnt and long unburnt sites, we used similarity percentages analysis on
the transformed matrix (SIMPER in PRIMER; Clarke & Warwick 2001). We selected
the 20 species that contributed the most to average similarity within a group (0, 0.5 and
115
20 years combined) and average dissimilarity between groups (compared to 3, 5 and 8
years combined). We used the distance to group centroids in the PERMDISP routine of
PERMANOVA+ to test for homogeneity of multivariate dispersion among ages
(Anderson 2006).
Indicator species analysis (Dufrene & Legendre 1997) identified species associated
with particular post-fire ages. This analysis uses the relative abundance of a species as
well as its relative frequency of occurrence to calculate a value between 0 (no
discrimination between ages) and 100 (perfect discrimination between ages, found only
at all sites of a particular fire age). Analysis was performed using PC-ORD (McCune &
Mefford 1999) on the fourth root transformed matrix (9999 permutations).
Throughout the paper, we treat statistical tests with P < 0.05 as significant. We have
not corrected for multiple tests (e.g. pair-wise PERMANOVA or indicator species
analysis), preferring to present the raw P and data values, allowing the reader to decide
significance (see Moran 2003).
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RESULTS
Of the 14 104 spiders collected nearly half were adults (48.6%), most of which were
males (61.8%, 4234 specimens). The most abundant families were the Gnaphosidae
(823 individuals), Corinnidae (805), Oonopidae (693), Prodidomidae (382), Miturgidae
(297), Salticidae (242) and Zodariidae (240). The males represented 179 species from
24 families, with only 32 species formally described. The most speciose family was the
Gnaphosidae with 34 species, followed by the Salticidae (19 spp.), Zodariidae (17 spp.),
Oonopidae (16 spp.), Theridiidae (12 spp.) and Prodidomidae (10 spp.) (Appendix B).
Abundance
Abundance of male spiders ranged from 85 to 250 individuals per site. Permutational
analysis of variance showed there was no clear pattern or significant difference in the
abundance of spiders with post-fire age (d.f. 5, 21, pseudo-F = 1.509, P = 0.23; Fig. 2a).
We did not consider abundance data further.
Species richness and evenness
Rarefied species richness ranged from 18.9 to 38.1 species per site. It was lowest in 3year-old sites and increased significantly with post-fire age to 20 years
(PERMANOVA, d.f. 5, 21, pseudo-F = 10.01, P = 0.0001). The experimentally burnt
sites (0 and 0.5 years since fire) were similar in richness to the 8-year-old sites (Fig.
2b). Pair-wise tests revealed significantly fewer species at 3-year-old sites than all other
sites. The 5-year-old sites also had significantly fewer species than the 0 and 20-yearold sites (Fig. 2b, Appendix C).
Sixty-two species (35% of total) only occurred in a single fire age: 0 years (8
species), 0.5 years (4 spp.), 3 years (9 spp.), 5 years (9 spp.), 8 years (11 spp.) and 20
years (21 spp.). However, it must be noted that the majority of these species were
singletons (49 of 62) and doubletons (10 of 62) (Appendix B).Evenness increased
between 3 to 20 years post-fire, with the Berger-Parker index increasing with time since
fire (Fig. 2c). A permutational analysis of variance found significant differences in
evenness (Berger-Parker) among post-fire ages (d.f. 5, 21, pseudo-F = 7.20, P =
0.0006). The pattern of evenness (Berger-Parker) with time was similar to that for
species richness, except average evenness for experimentally burnt sites was similar to
20-year-old sites and evenness increased more slowly between 3 to 8 years.
117
Species composition
There was a significant shift in the composition of species with post-fire age, and a clear
successional trajectory was evident from 3 years, to 5, 8 and 20 years since fire (Fig. 3;
PERMANOVA, d.f. 5, 21, pseudo-F = 2.63, P = 0.0001). The experimentally burnt
sites (0 and 0.5) clustered apart from the other ages and were more similar to 20-yearold sites than were the older 3-year-old sites (Fig. 4). A three dimensional ordination
(stress 0.15) was consistent with this 2-d result, in that it showed sites arranged in an
orderly sequence of post-fire ages. Pair-wise comparisons showed that the 0 and 20year-old sites differed significantly from all other post-fire ages except 0.5 years. In
addition, post-fire ages 3 and 8 years were also significantly different (Fig. 3, Appendix
C). These differences were attributable to changes among groups in multivariate
location, rather than multivariate dispersion, which was not significant (PERMDISP,
d.f. 5, 21, F = 2.597, P = 0.194). The pattern of dispersion with post-fire age was
somewhat hump shaped, with a maximum in 5-year-old sites: 0 years (average
dispersion 27.0), 0.5 years (27.9), 3 years (29.7), 5 years (34.4), 8 years (32.2) and 20
years (30.9).
The analysis of similarity percentages found sixteen species were more abundant
and four species less abundant in the 0-, 0.5- and 20-year old sites compared to the 3-,
5- and 8-year old sites (Appendix D). These 20 species contributed over half (52.38%)
of the average Bray-Curtis similarity (47.16%) between the experimentally and long
unburnt sites. They also contributed 28.61% of the average dissimilarity (59.12%)
between these sites and the other ages (3, 5 and 8 years). The 20 species represented 12
families and a wide range of life histories (Appendix D).
Indicator species analysis identified 30 species from 15 families that had significant
indicator values (Table 2). However, most of these species had relatively low indicator
values (range 21-67%), which suggests they are not consistently good predictors of fire
ages. Two-thirds of the indicator species were selected for recently burnt (0, 0.5 years)
or long unburnt (20+ years) sites with fewer indicator species identified for the
intermediate fire ages (3, 5, 8 years, Table 2). Graphing the abundances of several of the
species selected by indicator analysis shows their distinct preferences for recently burnt
(Fig. 5a) or long unburnt sites (Fig. 5c). Two lycosids [„Yalkara grp.‟ sp. 02 and
Hoggicosa bicolor (Hogg, 1905)] both had higher abundance in the 0 age sites, with
only a few individuals caught in 0.5-, 3- and 8-year-old sites (Fig. 5a). The reverse was
true for Ceryerda cursitans Simon, 1909 and Lamponata daviesae Platnick, 2000, with
most individuals collected in the 20-year-old sites (Fig. 5c). Indicators selected for the
118
intermediate ages show peaks in abundance for their particular fire age (Fig. 5b).
Gnaphosidae sp. 09 for example, has very high abundance in 3-year-old sites, but
declines in abundance over time.
DISCUSSION
Understanding the degree of determinism, why single or multiple basins of attraction
occur and under what conditions they occur is an important question for theory and
management (Chase 2003; Hobbs et al. 2007). From a management perspective,
knowing when there is a high degree of determinism is crucial, as it provides land
managers with some level of certainty as to how things will change over time. We
found the post-fire response of spider assemblages in an arid habitat following wildfires
to be deterministic when measured in terms of species richness, evenness and
composition. Changes in these parameters with increasing post-fire age, while nonlinear, followed a chronological sequence and became increasingly similar to long
unburnt sites with time.
The succession of reptiles in arid Australia also follows a highly deterministic
pattern (Masters 1996; Letnic et al. 2004), in contrast to mammals (e.g., Masters 1993;
Southgate & Masters 1996; Letnic 2003). For arid mammals, post-fire succession is
more aptly explained by multiple stable states, in which stochastic factors, particularly
rainfall, shape transitions between states. It is possible that the mode of thermal
regulation (ectothermic vs. endothermic) influences the level of determinism of postfire succession (Letnic et al. 2004). Thus, the pattern for spiders, being ectotherms,
lends support to this hypothesis. However, we note that in other environments reptiles
sometimes show little determinism (Driscoll & Henderson 2008; Lindenmayer et al.
2008) and mammals high determinism (Fox 1982). Therefore, habitat type and other
factors may interact to determine the degree of determinism.
Chase (2003) made a series of bold predictions as to when single or multiple states
or basins of attraction would occur. He predicted single states in systems with low
productivity, high rates of connectance, high disturbance and small regional species
pools, while multiple states would occur under the converse. Our results fit most
predictions for a single state (low productivity, high rates of connectance and high
disturbance). However, they contradict the prediction of a small region species pool.
We consider our study area to contain a high regional species pool, as many spiders in
the arid zone have large geographical ranges (extent of occurrence) and over 200
species occur at Lorna Glen (this study & Owen 2004).
119
Post-fire changes in species richness and evenness
The U-shaped pattern for species richness we found differs from chronosequence
studies of the response of spiders to fire in other more mesic habitats. These have shown
rapid recovery and a plateau in richness within the first three years (Moretti et al. 2002;
Brennan et al. 2006), little difference between ages (Niwa & Peck 2002) and/or a hump
shaped curve with time since fire (Buddle et al. 2000; 2006). In a longitudinal study,
Merrett (1976) found that species richness increased slowly over the first 10 years
following burning in English heathland, but richness was not high immediately
following fire, as seen in our study. Likewise, species richness declined immediately
after fire and increased gradually over the following two years in another longitudinal
study in semi-arid Western Australia (Strehlow 1993). Working in the Great Victoria
Desert of Australia, in similar vegetation to our study, Langlands et al. (2006) followed
spider assemblages for 14 years. They found no clear pattern in species richness
following fire. However, all three of these longitudinal studies suffer from limited
replication. A further constraint limiting comparisons between studies is the oftenunderappreciated importance of standardizing species richness by the number of
individuals at a site (see Gotelli & Colwell 2001; Buddle et al. 2005). Our high species
richness in recently burnt sites could be driven by both survival of species in-situ and
colonisation of new species and we return to these points in detail below.
We found that trends in evenness were similar to changes in species richness with
post-fire age. This result is not due to changes in species richness, as the Berger-Parker
index depends purely on evenness (Colwell 2009). Our result is identical with post-fire
changes in dominance of spiders found in the boreal forest of Canada. Buddle et al.
(2000) found that evenness was initially high one year after fires, but within two years
was quite low and increased steadily with increasing time since fire. Other studies have
found no difference in dominance post-fire when using the Berger-Parker index (Niwa
& Peck 2002). High evenness in recently burnt sites may be an indication that colonists
are still establishing and have not had sufficient time to establish dominance (Buddle et
al. 2000). This requires testing experimentally.
120
Shifts in species composition
Changes in the species composition of spiders in arid Australia appear to follow a
highly deterministic succession after wildfires, with similarity to long unburnt sites
increasing markedly over time. This is consistent with previous studies, which have
found species composition returns to, or converges towards, long unburnt states within
2-30 years (e.g. Huhta 1971; Buddle et al. 2000; Moretti et al. 2002; Brennan et al.
2006). We found no significant difference in multivariate dispersion, but the power of
our analysis may have been limited, with a minimum of 10 sites recommended for such
analyses (Anderson et al. 2008). A trend in decreasing multivariate dispersion over time
may have provided further evidence of a deterministic succession.
Multiple successional trajectories to long unburnt sites?
All sites appear to converge towards the long unburnt state, increasing in similarity with
long unburnt sites over time. However, the recently burnt sites do not fit an orderly
chronological sequence with increasing post-fire age. Therefore, our results suggest that
the system has a degree of inertia or that there may be two trajectories for post-fire
succession, one following large intense wildfires and one following small, less intense
experimental fires (Fig. 4). Although this could simply be a result of a noisy data set,
this seems unlikely, as we sampled continuously over a nine-month period and had
three to five sites per post-fire age. We therefore consider two biological mechanisms to
explain multiple trajectories.
Firstly, the lower intensities of the experimental burns allowed some species to
survive the fire in-situ. This would indicate a strong degree of inertia to low intensity
fires within the system. There would be evidence for this hypothesis if a longitudinal
study found that the 0.5 aged sites became more similar in species composition with the
3-year-old sites, and less similar with the 20-year-old sites (Fig. 4, trajectory 2a).
Secondly, the experimental burns extinguished most of the spider fauna, but the
smaller scale of the fires allows species to recolonise rapidly from the surrounding long
unburnt matrix. This would suggest that although there is a single attractor or cup
within this system, aspects of the disturbance (scale) can result in different return
trajectories or the pace of return (elasticity). If the 0.5 ages continued to increase in
similarity with the 20-year-old sites, this hypothesis would be supported (Fig. 4,
trajectory 2b). In Canadian forests, Buddle et al. (2000; 2006) found that succession of
spiders following timber harvesting converged with sites undisturbed for 70 years much
121
faster than sites that had been burnt. They highlighted the importance of species
surviving in-situ or the smaller scale of harvesting sites as potential explanations for the
faster recovery following harvesting. For arid mammal assemblages, Letnic et al.
(2004) suggested that the scale of fires studied could be a key factor in determining the
post-fire response. Due to logistical constraints, the scale of experimental fires is often
small. If the second trajectory is true and multiple return trajectories exist, it may be
important to ensure not only multiple fire ages, but also multiple fire scales or
intensities to maintain spider diversity (discussed further below).
In an attempt to shed light on these two hypotheses, we identified the top 20 species
that accounted for the similarity between the experimentally burnt and long unburnt
sites. There was no clear indication amongst these species of a particular life history or
phylogenetic pattern to explain their survival or recolonization of the experimentally
burnt sites. The burrowing nemesiid mygalomorph Kwonkan sp.01 is likely to have
survived in-situ deep it its burrow. Likewise, the pholcid Trichocyclus nigropunctatus
Simon, 1908, which often live in goanna (Reptilia: Varanus) burrows on our sites,
probably survived the fire. For the remaining species, it is likely that both survival in
refugia and immigration and recolonization are occurring.
Species responses and management implications
Species that are reliant on characteristics of a specific fire age, particularly recently
burnt or long unburnt habitats, may be at a heightened risk of extinction (Driscoll &
Henderson 2008). Inspection of the data identified 62 species (35%) found in only a
single post-fire age; however, as noted in our results, most of these were singletons,
which by definition are restricted to a single post-fire age. A further 27 species (15%)
were identified as significant indicator species for a post-fire age. Although again, the
low indicator values we found suggest few of these were consistently restricted to or
highly abundant in particular ages. We cannot rule out the possibility that these species
are simply tourists or occupy a broader range of post-fire ages or habitats. For species
that do survive in low densities in other post-fire ages or habitats, the risk of extinction
would be limited (Driscoll & Henderson 2008 and references therein). Therefore, it is
equivocal how many species are restricted to or reliant on a particular post-fire age.
Clearly, surveys of other habitats within Lorna Glen are required to establish habitat
preferences.
122
Lacking such data, a precautionary approach suggests we treat these species as
potential post-fire age specialists. This perspective suggests that it is important to have
areas representing multiple fire ages at any given time, lending support to the
„pyrodiversity begets biodiversity‟ hypothesis (see Parr & Andersen 2006). However,
the scale of fires required to initiate the full range of post-fire responses remains
unknown. From the results of our experimental fires, it seems likely that areas greater
than 9 ha are required. Actively creating pyrodiversity would also reduce the current
risk of a large wildfire removing most of the long unburnt habitat simultaneously. Fire
management plans for Lorna Glen have been prepared (Anon. 2003; Muller 2006), and
are continuing to be revised as we develop a better understanding of the biota and its
responses to fire. Trying to uncover the requirements of spiders and other fauna and
incorporate them into fire plans will be a considerable and continuing challenge (see
Clarke 2008).
In conclusion, we have found that the post-fire succession of the arid spider
assemblages we studied appears deterministic and largely in agreement with theoretical
predictions for a single stable state. However, longitudinal studies are required to
confirm these findings and determine the mechanism of return trajectories. Finally, for
half the species, further sampling is required to determine the risk of extinction by
inappropriate fire management.
ACKNOWLEDGEMENTS
Thanks to Bob Black,Volker Framenau, Don Driscoll and anonymous reviewers for
constructive comments on the manuscript and useful conceptual insights. For field
assistance we thank Karen Debski, Eliane Assis, Filomeno Cruz, Amanda McGinty,
Fernanda Ferreira, Christopher Taylor, Ted Griffiths, Bob and Natasha Langlands and
Graeme Liddlelow. Ryan Butler, Brad Barton, Julie Patten, Steve Toole, Luke
Puertoliano, Dave Atkins and Anthony Desmond assisted with experimental fires.
Fauna were collected with ethics approval (DEC AEC 2005/18). We are especially
grateful to the following taxonomists for providing assistance with spider
identifications: Barbara Baehr, Volker Framenau, Barbara York Main, Ricardo Ott,
Robert Raven and Julianne Waldock. Thanks also to Norma and Rex Ward from
Milrose Station for providing access to their property. Funding was provided by the
Western Australian Department of Environment and Conservation and the School of
Animal Biology at the University of Western Australia. PRL was supported by an
Australian Postgraduate Award.
123
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Uetz G. W. (1991) Habitat structure and spider foraging. In: Habitat Structure: The
Physical Arrangement of Objects in Space (eds S. S. Bell, E. D. McCoy and H. R.
Mushinsky) pp. 325-48. Chapman and Hall, Melbourne.
Weeks jr. R. D. & McIntyre N. E. (1997) A comparison of live versus kill pitfall
trapping techniques using various killing agents. Entomologia Experimentalis et
Applicata 82, 267-73.
Westman W. E. (1978) Measuring the inertia and resilience of ecosystems. BioScience
28, 705-10.
Young T. P., Chase J. M. & Huddleston R. T. (2001) Community succession and
assembly. Ecological Restoration 19, 5-18.
129
Table 1. The post-fire age of study sites with location (latitude and longitude) and the
date when last burnt.
Post-fire
age
0
0
0
0
0.5
0.5
0.5
3
3
3
3
3
5
5
5
5
5
8
8
8
8
8
20
20
20
20
20
Location
Number 26°S
121°E
1
21' 43''
25' 27''
2
15' 51''
06' 12''
3
16' 13''
06' 02''
4
21' 26''
14' 14''
1
21' 26''
24' 50''
2
13' 58''
11' 48''
3
21' 42''
25' 16''
1
14' 12''
17' 00''
2
09' 35''
16' 46''
3
11' 58''
18' 10''
4
12' 13''
19' 42''
5
08' 45''
16' 05''
1
16' 13''
02' 34''
2
16' '52'
21' 42''
3
17' 03''
11' 43''
4
21' 24''
13' 29''
5
11' 00''
02' 36''
1
20' 15''
26' 58''
2
15' 22''
07' 07''
3
13' 33''
11' 36''
4
16' 41''
21' 12''
5
11' 57''
17' 47''
1
16' 00''
06' 19''
2
14' 01''
11' 35''
3
21' 22''
25' 06''
4
21' 39''
14' 11''
5
11' 05''
02' 11''
Date Burnt
27 April 2006
26 April 2006
28 April 2006
27 April 2006
11 October 2005
9 October 2005
14 October 2005
25 November 2002
25 November 2002
25 November 2002
25 November 2002
25 November 2002
8 January 2001
8 January 2001
8 January 2001
8 January 2001
15 November 2000
23 December 1997
1 February 1998
1 February 1998
1 February 1998
1 February 1998
before 1988
before 1988
before 1988
before 1988
before 1988
130
Table 2. Species that were significant indicators (p < 0.05) for each post-fire age.
Post-fire
Family
Species
Indicator p
age
value
Lycosidae
„Yalkara grp.‟ sp. 02
66
0.002
Segestriidae
Genus 1 sp. 02
60
0.007
Lycosidae
Hoggicosa bicolor
43
0.026
Gnaphosidae
Encoptarthria sp. 01
43
0.028
Nemesiidae
Kwonkan sp. 01
32
0.021
Theridiidae
Steatoda sp. 01
31
0.024
Miturgidae
Genus 1 sp. 02
22
0.048
Thomisidae
Genus 1 sp. 02
67
0.009
Lamponidae
Lampona quinqueplagiata
50
0.040
Corinnidae
Poecilipta sp. 03
49
0.016
Pholcidae
Trichocyclus nigropunctatus
42
0.017
Oxyopidae
Oxyopes rubicundus
24
0.029
Theridiidae
Steatoda sp. 02
21
0.031
Gnaphosidae
Genus 1 sp. 09
48
0.001
Prodidomidae
Nomindra leeuweni
29
0.006
Corinnidae
Supunna picta
21
0.013
5
Gnaphosidae
Genus 1 sp. 03
43
0.033
8
Gnaphosidae
Genus 1 sp. 28
53
0.001
Segestriidae
Genus 1 sp. 01
45
0.044
Pholcidae
Trichocyclus arabana
45
0.037
Theridiidae
Steatoda sp. 05
41
0.030
Nemesiidae
Genus 1 sp. 02
36
0.023
Zoridae
Argoctenus sp. 01
27
0.001
Gnaphosidae
Ceryerda cursitans
63
0.006
Gnaphosidae
Genus 1 sp. 13
60
0.008
Prodidomidae
Wydundra sp. 04
60
0.016
Zoridae
Argoctenus sp. 08
60
0.016
Lamponidae
Lamponata daviesae
55
0.010
Trochanteriidae Fissarena castanea
44
0.008
Oonopidae
28
0.035
0
0.5
3
20
Opopaea sp. 13
131
Fig. 1. The location of sites (*) within the proposed Lorna Glen conservation park
(inset: park location in Western Australia). Site names denote fire age in years followed
by replicate number. Non-spinifex vegetation is shaded grey and lines mark unsealed
roads.
132
a
Abundance ±s.e.
250
a
200
a
a
150
a
a
a
100
0
b
5
10
15
20
Species richness ±s.e.
40
a
35
a
ad
ab
bd
30
c
25
20
0
Berger-Parker index ±s.e.
c
5
10
15
20
10
ab
8
a
a
abd
6
c cd
4
2
0
0
5
10
15
20
Post-fire age (years)
Fig. 2. Mean a) spider abundance, b) species richness rarefied to 85 individuals and c)
Berger-Parker evenness index with post-fire age in years. Unlike letters indicate
significant differences (p < 0.05) from PERMANOVA pair-wise tests and bars indicate
standard errors.
133
1.0
8-1
20-1
8-5
20-4
20-2
20-5
8
20
0.5
5-2
8-2
5
3-4
5-1 5-5
0.0
nmds axis 2
5-3
20-3
0.5-2
8-4
8-3
5-4
0.5
-0.5
0.5-1
0-1
3-2
0.5-3
3
0-2
3-3
0-3
0
-1.0
3-1
3-5
-1.5
-1.0
0-4
-0.5
0.0
0.5
1.0
nmds axis 1
Fig. 3. Non-metric multidimensional scaling (nMDS) of species composition of spiders
based on Bray-Curtis similarity from fourth root transformed data (Stress = 0.23). Small
numbers indicate sites (post-fire age in years – site number, see Table 1). As a visual
aid, for each post-fire age, sites are enclosed within ellipses and the centre of the ellipse
is indicated by large numbers.
134
Average similarity to 20 years
55
50
2b
45
2a
1
40
35
Hypothetical trajectories
30
0
5
10
15
20
Post-fire age (years)
Fig. 4. Trajectories of post-fire re-assembly as shown by the average similarity (BrayCurtis) of each post-fire age compared to 20-year-old sites. For 20-year-old sites it is
the average similarity within the age. Solid arrows mark the two inferred recovery
trajectories: 1) following wildfires (3- 20 years) and 2) experimental burns (0 & 0.5
years). Dashed arrows mark two possible outcomes for the experimentally burnt sites:
2a) inertia in the system or 2b) alternative recovery trajectory (see discussion). For
clarity, standard errors are shown above or below only.
135
a
Mean abundance +s.e.
81
Lycosidae 'Yalkara grp.' sp.02
Lycosidae Hoggicosa bicolor
Thomisidae Genus 1 sp.02
Corinnidae Poecilipta sp.03
16
1
0
0
0.5
3
5
8
20
b
Gnaphosidae Genus 1 sp.09
Gnaphosidae Genus 1 sp.03
Gnaphosidae Genus 1 sp.28
Mean abundance +s.e.
81
16
1
0
0
0.5
3
5
8
20
c
Mean abundance +s.e.
81
Gnaphosidae Ceryerda cursitans
Gnaphosidae Genus 1 sp.13
Prodidomidae Wydundra sp.04
Lamponidae Lamponata daviesae
16
1
0
0
0.5
3
5
8
20
Time since fire (years)
Fig. 5. Mean abundance for selected species that were identified by indicator analysis as
significant indicators of post-fire ages a) 0 and 0.5 years, b) 3, 5, and 8 years and c) 20
years (see Table 2). Analysis used fourth-root transformed data, but for ease of viewing,
graphs show untransformed abundance values with standard errors. There were five
sites each for 3 to 20 years, while 0 and 0.5 years had four and three sites respectively.
136
Appendix A
Detailed explanation of fire ignition procedure, weather conditions and temperatures of
experimental fires.
A 9 hectare area (300 x 300 m) was marked by 2 m wide fire breaks and sites were
prescribe burnt (lit in 5-10 m strips along the side opposite to the prevailing wind).
Ignition by drip torches ensured that almost all vegetation on each site was burnt. Table
A1 shows the time of ignition and completion for experimental fires (24 hrs), with the
observed weather conditions (ambient air temperature, humidity and wind speed).
Table A1.
Site
Ignition time
Finish (24 hrs)
Avg. relative
Avg. wind
Ambient temperature (˚C)
humidity (%)
speed (m.s-1)
0-1
10:30 (17)
12:10 (22)
31
2.2
0-2
14:00 (27)
17:00 (23)
34
2.8
0-3
14:00 (25)
16:40 (20)
25
1.7
0-4
14:31 (26)
21:35 (17)
26
1.7
0.5-1
18:00 (24)
21:35 (17)
15
0.6
0.5-2
17:10 (31)
20:10 (17)
13
0.3
0.5-3
16:46 (29)
22:30 (21)
20
0.8
To provide an indication of the intensity of the experimental fires, thermocouples were
used to record temperatures in five of the seven sites. Due to the small scale, the
experimental fires were unlikely to be as nearly as intense as large wildfires. However,
for all sites measured, the maximum temperature at ground level (0 cm) within spinifex
ranged between 456 and 709˚C. The maximum temperature recorded was 825˚C at 10
cm above ground within spinifex (Fig. A1).
137
Site 0-1: in spinifex, above ground
30 cm
10 cm
5 cm
2 cm
0 cm
800
700
600
500
400
300
200
100
0
Site 0-1: in bare soil, below ground
900
0
60
120
180
240
Temperature *C
Temperature *C
900
300
500
400
300
200
100
0
Site 0-3: in spinifex, above ground
30 cm
10 cm
5 cm
2 cm
0 cm
0
60
120
180
240
300
200
100
0
30 cm
0 cm
2 cm
5 cm
10 cm
0
120
240
360
480
600
Site 0.5-2: in spinifex, above ground
800
700
600
500
400
300
200
100
0
0
60
120
180
240
300
0 cm
2 cm
5 cm
10 cm
0
60
120
180
240
300
0 cm
2 cm
5 cm
10 cm
500
400
300
200
100
0
0
60
120
180
240
300
900
800
700
600
500
400
300
200
100
0
2 cm
5 cm
10 cm
15 cm
0
60
120
180
240
300
300
Seconds
2 cm
10 cm
20 cm
800
700
600
500
400
300
200
100
0
0
60
120
180
240
300
Site 0.5-3: in spinifex, below ground
Temperature *C
Temperature *C
500
400
300
200
100
0
240
Site 0.5-2: in bare soil, below ground
Site 0.5-3: in spider burrow, bare ground
900
800
700
600
180
800
700
600
900
90 cm
60 cm
30 cm
0 cm
Temperature *C
Temperature *C
900
120
Site 0.5-2: in bare soil, below ground
Temperature *C
Temperature *C
Site 0.5-1: in spinifex, above & below ground
900
800
700
600
500
400
300
60
900
Temperature *C
Temperature *C
500
400
300
200
100
0
0
Site 0-3: in spinifex, below ground
900
800
700
600
0 cm
2 cm
5 cm
10 cm
800
700
600
900
800
700
600
500
400
300
200
100
0
0 cm
2 cm
5 cm
10 cm
0
60
120
180
240
300
Seconds
Figure A1: The temperatures (˚C) recorded by thermocouples in some of the
experimentally burnt sites. For each graph the site, habitat (bare ground, spinifex or
spider burrow) and location (above or below ground) are indicated.
138
Species
Cheiracanthium sp.05
Clubiona sp.01
Clubiona sp.02
Clubiona sp.03
Clubiona sp.04
Battalus sp.04
Genus 1 sp.01
Poecilipta sp.02
Poecilipta sp.03
Supunna funerea Simon, 1896
Supunna picta (L. Koch, 1873)
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Phryganoporus sp.01
Genus 1 sp.01
Genus 1 sp.02
Family
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Desidae
Desidae
Desidae
Desidae
Dictynidae
Dictynidae
collected only from a single post-fire age.
8
20
0
0
8
1
6
0
25
0
21
0
0
0
0
1
0
1
0
0
0
0
0
1
1
40
0
18
0
0
0
0
0
0
1
0
139
1
0
0
0
3
2
283
1
1
1
1
0
0
0
0
2
0
0
2
42
0
5
0
212
2
0
0
0
0
2
0
0
2
0
0
3
59
1
7
4
119
1
0
1
0
0
0
0
2
0
0
0
2
5
0
4
1
75
2
0
0
0
2
1
0
0
0
1
20
15
25
14
17
13
21
15
49
10
20
40
27
25
40
12
20
3*
20
5
0
0
8
3
20
0.5
3
3*
20*
5
0*
8*
3
20*
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
5
1.000
0.604
0.311
0.565
0.900
0.013
0.685
0.016
0.551
1.000
1.000
0.142
0.286
0.252
0.143
0.933
1.000
p
abundance and frequency of occurrence, low values denote the opposite. Significant p values are bolded and the symbol * indicates species that were
the maximum value and p value (9999 permutations). High Indicator values denote species that were found in a post-fire age in high relative
Abundance of all 179 species collected within each post-fire age, ordered by family, with the indicator species value (IndVal, 0-100) for the age with
Appendix B
Species
Ceryerda cursitans Simon, 1909
Eilica sp.07
Eilica sp.11
Encoptarthria sp.01
Encoptarthria sp.08
Encoptarthria sp.15
Encoptarthria sp.33
Encoptarthria sp.34
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Genus 1 sp.09
Genus 1 sp.10
Genus 1 sp.12
Genus 1 sp.13
Genus 1 sp.16
Genus 1 sp.17
Genus 1 sp.18
Genus 1 sp.21
Genus 1 sp.22
Family
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Appendix B cont.
5
8
20
0
0
1
0
0
0
0
1
1
0
24
9
0
0
0
0
0
17
4
50
1
0
0
0
0
2
0
1
0
11
6
14
1
7
0
0
1
0
0
12
0
45
1
0
140
4
1
2
0
0
0
1
18
91
13
0
6
1
0
0
0
0
5
0
35
8
0
16
0
0
0
0
0
0
6
14
4
5
16
15
2
0
0
0
3
2
0
10
0
0
0
0
0
0
0
0
8
5
6
11
10
3
2
0
0
0
1
0
2
12
2
4
0
0
1
1
12
0
4
6
17
15
7
1
0
1
1
1
21
1
1
1
7
18
20
25
22
20
60
20
26
48
28
22
16
43
25
21
20
20
29
43
35
18
63
5
3*
3
0.5
20*
20
3*
0.5
3
20
20
5
5
5
0.5
20*
20*
0.5
0
0.5
5
20
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
0.374
1.000
0.345
0.235
0.008
1.000
1.000
0.001
0.186
0.216
0.489
0.033
0.941
0.330
0.315
1.000
1.000
0.028
0.203
0.078
0.006
0.634
p
Species
Genus 1 sp.24
Genus 1 sp.25
Genus 1 sp.27
Genus 1 sp.28
Genus 1 sp.29
Genus 1 sp.30
Genus 1 sp.31
Genus 1 sp.32
Hemicloea sp.20
Hemicloea sp.23
Hemicloea sp.26
Laronius sp.19
Asadipus banjiwarn Platnick, 2000
Lamponina asperrima (Hickman, 1950)
Lamponata daviesae Platnick, 2000
Lamponina elongata Platnick, 2000
Lampona quinqueplagiata Simon, 1908
Lamponina scutata (Strand, 1913)
Erigone prominens Bösenberg & Strand, 1906
Genus 1 sp.01
Hoggicosa alfi Langlands & Framenau, 2010
Hoggicosa bicolor (Hogg, 1905)
Family
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Linyphiidae
Liocranidae
Lycosidae
Lycosidae
Appendix B cont.
5
8
20
10
1
0
0
2
0
0
0
0
0
0
1
0
0
0
0
0
4
1
1
0
7
1
0
0
1
0
3
0
0
0
0
0
0
0
1
0
1
0
4
0
0
0
3
141
1
0
0
0
0
0
2
0
0
0
0
0
0
0
0
0
0
0
6
8
0
15
0
1
0
3
1
0
0
1
0
0
0
0
0
0
0
0
1
4
4
8
1
8
1
2
1
1
8
0
0
1
1
0
0
0
1
0
0
2
0
10
28
8
0
5
0
1
0
0
7
2
0
7
0
2
1
0
0
0
3
0
0
4
1
9
1
21
43
7
20
18
22
50
20
55
20
40
20
25
20
33
40
20
20
17
53
30
10
23
0
0
8*
5
20
0.5
3*
20
8*
20*
20*
0*
8*
0.5*
20*
0.5
5*
8
8
3
20
3
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
0.026
0.965
1.000
0.509
0.040
0.361
0.010
1.000
1.000
0.136
1.000
0.252
1.000
0.116
0.139
0.333
1.000
0.001
0.719
0.139
1.000
0.326
p
1
0
11
0
Knoelle clara (L. Koch, 1877)
„Pexa grp.' sp.04
„Yalkara grp.' sp.02
„Yalkara grp.' sp.03
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Miturga sp.05
Genus 1 sp.06
Miturga sp.07
Genus 1 sp.08
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.05
Kwonkan sp.01
Kwonkan sp.06
Yilgarnia sp.04
Cavisternum sp.07
Grymeus sp.04
Grymeus sp.09
Myrmopopaea sp.01
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
5
8
20
0
0
0
44
2
4
13
1
1
2
17
0
2
8
6
11
31
7
0
1
0
13
0
5
3
0
0
0
3
1
0
6
7
8
6
1
1
2
0
0
142
0
0
0
9
0
0
1
0
0
2
5
0
0
0
1
7
15
6
0
0
1
1
5
0
1
0
0
1
4
0
0
7
6
0
1
2
2
11
24
4
0
0
3
0
1
2
1
22
0
1
4
0
0
6
9
1
0
2
5
13
16
2
0
2
0
0
0
2
2
54
0
12
4
0
0
0
16
0
0
9
5
3
17
1
0
0
1
0
12
14
8
30
25
23
32
25
25
36
23
21
15
30
33
22
22
15
33
66
8
14
5
0.5
20
20
0*
0.5
0
0*
0*
8
0
0.5
0
0
0.5
0
0
3
0.5*
0
5
0
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
Species
Family
Appendix B cont.
0.885
0.599
1.000
0.185
0.252
0.021
0.323
0.258
0.023
0.262
0.500
0.318
0.461
0.161
0.134
0.048
0.707
0.868
0.002
0.116
1.000
0.569
p
Species
Myrmopopaea sp.05
Myrmopopaea sp.08
Myrmopopaea sp.14
Myrmopopaea sp.15
Opopaea sp.02
Opopaea sp.03
Opopaea sp.06
Opopaea sp.12
Opopaea sp.13
Opopaea sp.16
Xestaspis sp.10
Xestaspis sp.11
Oxyopes sp.01
Oxyopes sp.02
Oxyopes dingo Strand, 1913
Oxyopes rubicundus L. Koch, 1878
Genus 1 sp.01
Genus 1 sp.02
Trichocyclus arabana Huber, 2001
Trichocyclus nigropunctatus Simon, 1908
Cryptoerithus halli Platnick & Baehr, 2006
Cryptoerithus occultus Rainbow, 1915
Family
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oxyopidae
Oxyopidae
Oxyopidae
Oxyopidae
Philodromidae
Philodromidae
Pholcidae
Pholcidae
Prodidomidae
Prodidomidae
Appendix B cont.
5
8
20
3
1
0
0
0
0
4
0
0
1
0
0
0
7
1
3
46
1
0
0
0
9
0
0
14
0
0
1
15
5
0
1
0
0
6
2
0
3
41
0
0
1
0
23
143
0
1
2
0
0
1
9
5
0
0
0
0
0
1
0
6
56
0
1
1
0
12
0
2
2
0
0
1
14
1
0
0
0
0
0
1
0
0
28
1
0
0
0
2
1
1
1
6
1
0
14
1
0
0
0
3
3
7
0
0
86
0
0
0
1
32
0
3
15
2
0
0
11
0
1
0
1
2
9
15
0
1
64
0
0
1
0
59
37
22
42
45
20
15
24
39
20
19
20
36
27
28
25
30
19
14
20
15
20
26
0
20
0.5
8
8*
0.5
0.5
3
20*
0.5
20*
8
20
20
0*
3
8
0
3*
0.5
8*
20
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
0.069
0.017
0.398
0.037
1.000
0.029
0.549
0.050
1.000
0.340
1.000
0.073
0.035
0.285
0.263
0.157
0.378
0.570
1.000
0.550
1.000
0.124
p
1
0
3
0
Molycria vokes Platnick & Baehr, 2006
Nomindra sp.01 (cf. cooma)
Nomindra sp.02
Nomindra leeuweni Platnick & Baehr, 2006
Wesmaldra learmonth Platnick & Baehr, 2006
Wydundra sp.03
Wydundra sp.04
Wydundra kennedy Platnick & Baehr, 2006
‘Clynotis albobarbatus grp.' sp.10
Damoetas sp.13
Damoetas sp.17
Genus 1 sp.02 'big embolus grp.'
‘Neon' sp.15
Genus 1 sp.23
Genus 1 sp.27 'big embolus grp.'
Grayenulla sp.01
Holoplatys sp.07 (cf. planissima)
Holoplatys sp.14
Lycidas sp.08
Lycidas grp. sp.11
Lycidas grp. sp.12
Lycidas chlorophthalmus (Simon, 1909)
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
5
8
20
0
1
0
0
0
0
0
4
0
0
0
0
0
0
10
1
8
0
0
0
0
17
0
0
3
11
0
0
0
0
1
0
0
0
0
0
12
0
1
0
144
1
0
0
5
0
0
4
23
0
0
2
0
0
0
3
0
0
1
124
2
30
0
1
1
0
12
1
1
8
23
0
0
3
0
0
0
1
0
1
0
25
0
49
0
0
0
3
7
0
0
4
19
0
0
0
0
0
1
1
0
1
0
60
0
16
0
0
0
1
15
0
0
4
32
1
1
0
1
0
0
5
7
2
0
3
0
5
1
10
14
28
21
20
20
21
21
20
20
26
20
33
20
14
60
20
20
29
25
18
20
3
0
8
20
5*
5*
5
20
20*
20*
0
20*
0.5*
8*
20
20*
20
3*
3
3
3
20*
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
Species
Family
Appendix B cont.
1.000
0.570
0.224
0.550
1.000
1.000
0.420
0.775
1.000
1.000
0.175
1.000
0.112
1.000
0.016
0.643
0.400
0.006
1.000
0.347
0.766
1.000
p
1
0
Ocrisiona yakatunyae Żabka, 1990
Paraplatoides sp.03
Paraplatoides sp.06
Pellenes bitaeniata (Keyserling, 1882)
Zebraplatys keyserlingi Żabka, 1992
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.07
Genus 1 sp.08
Genus 1 sp.12
Genus 1 sp.13
Hadrotarsus sp.10
Hadrotarsus sp.11
Latrodectus sp.09
Steatoda sp.01
Steatoda sp.02
Steatoda sp.03
Steatoda sp.04
Steatoda sp.05
Genus 1 sp.01
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Segestriidae
Segestriidae
Sparassidae
Sparassidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Thomisidae
5
8
20
0
0
2
4
5
27
1
0
0
0
0
0
0
1
0
5
0
0
0
1
0
1
1
0
11
9
1
0
0
2
1
0
0
0
0
0
0
1
1
0
0
6
145
0
1
0
2
9
3
0
0
0
2
0
0
0
0
0
0
0
1
0
0
0
6
1
1
0
0
7
8
1
0
1
0
0
0
1
0
0
0
0
0
1
1
1
1
0
9
0
1
6
8
0
0
1
0
0
2
0
1
1
1
3
1
0
0
2
1
0
1
7
2
12
3
1
2
1
0
9
0
0
3
0
0
1
1
0
0
1
1
20
41
19
33
21
31
11
40
7
20
25
40
20
20
20
60
45
12
14
20
8
20
5*
8
0
0
0.5
0
0.5
20*
20
3
20
8*
5*
20
8*
0
8
0.5
0.5
5*
8
3
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
Species
Family
Appendix B cont.
0.030
1.000
0.332
0.031
0.100
0.024
0.855
0.145
1.000
0.394
0.279
0.142
1.000
0.387
0.007
1.000
0.044
0.753
0.629
1.000
1.000
0.545
p
Species
Genus 1 sp.02
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Stephanopis sp.03
Fissarena castanea (Simon, 1908)
Australutica quaerens Jocqué, 1995
Australutica sp.01 (cf. quaerens)
Cavasteron sp.32 (cf. crassicalcar)
Genus 1 sp.31
Genus 1 sp.33
Genus 1 sp.34
Habronestes bicornis Baehr, 2003
Habronestes sp.13 (cf. longiconductor)
Habronestes sp.16 (cf. grahami)
Habronestes sp.18 (cf. hamatus)
Habronestes sp.21
Habronestes sp.30
Masasteron piankai Baehr, 2004
Neostorena sp.02
Neostorena sp.03
Neostorena sp.05
Family
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Trochanteriidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Appendix B cont.
5
8
20
0
1
6
8
14
0
0
0
0
0
2
0
2
1
5
0
4
1
0
0
0
0
0
0
1
8
0
0
0
0
0
0
2
0
1
10
3
0
2
0
0
0
0
2
146
0
0
5
0
25
0
1
0
0
0
0
1
4
1
2
5
0
0
0
0
1
0
0
0
2
1
2
1
0
0
2
1
0
0
2
0
3
13
4
0
1
0
0
0
1
0
4
4
8
0
0
0
0
0
1
0
6
5
16
9
5
0
0
1
0
0
0
0
0
17
0
0
0
2
1
0
0
0
2
14
3
4
20
0
0
0
1
0
20
25
16
28
27
20
20
40
11
20
23
20
15
28
27
30
44
25
20
20
10
67
8*
0*
3
20
3
5*
3*
20*
5
5*
0
3*
8
0.5
0
5
20
0*
5*
8*
3
0.5*
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
1.000
0.262
0.862
0.207
0.215
1.000
1.000
0.145
1.000
1.000
0.189
1.000
0.785
0.175
0.292
0.008
0.117
0.262
1.000
1.000
0.009
1.000
p
Species
Spinasteron cavasteroides Baehr & Churchill, 2003
Argoctenus sp.01
Argoctenus sp.02
Argoctenus sp.03
Argoctenus sp.04
Argoctenus sp.05
Argoctenus sp.08
Genus 1 sp.10
Family
Zodariidae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Appendix B cont.
5
8
20
0
0
0
0
0
0
4
1
0
0
0
1
0
0
2
0
147
0
0
0
0
0
0
9
0
0
0
0
0
0
2
8
0
0
0
0
0
0
8
17
1
2
4
1
1
1
6
5
6
40
60
20
21
20
26
27
36
20*
20*
20*
0.5
20*
8
8
20
Age
IndVal
3
0
0.5
Indicator analysis
Post-fire age
0.016
0.136
1.000
0.314
1.000
0.001
0.206
0.096
p
Comparison
Post-fire
age
0 vs 0.5
0 vs 3
0 vs 5
0 vs 8
0 vs 20
0.5 vs 3
0.5 vs 5
0.5 vs 8
0.5 vs 20
3 vs 5
3 vs 8
3 vs 20
5 vs 8
5 vs 20
8 vs 20
Unique
perms
35
126
126
126
126
56
56
56
56
126
126
126
126
126
126
t
0.662
5.507
2.378
0.745
1.260
5.423
1.842
0.222
2.018
2.547
3.961
7.220
1.456
3.779
1.939
Richness
p values
perm
0.661
0.008
0.065
0.534
0.231
0.017
0.138
0.911
0.108
0.049
0.020
0.009
0.165
0.008
0.093
MC
0.529
0.001
0.049
0.487
0.247
0.001
0.115
0.829
0.090
0.034
0.004
0.000
0.181
0.005
0.089
are provided with significant (< 0.05) p values in bold.
148
Berger-Parker
p values
t
perm
0.126 0.914
3.142 0.009
2.566 0.031
1.341 0.229
0.321 0.757
5.918 0.018
3.475 0.021
2.544 0.053
0.235 0.861
0.180 0.820
3.647 0.023
5.319 0.008
2.259 0.076
3.954 0.016
2.543 0.057
MC
0.910
0.018
0.038
0.220
0.759
0.001
0.012
0.044
0.817
0.865
0.007
0.001
0.051
0.004
0.034
Species composition
p values
t
perm
MC
1.381 0.027
0.130
2.060 0.008
0.007
1.806 0.008
0.016
1.666 0.006
0.030
1.842 0.017
0.014
1.547 0.018
0.050
1.531 0.035
0.064
1.566 0.015
0.054
1.345 0.035
0.127
1.335 0.039
0.121
1.636 0.007
0.026
2.158 0.009
0.005
1.125 0.111
0.283
1.613 0.015
0.034
1.527 0.008
0.042
(PERMANOVA pair-wise tests). For each comparison the value of the test statistic (t) and both permutational (perm) and Monte Carlo (MC) values
Differences in species richness, Berger-Parker index and species composition between post-fire ages from a permutational analysis of variance
Appendix C
Species
Poecilipta sp.03
Supunna picta (L. Koch, 1873)
Phryganoporus sp.01
Eilica sp.11
Encoptarthria sp.08
Genus 1 sp.05
Genus 1 sp.06
Miturga sp.05
Kwonkan sp.01
Cavisternum sp.07
Myrmopopaea sp.05
Opopaea sp.13
Trichocyclus nigropunctatus Simon, 1908
Nomindra sp.01 (cf. cooma)
Nomindra leeuweni Platnick & Baehr, 2006
Family
Corinnidae
Corinnidae
Desidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Miturgidae
Nemesiidae
Oonopidae
Oonopidae
Oonopidae
Pholcidae
Prodidomidae
Prodidomidae
dis/similarity and cumulative contribution.
0.73
0.60
0.77
1.08
1.44
1.70
0.88
1.06
0.79
0.88
1.12
1.10
0.59
1.80
0.87
1.69
1.07
0.33
0.49
0.83
0.36
0.49
0.27
0.72
0.47
0.44
0.53
0.84
2.45
0.07
149
0.61
0.45
0.66
1.64
2.03
2.86
1.1
1.6
0.66
0.81
1.34
1.07
0.45
3.04
0.85
average
0/0.5/20
3/5/8
Similarity
Average abundance
0.66
0.53
0.66
2.12
2.11
8.01
1.07
2.14
0.66
0.84
1.06
0.77
0.53
8.15
0.66
/SD
1.30
0.96
1.41
3.49
4.31
6.07
2.34
3.40
1.39
1.72
2.84
2.26
0.95
6.44
1.81
(%)
Cont.
40.69
39.39
38.43
37.02
33.53
29.22
23.15
20.81
17.41
16.02
14.30
11.46
9.20
8.25
1.81
(%)
Cumul.
1.11
0.89
0.71
0.69
0.88
1.40
0.66
0.84
0.72
0.77
0.89
1.03
0.87
0.69
0.88
average
Dissimilarity
1.49
1.28
1.16
1.25
1.34
2.14
1.19
1.61
1.22
1.18
1.41
1.24
1.23
1.68
1.16
/SD
1.88
1.51
1.20
1.17
1.49
2.37
1.11
1.42
1.21
1.30
1.50
1.74
1.47
1.16
1.49
(%)
Cont.
22.02
20.14
18.63
17.43
16.26
14.77
12.40
11.29
9.87
8.66
7.36
5.86
4.12
2.65
1.49
(%)
Cumul.
within age groups along with average dis/similarity, dis/similarity divided by standard deviation (SD), percentage contribution to the total average
similarity between the experimentally burnt (0 and 0.5 years) and the long unburnt sites (20 years). For each species, there is the average abundance
(versus 3, 5 and 8 years combined) from an analysis of similarity percentages (SIMPER). These species are therefore important contributors to the
The twenty species that contributed the most to average Bray-Curtis similarity within the group (0, 0.5 and 20 years combined) and between groups
Appendix D
Species
Genus 1 sp.27 'big embolus grp.'
Lycidas sp.08
Steatoda sp.01
Fissarena castanea (Simon, 1908)
Masasteron piankai Baehr, 2004
Family
Salticidae
Salticidae
Theridiidae
Trochanteriidae
Zodariidae
Appendix D cont.
0.91
0.87
1.10
0.73
1.18
0.16
0.26
0.58
0.65
1.06
150
0.92
0.93
1.44
0.54
1.69
average
0/0.5/20
3/5/8
Similarity
Average abundance
0.83
0.85
1.33
0.52
2.06
/SD
1.94
1.97
3.06
1.15
3.57
(%)
Cont.
52.38
50.44
48.47
45.41
44.26
(%)
Cumul.
0.85
0.79
0.81
0.76
0.69
average
Dissimilarity
1.30
1.26
1.30
1.21
1.23
/SD
1.44
1.33
1.36
1.29
1.17
(%)
Cont.
28.61
27.17
25.84
24.48
23.19
(%)
Cumul.
CHAPTER 3
Untangling the drivers of structure in animal assemblages in
arid ecosystems: the influence of fire, rainfall, vegetation,
predators and spatial structure on spiders (Araneae)
Peter R Langlands
Karl E C Brennan
Bruce Ward
Formatted for Ecography
151
Abstract
A vast array of variables can act singly or in combination to influence an area‟s biota. A
critical challenge in ecology is to understand the degree to which these variables, or
combination of variables, influence assemblages of species. For those variables under
anthropogenic control, such knowledge also assists prioritising actions to conserve
biodiversity. In arid Australia, fire and rainfall are two key and potentially interacting
forces that contribute in shaping assemblages of plants and animals. However, the degree to
which spatial processes, environmental variables and biotic processes combine with fire
and rainfall to shape assemblages of animals remains poorly quantified. Using a
chronosequence approach in spinifex habitat we studied the influence of fire (0-20 years
previously) on spiders, while also examining the short-term effect of rainfall, the influence
of space, environmental variables (Soil, Floristics, Habitat structure) and biotic processes
(Predation by scorpions, small insectivorous mammals and reptiles). Predictor variables
explained 79% of the variation in species richness and 32% in composition of spiders using
distance-based redundancy analysis. Variation partitioning identified post-fire age as
explaining the largest proportion of this variation, 61% for species richness and 78% for
composition. However, spatially and non-spatially structured vegetation variables
(Floristics and Habitat structure) explained much of this variation. Rainfall explained a
large proportion of the explained variation for species richness (59%), but not species
composition (30%). There was little variation attributable to predation (0 & 14% for
species richness and composition, respectively) or pure spatial structure (5 & 5%). These
findings provide support for environmental variables structuring assemblages of spiders in
the arid zone and suggest that actively managing fire effects on habitat structure and
floristics is critical to conserving spider biodiversity.
152
Introduction
Quantifying the degree to which different variables interact in structuring assemblages of
animal and plant species is a central theme in community ecology (Quinn and Dunham
1983, Parris 2004, Cottenie 2005, Driscoll and Lindenmayer 2009, Legendre et al. 2009).
Environmental conditions can structure the species composition of assemblages (e.g.
species-habitat or niche-based models Whittaker 1956, Bray and Curtis 1957). This concept
appears similar to the species sorting perspective within metacommunity theory (see
Leibold et al. 2004). Additionally, biotic processes (dispersal, competition, mortality and
predation) can structure species composition (Hairston et al. 1960, Paine and Vadas 1969,
Connell 1983). Historical legacies from past natural (fires, droughts and storms) or
anthropogenic events (clearing and agriculture), may impose further structure on species
composition (e.g. Sousa 1984, Pickett and White 1986, Borcard and Legendre 1994).
Ecologists now recognise that variables can consist of spatially and non-spatially structured
patterns (Legendre and Legendre 1998). Spatially structured environmental variables can
produce spatial patterns in assemblages, as species track their habitat (Fortin and Dale
2005, Legendre and Legendre 1998). Alternatively, the biotic processes described above
may be contagious, with sites closer together being more similar in species composition
(Legendre 1993). The latter reveals itself as a pure effect of spatial location on assemblages
of species (Borcard et al. 1992). There is, however, a dearth of empirical studies
quantifying the influences of environmental variables and spatial processes for terrestrial
invertebrates in arid ecosystems in the Southern Hemisphere (Cottenie 2005).
Quantifying the pure and interacting influences of an often-vast array of environmental,
biotic and historical variables (while explicitly considering the influence of space) on
assemblages of species is a crucial, but formidable challenge. Although methods such as
variation partitioning have existed for more than 15 years (Borcard et al. 1992, Borcard and
Legendre 1994), it is only recently that such techniques have been refined (e.g. Peres-Neto
et al. 2006) and become widely accessible (e.g. Oksanen et al. 2008). Indeed, until the
recent development of a recursive algorithm by Økland (2003), such analyses have been
limited to no more than four groups of variables. These developments permit answers to
fundamental but hitherto unresolved questions for many land managers seeking to conserve
biodiversity, where there are many potential variables influencing assemblages of species.
Such questions include: 1) how much of a system is under anthropogenic control (Pozzi
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and Borcard 2001, de Warnaffe and Dufrene 2004)? and 2) how much of the composition
of species are they likely to be able to influence solely by influencing environmental
conditions? The latter question recognises that control of intrinsic processes within an
assemblage may not always be possible or desirable.
Fire and rainfall are two variables that ecologists have long recognized as potentially
important in governing the structure of faunal assemblages in arid ecosystems (Stafford
Smith and Morton 1990, Masters 1993, Letnic et al. 2004, Langlands et al. 2006) (Fig. 1,
arrow 1). For example, within the vast arid zone of Australia the vegetation is highly
flammable, and large swathes (> 10 000 km2) can be burnt due to lightning strikes and
human ignition (Allan and Southgate 2002, Turner et al. 2008). Additionally, extensive use
of fire by Aboriginal people can create a landscape characterised by a mosaic of different
post-fire ages (Burrows et al. 2006, Bird et al. 2008). In arid Australia, many studies
document marked changes in assemblages of animals following fire for vertebrates as well
as some invertebrate groups (Gunawardene and Majer 2005, Letnic et al. 2004, Smith and
Morton 1990). Rainfall is highly variable, leading to populations of many species
undergoing a cyclic pattern of boom followed by bust (Masters 1993, Dickman et al.
1999a, b). This is because massive downpours, often associated with low-pressure systems
that are the remnants of cyclones (hurricanes), occasionally interrupt long periods of
drought. For example, our study location received 110 mm, nearly half the median annual
rainfall, in just two days in January 2007 (Langlands unpubl. data).
It is important to appreciate, however, that fire and rainfall can be linked. Fuel-load and
fire-interval are strongly influenced by rainfall, with more fires following periods of high
rainfall (Turner et al. 2008, Fig. 1 arrow 2), making it important to consider the influence
of rainfall when examining faunal responses to fire (Blanche et al. 2001, Letnic et al. 2004,
Langlands et al. 2006, Fig. 1 arrow 3). Yet it remains poorly quantified to what degree fire,
rainfall and the interplay of these or other variables can explain variation in assemblages of
species. Here we consider this question on an assemblage of spiders.
Other variables, such as habitat structure, exert strong influences on assemblages of
spiders, with simplification of structure decreasing abundance (see meta-analysis by
Langellotto and Denno 2004). Experimental manipulations of habitat structure that increase
complexity cause increases in abundance and species richness and can alter species
composition of spiders (Uetz 1979, Gunnarsson 1990, Hatley and MacMahon 1980, Fig. 1
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arrow 4). In our system, the dominate ground cover, spinifex grass (Triodia basedowii), is
removed by fire, and with sufficient rainfall, grows gradually with increasing time since
fire. This leads to a gradual increase in the vertical structure of vegetation over time as
spinifex and long-lived plants develop (Griffin 1992, Fig.1 arrow 5).
Floristics and soil properties may also influence assemblages of spiders (Owen 2004,
Beals 2006, Schaffers et al. 2008, Fig. 1 arrows 6 and 7). Marked difference in species
composition of spiders among species of plants may arise through differences in
architecture of plants, flowering and the species of prey used by spiders (Robinson 1981,
Uetz 1991). The species richness of vegetation in spinifex habitats increases rapidly after a
fire with the germination of many short-lived herbs, forbs and grasses (Allan and Baker
1990, Fig. 1 arrow 8). Reduced competition from spinifex and increased nutrients
following the fire aid the flush of plant growth (Griffin 1990, Fig. 1 arrow 9). Within three
years, the flush of plants following the fire will senesce, but the shrubs, trees and spinifex
are still establishing.
While many studies have implicated post-fire changes in vegetation as driving post-fire
changes in faunal assemblages within the Australian arid zone, there has been far less
consideration of other processes, such as predation and parasitism. For spiders, these are
potentially important variables. Many studies have demonstrated strong top-down control
from predacious birds and lizards causing decreases in abundance or species richness of
spiders (Evelegh et al. 2001, Spiller and Schoener 1988, 1998, Gunnarsson 2007, Manicom
et al. 2008, Fig. 1 arrow 10). Indeed, in a global context, the reptile fauna of our study site
is exceptionally rich (Pianka 1969). However, rainfall, seasonality and perhaps habitat
structure can mediate the strength of top-down control (Gunnarsson 1990, Recher and
Majer 2006, Spiller and Schoener 2008, Fig. 1 arrow 11). Parasitoids and intraguild
predation can also exert strong influences by decreasing the abundance of spider
populations (Polis et al. 1989, 1998, Wise 1993, Fig. 1 arrow 12).
The aim of our study was to use variation partitioning to quantify the degree to which
fire, rainfall, along with environmental and biotic variables and spatial processes, combine
to shape a spider assemblage within fire-prone spinifex grasslands of arid Australia.
Although our approach is clearly correlative, it is an important initial step for determining
which variables might be most influential and generating hypotheses of potential causal
mechanisms (Legendre and Legendre 1998).
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Materials and methods
Study area and design
Our study was conducted in central Western Australia at the proposed Lorna Glen
(Matuwa) Conservation Park, located approximately 150 km NE of Wiluna (Fig. 2). Lorna
Glen contains a range of habitat types with the most widespread of these being the fireprone hummock grasslands (Bullimore). This is a vegetation assemblage dominated by
spinifex Triodia basedowii E. Pritz, 1918, an over storey of marble gums (Eucalyptus
gongylocarpa Blakely, 1936) with scattered mulga (Acacia aneura Benth, 1855) and
mallee (E. kingsmillii Maiden and Blakely, 1929 and E. lucasii Blakely, 1934).
We conducted our study at the landscape scale, with 27 sites selected to represent a range
of fire and potentially rainfall histories (described below) (Fig. 2). At each site, a 50 x 50 m
quadrat was established a minimum of 150 metres from the site boundary (change in fire
age) or road.
Fire history
We used Landsat satellite images from 1988 to 2005 to establish the fire history of the
study area. From these natural fire histories and some experimental fires, six treatments for
post-fire ages were selected: 0, 6 months, 3, 5, 8 and 20 plus years since the last fire. There
were three to five sites per post-fire age (Fig. 2). Patch size for each site was at least 9 ha.
To establish some recently burnt sites, seven sites that had not been burnt for at least
twenty years were burnt experimentally (three sites were burnt October 2005 [0.5 years
treatment] and four sites were burnt April 2006 [0 years treatment]). For details of fire
ignition procedure and weather conditions during burning see Langlands et al. (accepted).
Rainfall
Twenty-six rain gauges (Davis tipping buckets [165 mm diameter, 0.2 mm accuracy ± 5%
at 100 mm/hr] connected to Odyssey data loggers
[http://www.odysseydatarecording.com]), were installed within 200 m of most sites in
August 2005 (for site 8-1 the nearest gauge was 1500 m away). We installed rain gauges on
200 L (44 gallon) drums (~ 850 mm high), which we positioned from surrounding
vegetation at a distance of at least twice the height of the vegetation (Australian Bureau of
Meteorology). We ensured gauges were level.
156
We calculated the total monthly rainfall at each site from August 2005 to January 2007,
along with total rainfall for blocks of three and six months. The total rainfall before
trapping (August 2005 – April 2006) and total rainfall during trapping was also calculated.
Habitat structure and floristics
We used the line intercept method to estimate vegetation cover and structure. At each plot
taut measuring tapes along the diagonals created two 70 metre transects (140 metres total).
Using a pole marked in 5 cm sections we recorded the ground cover (height ≤ 50 cm) and
over storey cover (height > 50 cm). At each point on the tape where there was a change in
ground cover we recorded the distance and cover category. We did not record cover
changes of less than 5 cm length. There were eight categories of ground cover: bare
ground, live spinifex, dead spinifex, leaf litter, grass, dead grass, woody shrub and dead
woody shrub. Over storey cover was recorded as the length of transect covered by
vegetation in six categories: alive or dead vegetation of either woody shrubs, marble gums
or mulga. The proportion of each category of ground cover and over storey for the two
transects was calculated and averaged, giving the average proportion of ground covered by
each category of ground cover and over storey for a site.
We recorded the composition of plant species within each quadrat (50 x 50 m) at each
site. The abundance of each species was scored in five categories: 1, 2-10, 11-50, 51-100
and >100 plants.
Soil
Soil texture, pH, conductivity, organic carbon (%), and the concentration of nitrogen,
ammonium, phosphorus, potassium and sulphur were assessed using a sample of the top
5cm of soil. This was collected 1 m from each pitfall trap in August 2006 and bulked for
each site.
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Predators
As a measure of potential predation pressure, we used scorpions and an unintended bycatch of small mammals (Dasyuridae) and reptiles that prey on spiders caught in pitfall
traps. For each site, we calculated the abundance and species richness of reptilian and
mammalian predators, along with abundance of scorpions.
Spatial
We used trend surface analysis with the easting and northing values of sites from Universal
Transverse Mercator (UTM) coordinates used to create polynomial combinations up to the
third order with Spacemaker2 (Borcard and Legendre 2002). An irregular distribution of
sites over the study area prevented the use of principal coordinate analysis of neighbour
matrices (PCNM, Borcard and Legendre 2002).
Sampling and identification of spiders
Each quadrat contained five pitfall traps, which we opened 30 April 2006 and exchanged at
three-monthly intervals until 18 January 2007 (256-258 days per trap session). We
combined the data for each pitfall trap and collection period to give one sample per site.
We identified spiders to species level. It is very difficult to match males, females and
juveniles of the same species correctly, because taxonomic knowledge of the Australian
spider fauna is particularly poor compared with the northern hemisphere (Brennan et al.
2004). To avoid identification errors the results presented here are from males only with
species boundaries verified by taxonomic experts. For further details of the pitfall trapping
and identification procedures see Langlands et al. (accepted).
Data analysis
Spiders
To test for differences in abundance, species richness and species composition of male
spiders, we used a permutational analysis of covariance (Legendre and Anderson 1999,
Anderson 2001) with the fixed factor AGE (levels 0, 0.5, 3, 5, 8 and 20 years). As the
spatial coordinate northing3 explained the most variation with step-wise selection, it was
subsequently used as a covariate to account for the influence of site locations. These
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analyses used PERMANOVA+ (Anderson et al., 2008, version 1.01). To account for
differences in abundance between sites, prior to analysis, we rarefied the richness of
species using PRIMER (Clarke and Gorley, 2006, version 6.1.11) to the minimum number
of spiders collected from a site (85 males). For analyses of species composition, the
abundance of each species of spider was fourth root transformed, to decrease the influence
of abundant species and Bray-Curtis similarity calculated. To visualise the correlation of
selected explanatory variables with species composition we used distance-based
redundancy analysis (db-RDA, McArdle and Anderson 2001).
Throughout the paper we treat statistical tests with p < 0.05 as significant, unless
otherwise specified. We have not corrected for multiple tests (e.g. pair-wise
PERMANOVA), preferring to present the raw p and data values, allowing the reader to
decide significance (see Moran 2003).
Variation partitioning
We used the distance-based linear models (DISTLM) function in PERMANOVA+ to
perform variation partitioning. This allowed us to choose an appropriate similarity measure
for the data, Euclidean distance for richness and Bray-Curtis similarity for composition of
species. As the DISTLM function fits a linear model, we transformed predictor variables to
improve normality. We took the natural logarithm of soil variables, except for pH. Habitat
proportions were arcsine transformed, with Predator and Rainfall variables square root
transformed. To allow for non-linear relationships between the predictors and response
variables we calculated the squares and cubes of variables (Rainfall, Habitat, Soil and
Predators) after centering data on their means (Makarenkov and Legendre, 2002; Jones et
al., 2008). We coded post-fire age as a dummy variable to allow a non-linear response and
the fire age surrounding each site was included as a variable. The similarity between sites
in floristic composition was calculated using Bray-Curtis similarity. Principal coordinates
analysis (PCO) was then used to reduce the dimensionality of the floristic data to make it
suitable for incorporation into variation partitioning analysis.
For each group of explanatory variables (Fire, Rainfall, Habitat, Floristics, Soil, Predators
and Spatial, see Fig. 1), we used step-wise selection (9999 permutations) to identify
variables which explained a significant (p < 0.01) amount of variation in the species
richness or species composition of spiders. We were conservative in our selection of
159
variables for variation partitioning, as like regression, it is not possible to have more
explanatory variables than sites. Although the selection process chose variables with the
highest explanatory power, many variables within a group are likely to be inter-correlated.
Therefore, we used spearman correlation to find variables that had a correlation (> 0.60)
with the selected variables.
We used adjusted R2 values to allow comparison between groups with differing numbers
of variables selected (Peres-Neto et al., 2006). Adjusted R2 values are also displayed as a
percentage of the total variation explained, as it is more important and informative to
compare the relative amounts of variation explained between groups rather than the
absolute amount (Økland, 1999). This approach is also more useful for comparisons
between studies.
As the number of explanatory groups (n) included in variation partitioning increases, the
number of components also increases (2n-1). We therefore used the simplification method
of Økland (2003) to show only the significant components. This uses a value (l) as a
threshold to decide what higher order components are large/significant enough to be kept
and which higher order components should be distributed onto lower orders (see Økland,
2003, and calculations provided in Appendix B (supplementary online material)). We used
the more conservative method of calculating l, which uses the variation explained by single
predictor variables that corresponds to a chosen significance level (p = 0.05).
Results
Of the 14 104 spiders collected, nearly half were adults (48.6%), of which most were males
(61.8%, 4 234 specimens). The males represented 179 species from 24 families, with only
32 species formally described.
The predator by-catch considered to prey on spiders consisted of 426 vertebrates (313
reptiles and 113 mammals) and 172 scorpions. These represented 26 species of reptile
species, 5 mammals and an unknown number of species of scorpion.
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Abundance
Abundance of male spiders ranged from 85 to 250 individuals per site. There was no clear
pattern or significant difference in the abundance of spiders with post-fire age, based on a
permutational analysis of covariance; therefore we did not consider the data further (d.f. 5,
20; pseudo-F = 0.695, p = 0.62).
Species richness
Rarefied species richness of spiders ranged from 18.9 to 38.1 species per site, with the
lowest mean richness found in 3-year-old sites. The spatial covariate northing3 was
significant, and results reported henceforth are adjusted accordingly. Species richness,
varied significantly (Table 1), with similar richness at the experimentally burnt and 8-yearold sites, but with richness increasing with post-fire age from 3 to 20 years (Fig. 3a). Pairwise tests revealed significantly fewer species at 3-year-old sites than at the 0, 0.5, 8 and
20-year-old sites (Table 1). The 20-year-old sites had significantly more species than the
0.5- and 5-year-old sites.
In comparison, the post-fire response of the species richness of plants did not display the
same pattern. Plant richness increased rapidly in the first six months following fire, but
subsequently decreased, increased and decreased in the following years (Fig. 3a). Habitat
structure was markedly different between post-fire ages. For example, bare ground
increased from around 40%, to over 90% immediately after fire, but decreased over time to
return to 40% after 20 years (Fig. 3b). Part of this increase in bare ground was due to the
removal of live spinifex, which gradually regrew with increasing time since fire (Fig. 3b).
Eight explanatory variables from five groups (Fire, Rainfall, Habitat, Floristics and
Spatial location of the study sites) explained 79% of the total variation in the species
richness of spiders (Table 2). While the variables selected for Rainfall (Jan 20072, Nov
20053), Habitat (bare ground2) and Spatial (northing3) were the best in terms of explanatory
power, they were also correlated with several other variables within each group (Appendix
C). Rainfall in January 20072 was strongly correlated with rain from February to April in
2006, while November 20053 was correlated with rainfall during July to November 2006
(Appendix C). The Habitat variable bare ground2 was correlated with woody shrub cover,
as well as with dead and live spinifex.
161
Overall, Fire (61%) and Rainfall (59%) explained the greatest amounts of the total
variation explained, followed by Floristics (47%), Spatial (41%) and Habitat (22%) (Fig.
4). That said, there was a large degree of overlap between groups, with 51% of the total
variation explained shared in common between three or more groups (Fig. 4). All groups
shared 14% of the total variation explained, with Fire, Rainfall and Spatial sharing a further
22% in common. Fire, Rainfall and Floristics also shared 15% of the explained variation
(Table 2).
Species composition
Adjusting for the spatial covariate northing3, there were marked differences in the species
composition of spiders with increasing post-fire age (Table 3). Previous analyses indicated
a clear pattern from 3 years, to 5, 8 and 20 years since fire, while the experimentally burnt
(0 and 0.5 years since fire) sites were located away from the other ages (Langlands et al.
accepted). Pair-wise comparisons showed that the most recently burnt sites (0 years)
differed significantly from all other post-fire ages. Similarly, the long unburnt sites (20
years) differed significantly from all other ages, except 0.5 years (Table 3). Other
differences between site ages are shown in Table 3.
Partitioning of the variation in the species composition of spiders found that twelve
explanatory variables, representing six groups (Fire, Rainfall, Habitat, Floristics, Predators
and Spatial location), were significant in explaining 32% of the variation (Table 4). The
selected Rainfall variable (Feb-Apr 2006) was strongly correlated with rainfall from
February to July 2006 and January 2007 (Appendix C). Likewise, the selected Habitat
variables (live and dead spinifex) correlated strongly with themselves, and upper storey
woody shrubs. Predictably, the Predator variable of reptile abundance was correlated with
the number of reptile species and the spatial variable northing3 was correlated with
northing, as for species richness (Appendix C).
Five groups of variables (Fire, Rainfall, Habitat, Floristics and Spatial) shared 28% of the
total variation explained (Table 4). Fire, Habitat and Predators also shared 11%, with Fire
and Habitat explaining a further shared 19%. Fire explained the greatest proportion of the
total variation explained (78%) followed by Habitat (64%), Floristics (34%), Spatial (33%),
Rainfall (30%) and Predators (14%) (Table 4, Fig. 4). Similar variation partitioning results
were also obtained using the Hellinger transformation with traditional Redundancy
162
Analysis (RDA), indicating a high degree of robustness to similarity measure and
ordination technique.
A constrained ordination (distance-based RDA) of the species composition, using the
selected explanatory variables, identified which ages and variables were strongly correlated
(Fig. 5). The first axis was dominated by the Age of surrounds, being positively correlated
with recently burnt and long unburnt sites (all surrounded by 20+ years). The second axis
was strongly correlated with live spinifex, greater in older sites, as well as abundance of
reptiles and rainfall between February to April 2006, which were higher in recently burnt
sites. The Floristics principal coordinate 2 was strongly positively correlated with the third
axis (not shown).
Discussion
Untangling the myriad of variables influencing assemblages of species is a critical
challenge for developing a deeper mechanistic understanding of arid ecosystems, allowing
better management to conserve biodiversity. In this study, we have quantified for the first
time the degree to which Rainfall, Habitat structure, Floristics, Predators, Soil and Spatial
pattern explain the variation in an arid assemblage of spiders following disturbance by fire.
Although post-fire age explained the greatest amount of the variation explained for species
richness (61%) and composition (78%) of the spiders, much of this variation was also
explained by Floristics or Habitat structure (i.e. was not unique to fire). This suggests fire is
instrumental in shaping the plant assemblage, which in turn exerts a strong influence on the
spider assemblage. The variables representing Fire, Rainfall, Floristics and Habitat also
shared most of the variation explained by spatial location, suggesting that where the
landscape burnt and rain fell, along with underlying environmental gradients, generated
spatial structure in the vegetation to which the spiders are responding. The spider
assemblage we studied is explained best by changes in vegetation, which in turn is strongly
influenced by fire, with only a minor contribution of predators or intrinsic species processes
at this scale.
There was very little pure spatial structuring or spatial autocorrelation, which would have
provided support for contagious species processes (Borcard and Legendre 1994, Legendre
and Legendre 1998). Additionally, the crude measures of Predators we included failed to
account for any variation in species richness and explained only a minor part of species
163
composition. This suggests that the contribution of contagious species processes is small
relative to fire and rainfall mediated changes in vegetation. These findings provide strong
support for land managers wishing to conserve spider biodiversity in arid Australia: they
can have a large influence on the spider community through changes to the habitat and
floristics, particularly via fire. However, they will need to consider carefully the influence
of rainfall on the fire regime, as rainfall is largely beyond anthropogenic control.
Despite there being strong arguments as to why the top-down control via predators might
be particularly important in structuring assemblages of spiders (see introduction), our
results are consistent with findings from a recent meta-analysis across a range of non-spider
taxa in predominantly Northern Hemisphere temperate ecosystems. Cottenie (2005) found
that environmental variables were dominant, and the spatial or neutral processes were
important for only a few communities. Our results are also consistent with two previous
studies of spiders that have included environmental variables and spatial location, but did
not explicitly consider predators (Pozzi and Borcard 2001, Jeanneret et al. 2003).
Environmental variables and spiders
As noted above, amongst our explanatory variables, post-fire age explained the most
variation of species richness and composition of spiders. This result was expected, given
that, firstly, vegetation structure and floristics are well known to change in spinifex habitats
as greater time elapses following burning (see Introduction). Although habitat structure in
our study changed as described in previous work, changes in the species richness of plants
were less congruent. Although species richness of plants increased rapidly after the
experimental fires, and decreased by three years, there was not a consistent decline
thereafter. It is not clear why our results differ. Secondly, assemblages of spiders respond
strongly to alterations in habitat structure and floristics (discussed below).
The finding of a large amount of the variation explained by habitat structure is consistent
with many studies and the long-held importance of habitat in determining assemblages of
spiders (Hatley and MacMahon 1980, Robinson 1981, Halaj et al. 1998, 2000, Heikkinen
and MacMahon 2004, Brennan et al. 2006). Several mechanisms may explain changes in
assemblages of spiders with increasing habitat complexity, including access to alternative
prey, more effective prey capture, architectural attachments for webs, and particularly,
refuge from intraguild predation (Langellotto and Denno 2004). Interestingly, habitat
164
explained the least variation of the five groups selected for species richness. This may be
because whereas habitat structure generally increases in a continuous manner with post-fire
age in this habitat, species richness may follow a more complex pattern (see Fig. 3a).
Simplifying this pattern by excluding the recently burnt sites and re-running our analysis
resulted in habitat explaining the most variation and slightly more than floristics (for
brevity results not shown).
Rainfall explained nearly as much as post-fire age for species richness, but little for
species composition. Previous work in arid Australia suggested that rainfall in the year
before sampling was correlated with the species richness of spiders, but that was not
statistically significant (Langlands et al., 2006). Increased plant growth and florescence
following rain may lead to increased invertebrates and therefore spiders. Rainfall is clearly
a strong driving force in arid Australia, and trying to understand how it influences
vegetation development following fire and the subsequent influence on fauna will be vital
for management (see Letnic and Dickman 2006).
Although changes in soil properties (e.g NH4+, NO3-) are known following fire (Wan et
al. 2001), which presumably affects the subsequent regeneration of floristics and vegetation
structure, we found few differences in nutrient values among our study sites. As such, it is
not surprising that soil was unimportant in explaining variation within the spider
assemblage. This result agrees with Sanderson et al. (1995), who found no relationship
with soil in northeast England. However, a study conducted at our location, which
contrasted assemblages of spiders between habitat types associated with differing
geologies, found a correlation between the composition of spider species and soil texture
and ammonium nitrogen (Owen 2004).
Predation and spiders
Several studies have demonstrated the strong influence predators, particularly reptiles, can
have on spiders (Spiller and Schoener 1988, 1998, Manicom et al. 2008). However, we
found the effect of predation alone explained none of the variation in the species richness
of spiders and very little for composition. Most of the variation explained by predation for
species composition was shared with post-fire age and habitat. We interpret this as reptiles
and scorpions potentially responding to post-fire changes in habitat structure in a similar
manner to the spiders, rather than exerting direct control over the spider assemblage.
165
Additionally, our collection methods may have been inadequate for assessing predation
pressure on spiders, or the influence of top-down control may be ephemeral in our system.
Thus, before top-down control in our study system is considered negligible, more detailed
measures of the predator and parasitoid assemblage through periods of boom and bust
should be undertaken. Future studies should also consider the implications of intraguild
predation (Polis et al. 1989, Wise 1993).
Study limitations
While we were able to explain most of the variation in species richness (79%), we were
unable to explain 68% of the variation in species composition. This level of unexplained
variation is common in partitioning analyses, which range from 20 to 80% of species
composition explained (Cottenie 2005). The unexplained variation may be due to
unmeasured variables or random noise (Legendre and Legendre 1998). For example, our
study was constrained by the absence of long-term rainfall records for our study sites. It is
clear that the long-term history of rainfall plays an important role in the post-fire
regeneration of vegetation. Other aspects of the fire regime (patch size, frequency and
intensity) may also account for unexplained variation. Additionally, Økland (1999) has
suggested that a large proportion of unexplained variation in such analyses (50-85%) may
be due to lack-of-fit of data to the model. This is why we presented the proportion of the
total variation explained.
Another limitation of our study is that because it is correlative it does not provide proof
of causality. Individual variables selected as the best predictors within explanatory groups
were correlated with other variables within and among groups. Different variables were
also selected for species richness and composition, although these were often strongly
correlated. Therefore, although step-wise selection chose particular variables, other
measured or unmeasured variables may be causing the relationships. That said, the
variables selected should be considered as good candidates around which to generate
hypotheses for future manipulative experiments.
166
Concluding remarks
To develop a mechanistic understanding of arid ecosystems and conserve biodiversity, we
must untangle the influence of multiple variables on assemblages of species. We found that
an assemblage of spiders in the arid zone of Western Australia had significant responses in
the number of species and its species composition to post-fire age. Post-fire variation in the
spider assemblage we studied is largely explained by vegetation (Floristics and Habitat
structure), which in turn is strongly influenced by Fire, with only a minor influence of
Predators at this scale. These findings suggest that land managers striving to conserve
spider diversity in arid Australia have the potential to influence a large part of the variation
within the assemblage.
Acknowledgements - We thank the many people who provided assistance in the field,
particularly T Griffiths, B and N Langlands and G Liddlelow. Experimental fires were
conducted with the help of staff from the Kalgoorlie office of the Western Australian
Department of Environment and Conservation (DEC). Thanks for identifications to R
Cranfield (plants) and M Cowan (vertebrates). Fauna were collected with ethics approval
(DEC AEC 2005/18). We are especially grateful to B Baehr, VW Framenau, BY Main, R
Ott, RJ Raven and JM Waldock for providing assistance with identifications of spiders.
Rainfall data were generously provided by the WA Bureau of Meterology. Thanks to P
Legendre and R Økland for answers to questions regarding variation partitioning. GIS data
and assistance were provided by G Behn and L Shu. Thanks to R Black, BY Main and VW
Framenau for helpful comments that improved the manuscript. Funding was provided by
DEC and the School of Animal Biology at the University of Western Australia.
167
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173
Table 1. a) The species richness of spiders (rarefied to 85 individuals) among post-fire ages
as tested by a permutational analysis of covariance (PERMANOVA), with the spatial
coordinate northing3 as the covariate. There was no significant interaction between the
covariate and post-fire age (p = 0.89), therefore this term was not included in the final
analysis. b) Pair-wise comparisons amongst fire ages with pseudo-t and p values
(significant in bold). See Fig. 3.
a
Permutations
Source
df
3
b
SS
MS
Pseudo-F
p
unique
Northing
1
257.31
257.31
34.93
0.0001
9847
Post-fire age
5
211.19
42.24
5.73
0.0032
9952
Residual
20
147.35
7.37
Total
26
615.85
Post-fire
age
0
0.5
3
5
8
t
p
0.5
1.53,
0.212
3
3.21,
0.035
3.12,
0.047
5
1.78,
0.138
1.10,
0.328
1.56,
0.156
8
0.05,
0.967
0.22,
0.782
2.78,
0.037
1.47,
0.174
20
2.54,
0.055
3.55,
0.029
5.18,
0.004
3.94,
0.005
174
1.61,
0.121
Table 2. The adjusted R2 and relative percentage of the total variation explained in species
richness of spiders by five groups of explanatory variables: Fire, Rainfall, Habitat,
Floristics and Spatial location of sites. The individual variables representing each group
and selected as having the highest explanatory power, are shown in brackets. No variables
from Soil or Predators explained significant (p < 0.01) variation. Results from a
simplification value of l < 0.05 (see methods).
Partitioned components
Variation explained
R2 adj
Relative %
0.08
10
Rainfall (January 07 , November 05 )
0.06
8
Habitat (bare ground2)
0.06
8
Floristics (principal coordinate 5 and 8)
0.14
18
Spatial (northing )
0.04
5
Fire, Rainfall, Floristics
0.12
15
Fire, Rainfall, Spatial
0.18
22
Fire, Rainfall, Habitat, Floristics, Spatial
0.11
14
Total
0.79
100
Fire (post-fire age dummy variables 3 and 5)
2
3
3
175
Table 3. a) The species composition of spiders among post-fire ages as tested by a
permutational analysis of covariance (PERMANOVA), with the spatial coordinate
northing3 as the covariate. The interaction between the covariate and post-fire age was not
significant, but the p value was not sufficiently large (p > 0.25) to justify removing the term
from the analysis (Sokal and Rohlf, 1995). b) Pair-wise comparisons amongst fire ages
with pseudo-t and p values (significant in bold). See Fig. 5.
a
Permutations
Source
df
3
b
SS
MS
Pseudo-F
p
Unique
Northing
1
3901.7
3901.7
3.43
0.0001
9929
Post-fire age
5
14109.0
2821.8
2.48
0.0001
9847
Northing3 x Time since fire
5
6891.1
1378.2
1.21
0.0934
9812
Residual
15
17040.0
1136.0
Total
26
41942.0
Post-fire
age
0
0.5
3
5
8
t
p
0.5
1.57,
0.028
3
1.89,
0.001
1.26,
0.110
5
1.78,
0.007
1.51,
0.048
1.20,
0.166
8
1.58,
0.023
1.35,
0.114
1.42,
0.016
1.14,
0.203
20
1.96,
0.003
1.35,
0.073
1.68,
0.009
1.62,
0.019
176
1.50,
0.024
Table 4. The adjusted R2 and relative percentage of the total variation explained in the
species composition of spiders by six groups of explanatory variables: Fire, Rainfall,
Habitat, Floristics, Spatial location of sites and Predators. The individual variables
representing each group and selected as having the highest explanatory power, are shown in
brackets. No variables from Soil explained significant (p < 0.01) variation. Results using a
simplification value of l < 0.05 (see methods).
Partitioned components
Variation explained
R2 adj
Relative %
Fire (post-fire age dummy variables 0, 0.5, 3, 20 and age of surrounds)
0.063
20
Rainfall (February-April 2006)
0.008
2
Habitat (live spinifex, dead spinifex)
0.019
6
Floristics (principle coordinate 2)
0.020
6
Spatial (northing )
0.016
5
Predators (reptile abundance, scorpion abundance)
0.009
3
Fire, Habitat
0.062
19
Fire, Habitat, Predators
0.034
11
Fire, Rainfall, Habitat, Floristics, Spatial
0.090
28
Total
0.32
100
3
177
2
Rainfall
Spatial
11
11
Predators
prey of
spiders
9
Floristics
3
Soil
7
6
4
(birds, lizards &
small mammals)
8
1
5
Habitat
structure
Fire
7
11
10
Spiders
12
parasitoids
(wasps + flies)
intraguild
predation
12
Fig. 1. Simplified conceptual diagram of some of the key variables that can influence
assemblages of spiders either directly (solid arrows) or indirectly (dashed arrows). A spatial
box bounds all variables to signify that spatial processes can influence each variable or
variables can generate spatial pattern. Arrow numbers indicate a selection of supporting
references, see text for further details. Note, for clarity, we do not show all possible
connections (e.g. the influence of rainfall on floristics or in mediating parasitoid
populations). We did not assess the factors associated with grey arrows and lower case font
in this study.
178
Fig. 2. The location of sites (*) within the proposed Lorna Glen (Matuwa) Conservation
Park (inset: park location in Western Australia). Site names denote fire age in years
followed by replicate number. Non-spinifex vegetation is shaded grey and lines mark
unsealed roads.
179
a
Species richness ±s.e.
40
30
spiders
20
plants
10
0
Proportion of ground cover ±s.e.
b
1.0
0
3
5
8
20
5
5
5
5
n=7 4 3
0.8
bare ground
0.6
0.4
0.2
live spinifex
0.0
0
3
5
8
20
Post-fire age (years)
Fig. 3. a) Mean species richness of spiders rarefied to 85 individuals and adjusted for the
covariate northing3 with species richness of plants. b) Changes in mean proportion of bare
ground and spinifex with post-fire age. Experimental fires indicated by arrow, with pre-fire
vegetation samples for the seven sites burnt experimentally to the left of arrow.
180
Variation explained (%)
100
80
Richness
R2adj =
Composition
Total variation explained
0.79
R2adj = 0.32
60
40
20
Fire
Rainfall
Habitat
Floristics
Predators
Spatial
Soil
Fire
Rainfall
Habitat
Floristics
Predators
Spatial
Soil
0
Groups of explanatory variables
Fig. 4. The percentage of the total variation explained in the species richness and
composition of spiders by each of seven groups of explanatory variables. Shared patterns
indicate components of variation explained by multiple groups (e.g. Fire, Rainfall or
Floristics data explain equally well the component of variation in species richness
represented by horizontal parallel lines). Solid black indicates variation unique to an
explanatory group. The sum of the total variation explained by all the groups equals more
than 100% due to shared components. For species richness, the variables selected within
each group were as follows: Fire (post-fire age dummy variables 3 and 5), Rainfall
(January 072, November 053), Habitat (bare ground2), Floristics (principal coordinate 5 and
8) and Spatial location of sites (northing3). For species composition, the variables selected
were as follows: Fire (post-fire age dummy variables 0, 0.5, 3, 20 and age of surrounds),
Rainfall (February-April 2006), Habitat (live spinifex, dead spinifex), Floristics (principle
coordinate 2), Spatial location of sites (northing3) and Predators (reptile abundance,
scorpion abundance). See Tables 2 and 4 for the values of each component. Soil variables
did not explain significant (p < 0.01) variation in either species richness or composition.
181
d b R D A 2 ( 1 8 .9 % o f f itte d , 1 2 % o f to ta l v a r ia tio n )
40
Live
spinifex
20
8-38-2
5-3
5-4
3-1
8-4
0
20-1
8-1
2-3
ns
S co rpio
8-5
5-1
5-5
20-2
20-5
20-4
Dead spinifex
20
5-2
Northing3
3-5
3-3
3
PCO 2
3-4
Age of
surrounds
0.5
0.5-2
3-2
Reptiles
-20
0.5-1
Feb 0 0.5-3
-A p 0-4
r 06
0-3
0-2
0-1
-40
-40
-20
0
20
40
dbRDA1 (25.1% of fitted, 15.9% of total variation)
Fig. 5. Ordination from a distance-based RDA of species composition of spiders with study
sites. Non bold numbers represent the post-fire age for each site. The environmental
variables selected for variation partitioning are shown as multiple partial correlation
vectors, with the length of the vector indicating the strength of the relationship between the
variable and each axis, while taking into account the other variables. Fire (post-fire age
dummy variables 0, 0.5, 3, 20, age of surrounds), Rainfall (February-April 2006), Habitat
(live spinifex, dead spinifex), Floristics (principal coordinate 2), Predators (reptile
abundance, scorpion abundance) and Spatial location of sites (northing3).
182
Appendix A
The post-fire age of study sites with location (latitude and longitude) and the date when last
burnt.
Post-fire
age
Location
Number
26°S
121°E
Date Burnt
0
1
21' 43''
25' 27''
27 April 2006
0
2
15' 51''
06' 12''
26 April 2006
0
3
16' 13''
06' 02''
28 April 2006
0
4
21' 26''
14' 14''
27 April 2006
0.5
1
21' 26''
24' 50''
11 October 2005
0.5
2
13' 58''
11' 48''
9 October 2005
0.5
3
21' 42''
25' 16''
14 October 2005
3
1
14' 12''
17' 00''
25 November 2002
3
2
09' 35''
16' 46''
25 November 2002
3
3
11' 58''
18' 10''
25 November 2002
3
4
12' 13''
19' 42''
25 November 2002
3
5
08' 45''
16' 05''
25 November 2002
5
1
16' 13''
02' 34''
8 January 2001
5
2
16' '52'
21' 42''
8 January 2001
5
3
17' 03''
11' 43''
8 January 2001
5
4
21' 24''
13' 29''
8 January 2001
5
5
11' 00''
02' 36''
15 November 2000
8
1
20' 15''
26' 58''
23 December 1997
8
2
15' 22''
07' 07''
1 February 1998
8
3
13' 33''
11' 36''
1 February 1998
8
4
16' 41''
21' 12''
1 February 1998
8
5
11' 57''
17' 47''
1 February 1998
20
1
16' 00''
06' 19''
before 1988
20
2
14' 01''
11' 35''
before 1988
20
3
21' 22''
25' 06''
before 1988
20
4
21' 39''
14' 11''
before 1988
20
5
11' 05''
02' 11''
before 1988
183
Appendix B
Excel file with calculations used to simplify results from variation partitioning, following
the method of Økland (2003). See enclosed CD.
184
Species Richness (rarefied 85 inds)
Env. Factors selected by Distlm, step-wise, in PERMANOVA, P<0.01, 9999 perms
Groups
F = fire age
X = Spatial
R = Rainfall
H = Habitat
V = Vegetation (floristics)
step
No. RDA
Variables
3, 5
y3
Jan07 2, Nov05 3
BG2
PCO5, PCO8
unique
partial
union VE intersection VE
0.01878
0.0015
-0.0058
-0.0015
0.06733
constraining
F
X
R
H
V
partial
XRHV
RHVF
HVFX
FXRV
FXRH
6
7
8
9
10
11
12
13
14
15
FX
FR
FH
FV
XR
XH
XV
RH
RV
HV
RHV
HVX
VXR
XRH
HVF
VFR
FRH
XFV
XFH
XFR
0.02801
0.05412
0.04903
0.07044
0.03238
0.00095
0.08148
-0.0113
0.10886
0.11867
0.00773
0.04114
0.03175
-0.01567
0.03668
0.00095
0.01265
-0.004
0.04733
0.05284
3
3
3
3
3
3
3
3
3
3
16
17
18
19
20
21
22
23
24
25
XFR
XFH
XFV
XRH
XRV
XHV
FRH
FHV
RHV
FRV
HV
RV
RH
FV
FH
FR
XV
XR
XF
XH
0.26186
0.06364
0.08795
0.02552
0.15123
0.14395
0.07109
0.18131
0.14412
0.24422
0.16183
0.00443
-0.00437
-0.00231
-0.00846
0.01018
-0.00928
0.02778
-0.01208
0.09111
4
4
4
4
4
26
27
28
29
30
XFRH
XRHV
XHVF
FRHV
XFRV
V
F
R
X
H
0.2897
0.18995
0.22454
0.39365
0.50043
0.0078
-0.00536
0.01016
0.06392
0.04865
5
31 XFRHV
0.78818
0.11247
1
1
1
1
1
1
2
3
4
5
2
2
2
2
2
2
2
2
2
2
L = <0.05
0.11
Distributed
3rd
5
31 XFRHV
0.11247
4
4
4
4
4
26
27
28
29
30
XFRH
XRHV
XHVF
FRHV
XFRV
V
F
R
X
H
0.0078
-0.00536
0.01016
0.06392
0.04865
3
3
3
3
3
3
3
3
3
3
16
17
18
19
20
21
22
23
24
25
XFR
XFH
XFV
XRH
XRV
XHV
FRH
FHV
RHV
FRV
HV
RV
RH
FV
FH
FR
XV
XR
XF
XH
0.16183
0.00443
-0.00437
-0.00231
-0.00846
0.01018
-0.00928
0.02778
-0.01208
0.09111
0.175943
0.00892
0.010333
-0.0017
0.002363
0.01138
0.00865
0.0463
0.00256
0.119253
2
2
2
2
2
2
2
2
2
2
6
7
8
9
10
11
12
13
14
15
FX
FR
FH
FV
XR
XH
XV
RH
RV
HV
RHV
HVX
VXR
XRH
HVF
VFR
FRH
XFV
XFH
XFR
0.00773
0.04114
0.03175
-0.01567
0.03668
0.00095
0.01265
-0.004
0.04733
0.05284
0.014148
0.044023
0.05304
0.003207
0.039874
0.004177
0.020675
-0.00083
0.048971
0.07292
1
1
1
1
1
1
2
3
4
5
F
X
R
H
V
XRHV
RHVF
HVFX
FXRV
FXRH
0.01878
0.0015
-0.0058
-0.0015
0.06733
2nd
After
=
1st
0.00195
-0.0013
0.00254
0.01598
0.01216
0.00195
-0.0013
0.00254
0.01598
0.01216
0.00195
0.00195
0.00254
0.00195
-0.0013
-0.0013
0.00195
0.00254
-0.0013
0.01598
0.01216
0.00254
0.01216
-0.0013
0.01216
0.00254
0.01598
0.01598
0.01598
0.01216
0.003
0.0034
-6E-04
0.0008
0.0038
0.0029
0.0154
0.0009
0.14
0.1759
0.22
0.1193
0.15
0.0760
0.0409
0.0617
0.0617
0.1402
0.096
0.052
0.078
0.078
0.178
0.003
0.0034
-6E-04
0.0008
0.0038
0.0029
0.0154
0.0009
0.003 0.0034
0.0029
0.0029 0.0154
0.0034 0.0154
0.003 -6E-04
-6E-04 0.0038
0.0034 0.0008
-6E-04 0.0029
0.0008 0.0009
0.0038 0.0154
0.0071
0.0071
0.0235
0.025
0.0016
0.1125
0.0235
0.0199
0.0199
0.0021
0.0103
0.0071
0.022
0.0265
0.0016
0.0199
0.0021
0.0103
-4E-04
0.0245
0.0365
0.003
0.0008
0.0038
0.0009
0.0009
0.025
0.0021
-4E-04
-4E-04
0.0245
0.0016
0.0103
0.0245
0.0365
0.0365
0.0071
0.0235
0.025
0.0016
0.0199
0.0021
0.0103
-4E-04
0.0245
0.0365
Appendix C
The Spearman correlation between selected variables (bold) and other variables.
Species Richness
Rho
Species composition
Jan 20072
Rainfall
Rainfall
Feb-Apr 2006
2
0.73
Feb-Jul 2006
1.00
Feb-Jul 20062
0.68
Apr 2006
0.83
0.67
3
0.79
3
Feb 2006
Feb-Jul 2006
Feb-Apr 2006
2
Feb-Apr 2006
Feb-Apr 2006
0.66
0.65
Feb-Jul 2006
Mar 2006
0.78
0.72
Feb 20063
0.64
Nov-Jan 20073
0.71
Feb-Jul 20063
0.64
Feb 20063
0.71
3
Feb-Apr 2006
Aug 2005-Apr 2006
0.64
0.63
3
Apr 2006
Feb 2006
0.70
0.69
Nov-Jan 20073
0.61
Feb 20062
0.69
0.61
2
Jan 2007
Jan 2007
0.65
0.63
Aug 2005-Apr 20063
0.63
Aug 2005-Apr 2006
3
Nov 20053
2
Nov 2005
Nov 2005
0.97
0.88
Habitat
live spinifex
Sept 2006
3
Sept 2006
2
0.71
Aug-Oct 2006
3
-0.66
upper storey woody shrub
0.69
Sept 2006
-0.63
2
-0.63
3
-0.62
3
-0.61
Jul 2006
Jan 2006
-0.72
live spinifex
live spinifex
upper storey woody shrub
dead spinifex
0.71
0.67
woody shrub3
-0.67
dead spinifex
3
0.63
dead spinifex
2
0.61
live spinifex
2
0.60
-0.71
dead spinifex2
0.92
3
0.92
3
-0.71
2
0.67
dead spinifex
-0.76
2
0.90
3
dead spinifex
bare ground
woody shrub
3
bare ground
2
Habitat
Spatial
Rho
bare ground
bare ground
Predators
Reptile abundance
Reptile species
Spatial
northing3
northing
0.93
185
0.61
northing3
northing
0.93
Appendix D
The ten plant species most correlated with the three floristics axes that were selected as
significant variables for variation partition of species richness or species composition of
spiders. Axes were generated using principle coordinate analysis (PCO) of floristic data.
PCO
Species
Species richness
PCO 5
-0.59
Acacia aneura
-0.55
Ptilotus sessilifolius
-0.45
Kennedia prorepens
0.42
Eucalyptus gongylocarpa
-0.41
Solanum centrale
0.39
Genus 1 sp.46
0.36
Glischrocaryon aureum
0.36
Euphorbia boophthona
0.36
Eucalyptus lucasii
-0.35
Codonocarpus cotinifolius
PCO 8
0.54
Halgania cyanea
0.50
Acacia burkittii
0.46
Ptilotus obovatus
0.41
Spartothamnella teucriiflora
0.38
Acacia grasbyi
-0.38
Goodenia triodiophila
0.38
Hakea rhombales
-0.35
Solanum sturtianum
-0.33
Glischroncaryon aureum
-0.33
Goodenia mueckeana
Species composition
PCO 2
-0.76
Solanum lasiophyllum
-0.62
Euphorbia boophthona
-0.58
Codonocarpus cotinifolius
-0.53
Dicrastylis brunnea
-0.53
Triodia basedowii
-0.53
Aristida contorta
-0.52
Abutilon otocarpum
-0.45
Eragrostis lanipes
0.45
Aluta maisonneuvei
-0.45
Eragrostis eriopoda
Family
Fabaceae
Amaranthaceae
Papilionaceae
Myrtaceae
Solanaceae
Poaceae
Haloragaceae
Euphorbiaceae
Myrtaceae
Gyrostemonaceae
Boraginaceae
Fabaceae
Amaranthaceae
Lamiaceae
Fabaceae
Goodeniaceae
Proteaceae
Solanaceae
Haloragaceae
Goodeniaceae
Solanaceae
Euphorbiaceae
Gyrostemonaceae
Lamiaceae
Poaceae
Poaceae
Malvaceae
Poaceae
Myrtaceae
Poaceae
186
CHAPTER 4
Predicting the post-fire responses of animal assemblages:
testing a trait-based approach using spiders
Peter R Langlands
Karl E C Brennan
Volker W Framenau
Barbara Y Main
Formatted for the Journal of Animal Ecology
187
Summary
1. Developing a predictive understanding of how species assemblages respond to fire is a
key conservation goal. In moving from solely describing patterns following fire to
predicting changes, plant ecologists have successfully elucidated generalisations based on
functional traits. Using species-traits might also allow better predictions for fauna but there
are few empirical tests of this approach.
2. We examined whether species traits changed with post-fire age for spiders in 27 sites,
representing a chronosequence of 0-20 years post-fire. We predicted a priori whether
spiders with ten traits associated with survival, dispersal, reproduction, resource-utilization
and microhabitat occupation would increase or decrease with post-fire age. We then tested
these predictions using a direct (fourth-corner on individual traits and composite traits) and
an indirect (emergent groups) approach, comparing the benefits of each and also examining
the degree to which traits were inter-correlated.
3. For the seven individual traits that were significant in the fourth-corner analysis, three
followed predictions (body size, abundance of burrow ambushers and burrowers was
greater in recently burnt sites); two were opposite (species with heavy sclerotisation of the
cephalothorax and longer time to maturity were in greater abundance in long unburnt and
recently burnt sites respectively); and two displayed response patterns more complex than
predicted (abdominal scutes displayed a U-shaped response and dispersal ability a hump
shaped curve). However, within a given trait, there were few significant differences among
post-fire ages.
4. Several traits were inter-correlated and scores based on composite traits used in a fourthcorner analysis found significant patterns, but slightly different to those using individual
traits. Changes in abundance with post-fire age were significant for three of the five
emergent groups. The fourth-corner analysis yielded more detailed results, but overall we
consider the two approaches complementary.
5. While we found significant differences in traits with post-fire age, our results suggest
that a trait-based approach may not increase predictive power, at least for the assemblages
of spiders we studied, as shown for plants. That said, there are many refinements to faunal
traits that could increase predictive power.
188
Introduction
Ecologists have long sought to understand and predict the consequences of disturbances
(flooding, grazing, habitat fragmentation, fire etc.) on ecosystems and assemblages of
plants and animals (Connell 1978; Lavorel et al. 1997). A formidable challenge is
elucidating how individual species of plants and animals might respond to a particular
disturbance, especially for highly diverse groups, where taxonomic knowledge is poor
and/or there is an absence of knowledge on the autecology of individual species. Therefore,
studying solely the responses of individual species is unlikely to lead to a rapid increase in
predictive power for unstudied species because it only generates location and taxa-specific
information (Weiher & Keddy 1995). However, an understanding of which traits determine
a species‟ response to disturbance may lead to generalizations, which can predict how other
species with the same traits will respond (Lavorel & Garnier 2002; McGill et al. 2006). We
define a trait following McGill et al. (2006) as “a well-defined, measurable property of
organisms, usually measured at the individual level and used comparatively across
species”. Ideally, we might hope to be able to collect an animal from any locality and from
only its morphological and behavioural traits predict the species‟ change in abundance
following disturbance.
A species-traits approach has yielded impressive advances in increasing predictive
power for plants (Shipley, Vile & Garnier 2006; Keith et al. 2007). A prominent example is
the marked distinction in post-fire responses between seeders versus resprouters (Noble &
Slayter 1980). However, correlations between traits cause most species to occur only within
a limited portion of the total multidimensional trait-space (Hubbell 2001). Therefore, to
develop a better mechanistic understanding of post-fire responses it is important to identify
groups of traits that are inter-correlated and might be functional (strongly influence
organismal performance).
The adoption of a trait-based approach for fauna and fire lags behind that for plants
(notable exceptions are Jonas & Joern 2007; Moretti et al. 2009; Moretti & Legg 2009).
Using previous approaches for fire, we adapt the vital attributes (Noble & Slatyer 1980)
and critical life cycles approaches (Whelan et al. 2002) to classify traits under five
categories: survival, dispersal, reproduction, resource-utilization and microhabitat
occupation. The interest of our search is convergent traits (Grime 2006; Pillar et al. 2009).
That is, due to environmental filters, the species within a community and the traits they
189
possess are more similar or under-dispersed (Weiher & Keddy 1995). We use current
theories and functional understandings (existing mechanisms) of traits to predict how each
trait might respond with increasing post-fire age. We then compare these qualitative
predictions to the observed results.
Several methods explore potential links between species-traits and environmental
conditions. These can either test the link indirectly (e.g. emergent groups), or directly (e.g.
fourth-corner or RLQ analysis). Emergent groups are suites of species selected for sharing
similar traits (Lavorel et al. 1997). The fourth-corner is an approach that combines
information on species traits and environmental characteristics via a matrix of species
abundances. While RLQ analysis is complementary to the fourth-corner, it focuses
primarily on ordination and interpretation, rather than testing the significance of
relationships (Dolédec et al. 1996; Legendre, Galzin & Harmelin-Vivien 1997). Most
applications use an indirect approach, partly due to the initial limitation of the fourth-corner
to presence-absence data only. However, the fourth-corner approach now incorporates
abundance data and may yield additional insights compared to emergent groups (Aubin et
al. 2009). That said, emergent groups easily incorporate links between traits, but for the
fourth-corner this remains an outstanding problem (Dray & Legendre 2008). Inclusion of
linked traits into fourth-corner analyses may increase the chance of type I error (Aubin et
al. 2009) and ignores biological reality. Ultimately, a direct approach that can incorporate
linked traits is required. In the interim, however, it is unclear whether researchers should
follow a direct or indirect approach, as only a single study has explicitly compared these
approaches for the same data (see Aubin et al. 2009).
Despite the usefulness of the approaches described above, some problems remain.
Neither the fourth-corner or emergent groups can yet incorporate potential spatial
autocorrelation of sites or phylogenetic signal between species (See Dray & Legendre
2008, p.3411). For faunas that are poorly known taxonomically and where autecological
information is scant, there will be a reliance on inferring behavioural traits at higher
taxonomic levels using information gleaned from related taxa. Thus, greater caution will be
required when considering behavioural traits compared to morphological traits measured
directly from each taxon. Even with these unresolved issues, however, the fourth-corner
and emergent groups approaches represent the best techniques currently available and offer
new insights into trait-environment relationships. As such, and because the search for a
190
responsive set of traits for fauna is still in its infancy, to assist future workers we have
included both morphological and behavioural traits.
Spiders are an interesting group for considering linkages between post-fire
environments and traits because they show marked changes in species composition with
fire (Buddle, Spence & Langor 2000; Brennan et al. 2006; Langlands, Brennan & Pearson
2006) and possess a diverse array of potentially influential traits. Spiders represent a range
of body sizes; our species differed by an order of magnitude (0.6-9.4 mm). While spiders
are unable to fly, many families possess the ability to drift passively (“ballooning”) by
using extensions of silk (Bell et al. 2005). Whilst spiders generally have soft abdomens,
some species also possess morphological adaptations that reduce desiccation, such as the
presence of hard plates (scutes) on the abdomen or heavy sclerotisation of the
cephalothorax (Main 1984). While almost all spiders are obligate carnivores, there is a vast
array of different hunting strategies, which have attracted interest as feeding guilds (Wise
1993; Uetz, Halaj & Cady 1999). Additionally, while many have a broad diet others show
increasing specialization. For example, some species are specialist predators of ants
(myrmecophagous) or other spiders (araneophagous) (Polis & Yamashita 1991).
In this paper, we examine if the species-traits of spiders can make better predictions of
post-fire responses using both the fourth-corner and emergent groups approaches. We
address four questions: 1) Are individual traits of spiders linked with post-fire age? In
short, we hypothesized that the abundance of spiders with the following traits would
decrease with increasing post-fire age: larger body size, heavy sclerotisation (cephalothorax
plus abdominal scutes), greater dispersal ability (ballooning) and using burrows. We
hypothesized the abundance of spiders with the traits of slow maturation, short seasonal
activity, diet specialization and a flattened body would increase with post-fire age. In our
methods, we describe how each of these traits might act to structure assemblages of spiders
following disturbance. 2) If significant relationships with traits are found, are these traits
inter-correlated? and if so, 3) Do combinations of these inter-correlated traits have
significant associations with post-fire age? Finally, 4) Are emergent groups of spiders
linked with post-fire age and what additional insights does the fourth-corner approach offer
over this method?
191
Materials and Methods
STUDY LOCATION AND DESIGN
The study site was the proposed Lorna Glen (Matuwa) Conservation Park in central
Western Australia (26°13'33" S, 121°33'28" E). Satellite images were used to select sites
representing six treatments of post-fire ages: zero (4 sites), six months (3 sites), three years
(5 sites), five (5 sites), eight (5 sites) and twenty plus (5 sites) years since the last fire. See
Appendix S1 and Langlands et al. (accepted) for further details of study location, sites and
fires.
SAMPLING AND IDENTIFICATION OF SPIDERS
Ground active spiders were sampled continuously over a nine-month period (30 April
2006-18 January 2007) using five pitfall traps (2 L jars with a mouth of 82 mm) per site.
Traps were exchanged every three months. Male spiders were identified to species level.
Due to taxonomic difficulties of correctly matching females and juveniles to males for
many of the undescribed taxa, the results presented here are only for males. All specimens
are deposited in the Western Australian Museum.
TRAITS
We scored morphological and behavioural traits where there was a potential mechanism to
explain post-fire responses. As noted in the introduction, owing to limited autecological
information, behavioural traits were inferred at the family or sub-family level. We included
only behavioural traits that we were confident had sufficient information available for such
inferences. As we measured morphological traits directly from the specimens, these data
are robust and independent of whether they have been named by taxonomists.
We classified these traits into five key categories: survival, dispersal, reproduction,
resource-utilization and microhabitat occupation. The placement of traits within these
categories is not mutually exclusive because burrowing could be placed under survival or
microhabitat, but we consider the categories a useful framework on which to build. Those
working with spiders in other areas or indeed other groups may find that some traits such as
flat bodies specialized to live under eucalypt bark are not relevant, but the categories may
192
help to find other relevant traits. A summary of each trait follows with a full list of species
and traits in the online supplementary material (Table 1, Appendix S2).
Survival
Body size (measured as carapace length): Having soft abdomens, spiders are vulnerable to
desiccation, particularly small spiders (Main 1984). As body size increases, the surface area
to volume ratio decreases. Therefore, the body size of arthropods was predicted to increase
with aridity (Remmert 1981), as shown for spiders in Europe (Entling et al. 2010). We
hypothesised that species with a larger body size and therefore a decreased surface area to
volume ratio, may be better able to cope with the greater variability in temperature and
humidity associated with recently burnt habitats. Indeed, the large body size of lycosids
might be an adaptation to withstand larger temperature variation in open habitats (Coyle
1981). As an estimate of body size for each species, we measured the mean carapace length
of five individuals. Abdomen length was not included as spider abdomens are soft and can
change greatly in size when preserved.
Burrowing: The intensity of heat from fires decreases rapidly with increasing soil depth
(Whelan 1995). Some species of spiders can construct burrows in the ground, creating a
microhabitat that shields them from direct disturbance by fire. Species exhibiting this
behaviour might have a greater chance of surviving the passage of fire relative to nonburrowing species and therefore occur in greater abundance in recently burnt areas.
Degree of sclerotisation: The development of thick plates or shields on soft body parts is
considered an adaptation which reduces water loss, particularly for small-bodied species
which, when compared with larger bodied species, have a higher surface area to volume
ratio (Main 1984). We scored two traits for sclerotisation. Heavy sclerotisation of the
cephalothorax (head-thorax) was scored as present (the cephalothorax was a rigid case,
often pitted and dark red) or absent. Secondly, we scored the presence of scutes (hard
plates) on either the dorsal or ventral side of the abdomen as absent, partial coverage or full
coverage.
193
Dispersal
Ballooning: The ability to disperse would be advantageous in colonising recently disturbed
habitats. Previous studies of spiders and some insect groups show that dispersal ability is
important for re-colonising disturbed sites (Crawford, Sugg & Edwards 1995; Moir et al.
2005). Many species of spiders can disperse over large distances by ballooning, releasing
silk threads as juveniles to catch wind currents while others can disperse only by walking
(Main 1984). Species were scored as ballooners if there was a published record of
ballooning for the genus or family (Bell et al. 2005). While species may possess the ability
to balloon, the distance can vary greatly along a continuum from only a few meters to many
kilometres (Bell et al. 2005). To simplify the analysis, we treated ballooning as a binary
response.
Reproduction
Time to maturity: Species can be divided into two broad life history categories, r- or Kselected (Southwood 1977). Although not without limitations, this can provide a useful
dichotomy of the life history of species (Polis & Yamashita 1991). One aspect of these
categories is time to maturity, short for r- selected and long for K- selected species. Species
with short maturity times would have an advantage in colonising and reproducing in
recently disturbed areas. The time taken to mature can vary widely between species of
spiders from one to several years (Main 1984). To differentiate between species we scored
maturation time as less than or greater than 3 years. We did not attempt a finer separation in
time to maturity ages due to the lack of natural history information.
Phenology: The reproductive activity of spiders can be highly seasonal with males sexually
mature and actively searching for females for limited periods (Merrett 1967; Framenau &
Elgar 2005). Fire may disadvantage those species with highly specific environmental
triggers for mating activity compared with species that can mate anytime throughout the
year. As a crude measure of phenology, species were scored according to the length of time
over which they were collected: three, six or nine months.
194
Resource-utilization
Hunting strategy: Spiders are almost all obligate predators, but the strategies they use to
catch prey differ substantially. Some are active hunters, others may sit-and-wait, while
many use different types of webs to capture prey (Turnbull 1973; Wise 1993). We used
taxonomic literature and expert opinion to allocate species to one of five hunting strategies:
active hunters, sit-and-wait hunters, burrow-dwelling sedentary hunters, terrestrial webs
and aerial webs.
Diet specialization: While as a group spiders are viewed as polyphagous predators, some
have specialised feeding habits (Marc & Canard 1997). For example, zodariids are
specialist ant predators (Jocqué 1991). Species with restricted diets may be limited to
habitats that support suitable supply of the required food. Hence, diet specialization may
increase with time since disturbance. We scored species that are known ant specialists as a
binary trait. We did not score species that mimic ants as potential predators of ants, because
mimicry can also evolve to evade predators (see Cushing 1997).
Microhabitat
Flattened body: Several groups of Australian spiders exhibit an extremely flattened body
shape, which might have evolved with the rapid speciation of Eucalyptus trees and the
crevice habitat provided under the peeling bark (Żabka 1991). In instances where the bark
is thick and fire intensity is low, by sheltering under bark some spiders might survive the
passage of fire (Brennan, Moir & Wittkuhn in press). However, for species of eucalypt with
thin bark (or for trees with thicker bark but where fire intensity is high), most of the bark
may be consumed by the fire or slough off in ensuing months. Thus, there may be limited
microhabitat for crevice-dwelling spiders for several years. At our study site, fire resulted
in a loss of bark crevices and so a flattened body might not confer a survival advantage
during burning and the lack of suitable crevices post-fire may inhibit recolonization.
STATISTICAL ANALYSIS
To test the link between environmental conditions and individual spider traits directly, we
used the fourth-corner analysis (Legendre, Galzin & Harmelin-Vivien 1997; Dray &
195
Legendre 2008). This analysis uses three data matrices (Matrix R: environment by sites,
Matrix L: species by sites, Matrix Q: species by traits) to test directly the link between
environmental characteristics and species-traits via the observed abundance of species
(Appendix S3). We used the two-stage permutation test recommended by Dray & Legendre
(2008), which combines the results from permutation models 2 and 4 (see Dray &
Legendre 2008: Figures 2 & 3). Previous work indicated that the post-fire age of sites in
years was a good predictor of the spider community (Langlands et al. accepted); we
therefore chose this variable to represent the matrix R (environmental characteristics).
Matrix R was coded as dummy variables following Aubin et al. (2009), which allows for
non-linear patterns with increasing post-fire age. Matrix L was represented by a matrix of
abundances of spiders that were fourth root transformed to reduce the dominance of
abundant species. A matrix of the ten traits scored for each species represented Matrix Q,
all traits were coded as qualitative variables except for body size, which was quantitative.
Analyses were conducted using the „fourthcorner‟ function with 9999 permutations in the R
package ade4 (Dray & Dufour 2007).
To examine which traits were linked, we calculated a similarity matrix between all
species based on the ten traits. We used the Gower coefficient because it can incorporate
both quantitative and qualitative variables. A principal coordinate analysis (PCoA) was
then employed on the resulting matrix to simplify the inter-correlated traits to a reduced
number of axes. We chose this method as it allows any similarity measure. To relate the
resulting axes back to the original traits we used vector overlays of the correlation between
axes and traits.
To test the link between environment and combined traits directly, and address the
inability of the fourth-corner to incorporate linked traits, we devised the following
approach. We incorporated the axis scores for each species from the PCoA into a fourthcorner analysis as matrix Q (Appendix S3). We recognise that this method, although
theoretically sound, is somewhat crude as it contains multiple steps. We again used the
two-stage permutational test (models 2 & 4).
To test the link between environmental conditions and traits indirectly we used
emergent group analyses based on the similarity matrix constructed from the ten traits
(Appendix S3). This method is indirect as it requires two steps (Dray and Legendre 2008).
Traits and species abundances (matrices Q & L) are first linked, and then related to
196
environmental conditions (Matrix R). Ward‟s method was used to cluster species and the
resulting dendrogram was arbitrarily split into five emergent groups. The abundance of
species within each emergent group was then summed for each site. Permutational analysis
of variance (PERMANOVA) was then used to test for significant differences in the
abundances of groups between post-fire ages. PERMANOVA is highly robust as it uses
permutation for significance testing and any dissimilarity measure may be used (Legendre
and Anderson 1999). We used Euclidean distance with unrestricted permutation of the raw
data, type III sums of squares and 9999 permutations. As argued by Moran (2003), we have
not corrected for multiple analyses. While none of the above methods can currently
incorporate spatial autocorrelation, we have shown elsewhere that spatial location
explained less than 4% of the variation in species richness or composition of our spider
assemblages (Langlands 2010). Analyses were performed using PERMANOVA+
(Anderson, Gorley & Clarke 2008, version 1.01) and R (R Development Core Team 2009).
Results
Our dataset comprised 4234 male specimens representing 179 species of spider from 24
families, of which only 32 species (=17.9%) had scientific names. Previous analyses
indicated significant differences in the species composition of spiders with increasing postfire age (Langlands et al. accepted, Appendix S4). Matching these differences in species
composition, were shifts in the abundance of species with particular traits among post-fire
ages. The fourth-corner analysis showed significant links between post-fire age and spiders
for seven of the ten traits measured (Table 1). There were significant results within all of
the groups of traits except microhabitat occupation. There were more large-bodied
individuals at recently burnt sites (0-year-old) (Fig. 1a). Abundance of species with heavy
sclerotisation of the cephalothorax increased in 8-year-old sites and was significantly
higher in 20-year-old sites (Fig. 1b). Abdominal scutes displayed a U-shaped pattern with
significantly fewer scutes in 5-year-old sites and high abundances in recently burnt and
long unburnt sites (Figs. 1c). The abundance of spiders that can disperse via ballooning was
lowest in 0 aged sites and highest in 5-year-old sites (Fig. 1d). There were significantly
more long-lived individuals in 0-year-old sites, compared to all other ages (Fig. 1e).
Likewise, both burrow-dwelling sedentary hunters and burrowing spiders were in
significantly greater abundance in 0 aged sites compared to all other ages (Figs. 1f, g).
197
However, within a particular trait there was usually only one post-fire age that differed
significantly from all others.
The first three axes of the principle coordinate analysis (PCoA) explained 91.7% of the
variation between species based on the ten traits. High values along axis 1 were associated
with the presence of partial abdominal scutes, an active hunting strategy and to a lesser
extent, a more specialized diet (ants), and not using burrows (Fig. 2, Appendix S5). High
values along axis 2 were strongly associated with high dispersal ability (ballooning) and to
a lesser extent hunting from terrestrial webs. Axis 3 was associated with phenology.
Plotting of unique vectors for each trait onto the PCoA ordination showed that ballooning
and hunting using a terrestrial web were strongly inter-correlated (Fig. 2). Similarly
strongly inter-correlated were heavy sclerotisation of the cephalothorax, diet specialization
on ants, the presence of full abdominal scutes and active hunting. Correlated to a lesser
extent were body length, time to maturity, and burrowing Ordination also showed a clear
influence of phylogeny as many species within a family clustered together in trait space.
For example, five of the six species of Nemesiidae clustered very tightly in the lower left
corner of the ordination (Fig. 2). Other families such as the Zodariidae clustered together
more loosely in trait space.
Using the PCoA axes in a fourth-corner analysis found PCoA axes 1 and 2 to be highly
significant with the 0-year-old sites (Table 2). The negative correlation of 0-year-old sites
with axis 1 indicated that recently burnt sites had a greater abundance of species without
abdominal scutes and a lesser abundance of species with partial abdominal scutes or an
active hunting strategy. It also indicated to a lesser extent that 0-year-old sites had greater
abundance of species using burrows and a lesser abundance of species with a specialized
diet (ants) (Appendix S5). For axis 2 there was a positive correlation; hence the 0-year-old
sites had fewer individuals that disperse via ballooning.
For the indirect analysis, five emergent groups of species chosen from the cluster
analysis contained 12 to 65 species each. Several families had species within multiple
groups (Table 3, Appendix S6). Subsequently, permutational analysis of variance
(PERMANOVA) found abundances of only three of the groups displayed significant
responses to post-fire age (Groups III, IV & V, Fig. 3). Group III consisted of small to
large, active hunters, which were mostly myrmecophageous and non-ballooning, with a
complex pattern in abundances with post-fire age (d.f. 5, 21; pseudo-F = 2.89; p = 0.04).
198
Group IV were small, active hunters with full scutes, predominately Oonopidae, and were
more abundant in recently burnt and long unburnt sites (d.f. 5, 21; pseudo-F = 5.17; p =
0.004). Group V consisted mainly of mygalomorphs and lycosids, which were more
abundant in 0-year-old sites (d.f. 5, 21; pseudo-F = 6.93; p = 0.002, Fig. 3).
Discussion
We found significant patterns in the species-traits of spiders with post-fire age, namely
recently burnt sites (0-years-old) had more individuals with a large body, limited dispersal
ability (i.e. presumed unable to balloon), burrowing habit and an ambushing hunting
strategy from burrows. Although a majority (7 of 10) of our traits differed among post-fire
ages, within traits there were few significant differences between post-fire ages. In four
instances out of seven, only the recently burned sites differed from all other ages (Fig. 1).
Furthermore, the patterns of difference did not consistently match our predictions. Of the
seven spider traits that were significantly different among post-fire ages, three followed
predictions (body size, hunting strategy and burrowing behaviour), two were opposite
(heavy sclerotisation of cephalothorax & time to maturity) and two displayed more
complicated response patterns than predicted (abdominal scutes & ballooning). Given the
limited research effort into the trait-based approach for fauna and fire, it is not surprising
that our results are not as clear as found recently for plants (e.g. Keith et al. 2007; Aubin et
al. 2009).
ARE INDIVIDUAL TRAITS LINKED WITH POST-FIRE AGE?
Survival
All four traits within the survival category had significant links with post-fire age; however,
as noted above, only two of these followed predictions. Body size was expected to
influence survival via differences in desiccation rate, with larger bodied spiders having an
advantage in recently burnt and open habitats. In Europe, the body size of female
Linyphiidae increased with increasing disturbance from flooding; however, Lycosidae were
larger in less disturbed sites (Lambeets et al. 2008). However, body size often correlates
with other traits (Peters 1983; Gaston & Blackburn 2000), and in our study it was
correlated with burrowing. It is therefore unclear whether body size or burrowing is
functional.
199
The response of spiders with sclerotisation of the cephalothorax was opposite to the
prediction of greater sclerotisation immediately post-fire. Thus, the mechanism for heavy
sclerotisation of the cephalothorax and abdomen also requires attention. It is unclear why
there would be more spiders with this trait in long unburnt sites. The response of abdominal
scutes was similar with high abundance in long unburnt sites, but there was also relatively
high abundance in recently burnt sites. Most of the species with full scutes were from the
Oonopidae, which are leaf-litter dwellers. At our study sites the proportion of ground
covered by leaf-litter followed a U-shaped pattern and remained high in the recently burnt
sites as scorched trees shed leaves and bark (Langlands unpublished data). Oonopid spiders
selecting post-fire ages with more leaf-litter may explain why spiders with full scutes were
more common in recently burnt and long unburnt sites. If so, the reduction in desiccation
that spiders receive from possessing full scutes may not act directly to influence changes in
the composition of species of spiders with post-fire age.
Dispersal
Contrary to our predictions, and to previous studies of primary and secondary successions,
we found spiders that had greater dispersal ability via ballooning most abundant in 5-yearold sites, rather than those burnt recently. Although clearly different to disturbance by fire,
ballooners dominated early colonists during primary succession following glaciations and
volcanic eruptions (Crawford, Sugg & Edwards 1995; Hodkinson, Webb & Coulson 2002),
and for two spider families in areas frequently disturbed by flooding (Lambeets et al.
2008). Perhaps this inconsistency relates to two things. Firstly, although we were able to
discriminate between ballooning and non-ballooning species, we were unable to consider
differences in ballooning or walking ability. Secondly, patch size might play an important
role in determining the influence of traits associated with dispersal ability. Logistical
constraints meant that our recently burnt sites were only 300 by 300 m, so dispersal by
walking may have been sufficient for colonization. It may be beneficial to incorporate the
walking abilities of non-ballooning species.
Reproduction
Time to reach maturity was also opposite to our predictions with a very high abundance of
long-lived species in recently burnt sites. This might be because males from long-lived
burrowing species (Nemesiidae) survived the fire in situ and then left to find mates and fell
into our pitfall traps. This possibly indicates a degree of inertia immediately following
200
burning (see Langlands et al. accepted). Another explanation that cannot be excluded is that
large wandering spiders are more likely to be caught by pitfall traps in burnt areas with
little ground cover (Topping and Sunderland 1992). This may partially explain the
significant results found for body size and burrowing in the 0-year-old sites. However,
inspection of the raw data indicated clearly that long-lived species did not solely drive the
significant 0-year-old result. Two large lycosid species, one of which burrows [Hoggicosa
bicolor (Hogg, 1905)] were abundant in the 0-year-old sites. The phenology of species was
not significantly different among post-fire ages, although our measure of seasonal activity
was rather crude, and data with finer temporal resolution may yet again provide better
insights.
Resource-utilization
Although abundance of burrowing ambushers was significantly higher in recently burnt
sites, a lack of significant differences between other post-fire ages suggests hunting
strategy does not differ markedly with time since fire. However, many studies show that
web-hunting spiders require specific habitat architecture and respond to changes in
vegetation accordingly (Riechert & Gillespie 1986; Uetz 1991). Therefore, our results for
web building spiders may be due in part to our sampling method. Due to the remote
location and low catch rates from hand collecting and vacuuming in this habitat we were
restricted to using pitfall traps (Owen 2004). Pitfall traps sample many of the foliage and
web building species (Brennan, Moir & Majer 2004). However, these taxa will probably be
underrepresented in our data set and thus constrain our ability to detect post-fire changes in
abundance of species utilizing an aerial web for hunting. For our study, it seems that
specialised food sources are not limiting with no detectable result for diet specialization on
ants. This result is contrary to predictions that niche breadth decreases with increasing time
since disturbance (Odum 1969; Brown & Southwood 1983).
ARE TRAITS INTER-CORRELATED?
Several traits were inter-correlated from different categories of traits (e.g. survival,
dispersal, reproduction etc.). Uncovering the functional significance of each trait is critical
to developing a better mechanistic understanding of post-fire response patterns.
Methodological issues also demand the consideration of links between traits. Aubin et al.
(2009) suggest including highly correlated or linked traits in the fourth-corner analysis
201
could increase the level of Type-I errors. Their proposed solution is to test for correlated
traits and exclude redundant traits. Our maximum correlation was only 0.69 (burrowing and
time to maturity) which we considered moderately high. Our preferred solution however,
was to use PCoA to incorporate axes representing combinations of traits into a fourthcorner analysis.
ARE COMBINATIONS OF TRAITS LINKED WITH POST-FIRE AGE?
Fourth-corner analysis showed the composite scores of traits from the PCoA had some
significant links with the 0-year-old sites. This more biologically realistic approach
detected some of the pattern from the analysis on individual traits; there was lower
abundance of heavy sclerotisation of the cephalothorax and higher abundance of burrowers
and burrow hunters in 0-year-old sites. However, it did not detect significant links between
other post-fire ages and suggested some different patterns for traits. A strong loading of
abdominal scutes for axis 1 suggested this trait is significantly less abundant in the 0-yearold sites, compared with 5-year-old sites as identified by the analysis on individual traits. It
also suggests diet specialisation on ants is less abundant in 0-year-old sites, a finding not
found analysing traits separately. A major problem with this approach however is that a
large number of traits correlated with axis 1 made it difficult to interpret the significant
result. Interpretation of the second axis is easy, with only ballooning strongly correlated;
however, this approach did not detect greater abundance of ballooners in 5-year-old sites.
ARE EMERGENT GROUPS LINKED WITH POST-FIRE AGE?
The indirect method of using emergent groups found links between post-fire age and the
post-fire response of spiders. Of the five groups defined, three had significant changes in
abundance. However, the post-hoc tests found these changes with post-fire age were not
linear or simple. The responses of Group IV appear strongly related to abdominal scutes,
while group V are related to body size, burrowing and time to maturity. Therefore, the
results from the emergent group approach, particularly for these traits, were largely
congruous with those of the fourth-corner. However, the significance of traits such as
dispersal ability and heavy sclerotisation of the cephalothorax were less clear compared to
the fourth-corner approach with individual traits.
202
A key advantage of emergent groups is that it generates response groups ultimately leading
to the creation of functional types (e.g. plant functional types). We strived to select a
limited number of groups that were biologically meaningful. However, there is a trade-off
inherent with the size and number of emergent groups selected. While selecting more
groups of smaller size may increase predictive accuracy and generate more statistically
significant responses, this ultimately reduces practicality and the ability to generalize
(Noble & Gitay 1997; Keith et al. 2007). Indeed, we note that the three response groups
that had significant responses had the fewest species.
CURRENT CONSTRAINTS AND FUTURE DIRECTIONS
Our natural history knowledge and taxonomic understanding of Australian spiders is still
poor for many families (Brennan, Moir & Majer 2004). This means that while we can have
strong confidence in morphological traits measured directly from specimens, the quality of
data available for behavioural traits may continue to hinder a trait-based approach. Indeed,
we have spent much of the discussion of this paper wondering if a finer resolution of detail
for behavioural traits would have distinguished more of the post-fire ages. This is
somewhat disappointing. It is for faunas where autecological knowledge at species level is
poor that the trait-based approach might offer the greatest benefit to develop rapidly a
predictive understanding of faunal responses to disturbance. Two other potentially
contributing factors also deserve mention. Firstly, Moretti et al. (2009) have questioned
whether the response of traits to fire can be generalized between regions where fire history
differs at evolutionary time scales. They suggest that for areas with a long history of fire,
community level changes in traits may exhibit greater inertia/resilience. Thus, the long
history of fire in arid Australia may have contributed to the limited functional responses we
observed. Secondly, while searching for convergent traits, the suite of traits we measured
may contain divergent traits (limiting similarity). These function to allow species to coexist
under competition, rather than under similar environmental conditions (Weiher & Keddy
1995).
As noted in our introduction, our interest was the ability of morphological and
behavioural traits to predict changes in the abundance of species following disturbance.
Therefore, we focused on traits at the individual level, and chose not to include community
level traits such as rarity (e.g. geographic range, habitat specificity). These traits can be
203
powerful for well-known faunas (e.g., Bonte, Lens & Maelfait 2006; Lambeets et al. 2008),
but will often be unavailable for poorly known faunas.
Finally, we echo previous calls for statistical advances. The most important of these are the
ability to incorporate phylogeny and spatial autocorrelation of sites into the fourth-corner
approach (Dray & Legendre 2008, Aubin et al. 2009).
Conclusions
We set out to test, using spiders, if the species-traits of fauna might increase the predictive
power of post-fire responses. Ideally, we might hope to be able to collect a spider from a
location and predict its change in abundance following fire from only morphological traits
measured from specimens and inferred behavioural traits. We found significant
relationships between species-traits of spiders associated with survival, dispersal,
reproduction and resource-utilization and post-fire age. Both a direct and an indirect
method of assessing links between traits and the environment showed significant links and
we consider the combination of the two approaches complementary. Overall, while our
analysis suggests caution over the predictive power of a trait-based approach of faunal
responses post-fire, it is still too early to assess its full potential. We look forward to further
studies using novel data sets, refined traits and experimental studies that test underlying
mechanisms.
204
Acknowledgements
We thank R. Raven, B. Baehr and J. Waldock for useful insights into the biology of
Australian spiders. Thanks to R. Black, D. Reed, two anonymous reviewers and the
associate editor for useful comments that improved the manuscript. Fauna were collected
under licenses and with ethics approval (WA Dept. of Environment and Conservation, AEC
2005/18). The WA Department of Environment and Conservation and the University of
Western Australia provided funding.
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Table 1. Test of the direct link between the species-traits of spiders and increasing post-fire
age from a combined fourth-corner analysis (permutation models 2 & 4) using 9999
permutations. For each trait are, the states scored, the test statistic, and the value of the test
statistic for each post-fire age with significance indicated (* denotes p <0.05, ** denotes p
< 0.01).
Traits
Scored states
Test
Post-fire age (years)
statistic
0
0.5
3
5
8
20
Chi
15.9**
0.7
3.0
0.0
0.4
3.2
pseudo-F
21.6**
0.0
4.5
0.1
0.1
2.4
Survival
Burrowing
yes/ no
Body size (length)
mean carapace
length (mm)
Heavy sclerotisation
of the cephalothorax
normal/
sclerotised
Chi
2.0
0.1
2.4
1.4
1.9
7.0*
Abdominal scutes
none/ some/
whole surface
Chi
4.0
1.0
3.7
8.6*
0.5
7.7
yes/ no
Chi
7.3*
1.2
3.1
5.3*
2.3
0.5
< 3 years/
> 3 years
3/ 6 / 9 months
Chi
6.6*
0.0
3.0
0.4
0.1
1.7
Chi
1.3
3.5
5.1
0.4
0.7
1.6
Hunting strategy
active/ burrow/ sit &
wait/ aerial webs/
terrestrial webs
Chi
16.1**
1.6
5.1
0.0
1.2
3.4
Diet specialization
(ants)
yes/ no
Chi
0.2
1.3
0.0
0.3
1.3
0.1
yes/ no
Chi
0.4
0.1
0.5
0.0
0.0
0.5
Dispersal
Ballooning
Reproduction
Time to maturity
Phenology
Resource-utilization
Microhabitat
Flattened body
211
Table 2. Test of the direct link between combinations of traits and post-fire age. Principal
coordinate analysis (PCoA) was used to reduce the ten species-traits of spiders (with
varying degrees of inter-correlation) to three axes, which were then used as matrix Q in a
fourth-corner analysis. Values represent a pseudo-F statistic. For details of axis correlation
with traits, see Fig. 2 and Appendix S4. ** denotes p < 0.01.
PCoA
axes
Post-fire age (years)
0
1
2
3
0.5
11.28** 0.14
9.48** 1.66
0.02
0.15
Variation
(%)
3
5
8
20
4.70
4.75
0.65
0.44
4.14
0.22
0.17
2.19
0.08
2.82
0.43
0.15
Cumulative
variation (%)
37.5
32.3
21.9
37.5
69.8
91.7
Table 3: The five groups of species selected from cluster analysis with the number of
species, shared traits and taxa for each group. Note, species from some families are within
multiple groups. For each family, superscripts denote the fidelity of species within a group,
A
: all species in a family, S: Some species, F: Few species.
Cluster
Number
groups
I
of species
65
Small to large, with no scutes,
active, sit-&-wait hunters and
terrestrial webs
II
48
III
27
IV
27
V
12
Shared traits
Taxa
A
A
A
Clubionidae , Desidae , Dictynidae ,
S
A
F
Gnaphosidae , Linyphiidae , Lycosidae ,
A
A
A
Miturgidae , Oxyopidae , Philodromidae ,
F
F
A
Prodidomidae , Salticidae , Sparassidae ,
A
A
Thomisidae , Zoridae
F
S
A
Small to Medium, some with
flattened bodies, ballooning,
mostly active hunters with
some terrestrial webs
Small to large, ant eaters,
active hunters and mostly
non-ballooning
Small, with full scutes and
active hunters
Corinnidae , Gnaphosidae , Pholcidae ,
S
S
Salticidae , Theridiidae
Large, without sclerotisation,
mostly slow maturing and
burrowing behaviour
Nemesiidae , Segestriidae , Lycosidae
212
F
S
F
Corinnidae , Lamponidae , Prodidomidae ,
A
Zodariidae
F
F
F
Corinnidae , Gnaphosidae , Lamponidae ,
A
A
F
Liocranidae , Oonopidae , Salticidae ,
F
Theridiidae
A
A
S
b
Body size
Mean abundance of species
with sclerotised cephalothorax
Mean length (mm)
3.5
*
3.0
2.5
2.0
1.5
0
5
c
10
15
20
d
Abdominal scutes
Mean abundance of
species with a full scute
15
10
*
5
0
0
10
15
20
Time to maturity
4
1
*
3
2
1
0
0
5
10
15
20
*
2.0
1.5
1.0
*
0.5
0.0
0
5
10
15
20
Hunting Strategy- Burrowing
8
*
2
4
Ballooning
f
3
Heavy sclerotisation
of cephalothorax
2.5
Mean abundance
of burrow hunters
Mean abundance
of long lived species
e
5
Ratio: ballooning/ non-ballooning
a
*
6
4
2
0
0
0
5
10
15
0
20
5
10
15
20
Post-fire age (years)
Ratio:Burrowing/
non-burrowing species
g
Burrowing
0.15
*
0.10
0.05
0.00
0
5
10
15
20
Post-fire age (years)
Fig. 1. Mean abundance (4th root) or ratio, ± SE, with post-fire age (years). Asterisk
denotes significant ages based on fourth-corner analysis not graphs (Table 1).
213
Family
Gnaphosidae
Lamponidae
Lycosidae
Nemesiidae
Oonopidae
Zodariidae
Other
0.4
Ballo
Ph
en
-9
cu
A bS
l
artia
te-P
it
ent
AbScute-Abs
Ab
Sc
g
wi n
rro rrow
u
B Bu
ntHu
to
m
at
Le
ng urity
t
Phe
h
n-3
mth
s
ute
-F
Hu
ull
ntAc
Ce
tive
p
Di ha
lot
et
sp h o
ra
ec
x
ia
li z
at
ion
(a
Bo
-0.2
dy
e
Ti
m
PCoA 2 (32.3% of total variation)
d b o dy
0
it&wa
Flattene
eb
errW
nt-T
Hu
s
th
m
-6
en
Ph
HuntS
m
ths
g
oni n
0.2
nt
s)
-0.4
-0.4
-0.2
0
0.2
PCoA 1 (37.5% of total variation)
0.4
Fig. 2. Principal coordinate analysis of the similarity based on ten traits between 179
species of spiders (Table 1). Vectors represent the Spearman correlation of traits, with the
length and direction indicating the relationship with PCoA axes. Abbreviations: Phen=
Phenology, AbScute= Abdominal Scutes, Hunt= Hunting strategy, Cephalothorax= Heavy
sclerotisation of cephalothorax. Six dominant families display unique symbols with the
remaining species pooled into one symbol for clarity. The third PCoA axis explained
21.9% of the total variation (91.7% for all three axes) and correlates strongly with
Phenology (Appendix S4).
214
Group III
Mean abundance
15
c
abc
10
ac abc
ab
b
5
0
0
5
10
15
20
Group IV
15
Mean abundance
c
a
10
a
abc
ab
b
5
0
0
5
15
20
Group V
8
Mean abundance
10
a
6
ab
4
bc
2
bc
bc
c
0
0
5
10
15
20
Post-fire age (years)
Fig. 3. Mean abundance (4th root) ± SE for emergent groups which had a significant
response with post-fire age (years). For the traits and species of each group see Table 3.
Unlike letters indicate significant differences in pair-wise tests.
215
Appendix S1
Study area
The study was conducted in central Western Australia at the proposed Lorna Glen
(Matuwa) Conservation Park, located approximately 150 km NE of Wiluna. The former
sheep and cattle station receives a median annual rainfall of 235 mm (range 86–654 mm)
and experiences mean monthly temperatures from 21–38 ˚C in summer and 5–21 ˚C in
winter (Australian Bureau of Meteorology).
Lorna Glen contains a range of habitat types with the most widespread of these being
the fire-prone hummock grasslands (Bullimore). This is a vegetation assemblage dominated
by spinifex Triodia basedowii E. Pritz, 1918, an over storey of marble gums (Eucalyptus
gongylocarpa Blakely, 1936) with scattered mulga (Acacia aneura Benth, 1855) and
mallee (E. kingsmillii Maiden and Blakely, 1929 and E. lucasii Blakely, 1934). Spinifex is
highly flammable, but fires are unlikely to spread within ages under 10-15 years unless
preceded by periods of high rainfall, which increase biomass and promote the growth of
short-lived soft grasses (Allan and Southgate 2002).
Sites and fires
Our study was conducted at the landscape scale with 27 sites selected to represent the
majority of fire ages present at Lorna Glen. Prior to 2001 Lorna Glen had a recent history
of fire suppression by pastoralists; however, infrequent and large scale (>100 km2) fires
still occurred. We used Landsat satellite images from 1985 to 2005 to establish the recent
fire history of the study area. From these natural fire histories and some experimental fires,
we selected six treatments for post-fire ages: 0, 0.5, 3, 5, 8 and 20+ years since the last fire.
The patch size in which each site was located was at least nine hectares (90 000 m2) and
there were three to five sites per post-fire age. At each site, a 50 x 50 m (0.25 ha) quadrat
216
was established a minimum of 150 m from the site boundary (change in fire age) or road.
We installed five pitfall traps in each quadrat, one at each corner and one in the centre.
Many fire ecology studies conducted at the landscape scale have difficulties finding
multiple fires of the same age within a study area that can act as true replicates (Brennan et
al. 2009). Our study design was similarly constrained by the pyrodiversity present at Lorna
Glen with very few sites burnt recently (< 1 year-old). For some post-fire ages (3, 5 and 8
years) multiple sites were located within a single fire scar. However, in these instances,
sites were interspersed with other ages and located as far apart as possible (the minimum
distance between two sites within the same fire scar was 1.9 km and was more often in the
order of 5–10 km). To resolve the problem of a lack of very recent burns we burnt seven
patches of habitat not burnt for at least twenty years. We burnt three patches in October
2005 and four patches in April 2006 to examine two additional post-fire ages, 0 and 0.5
respectively. Each patch had a single sampling site (quadrat).
References
Brennan, K. E. C., Christie, F. J. & York, A. (2009) Global climate change and litter
decomposition: more frequent fire slows decomposition and increases the functional
importance of invertebrates. Global Change Biology, 15, 2958-2971.
217
Species
Cheiracanthium sp.05
Clubiona sp.01
Clubiona sp.02
Clubiona sp.03
Clubiona sp.04
Battalus sp.04
Genus 1 sp.01
Poecilipta sp.02
Poecilipta sp.03
Supunna funerea Simon, 1896
Supunna picta (L. Koch, 1873)
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Phryganoporus sp.01
Genus 1 sp.01
Genus 1 sp.02
Ceryerda cursitans Simon, 1909
Eilica sp.07
Eilica sp.11
Encoptarthria sp.01
Encoptarthria sp.08
Encoptarthria sp.15
Family
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Desidae
Desidae
Desidae
Desidae
Dictynidae
Dictynidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
218
2.9
3.5
3.4
1.1
0.9
1.2
0.5
0.9
1.2
4.6
2.2
1.4
3.0
3.6
2.7
2.0
1.5
2.9
2.7
2.0
2.1
1.8
2.7
length (mm)
behaviour
No
Carapace
Burrowing
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Heavy
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
Some
Some
Some
None
None
None
None
None
None
None
None
None
Some
Some
Some
Full
Full
Some
None
None
None
None
None
scutes
Abdominal
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
A list of all species with scored traits and emergent group allocation (note: due to size, the table has been split into two sections)
Appendix S2
Species
Encoptarthria sp.33
Encoptarthria sp.34
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Genus 1 sp.09
Genus 1 sp.10
Genus 1 sp.12
Genus 1 sp.13
Genus 1 sp.16
Genus 1 sp.17
Genus 1 sp.18
Genus 1 sp.21
Genus 1 sp.22
Genus 1 sp.24
Genus 1 sp.25
Genus 1 sp.27
Genus 1 sp.28
Genus 1 sp.29
Genus 1 sp.30
Genus 1 sp.31
Genus 1 sp.32
Hemicloea sp.20
Family
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Appendix S2 cont.
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
219
1.4
1.3
1.5
2.0
1.6
1.9
2.3
1.3
1.9
1.1
1.8
1.3
1.3
1.7
1.6
1.2
1.7
1.6
0.9
0.8
1.9
1.1
1.4
2.0
4.1
length (mm)
behaviour
No
Carapace
Burrowing
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
None
Full
None
None
Some
None
None
None
Some
None
None
None
Some
Some
Some
Some
Some
Some
None
None
Some
Some
Some
Some
Some
scutes
Abdominal
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
Yes
Yes
No
No
Hemicloea sp.26
Laronius sp.19
Asadipus banjiwarn Platnick, 2000
Lamponina asperrima (Hickman, 1950)
Lamponata daviesae Platnick, 2000
Lamponina elongata Platnick, 2000
Lampona quinqueplagiata Simon, 1908
Lamponina scutata (Strand, 1913)
Erigone prominens Bösenberg & Strand, 1906
Genus 1 sp.01
Hoggicosa alfi Langlands & Framenau, 2010
Hoggicosa bicolor (Hogg, 1905)
Knoelle clara (L. Koch, 1877)
‘Pexa grp.' sp.04
‘Yalkara grp.' sp.02
‘Yalkara grp.' sp.03
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Genus 1 sp.06
Genus 1 sp.08
Miturga sp.05
Miturga sp.07
Gnaphosidae
Gnaphosidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Linyphiidae
Liocranidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
No
No
No
No
No
No
No
No
Yes
Yes
No
No
No
No
No
No
No
No
No
No
No
Hemicloea sp.23
220
9.0
5.0
4.1
3.8
3.9
4.6
3.5
3.4
5.9
6.8
4.5
7.9
7.4
9.4
1.0
0.8
3.8
2.2
2.8
1.2
2.4
1.9
2.5
1.8
2.0
length (mm)
behaviour
Gnaphosidae
Carapace
Burrowing
Species
Family
Appendix S2 cont.
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Heavy
Normal
Heavy
Heavy
Heavy
Heavy
Heavy
Heavy
Normal
Normal
Normal
carapace
Sclerotisation of
None
None
None
None
None
None
None
None
None
None
None
None
None
None
Full
None
Some
Some
Some
Some
Some
Full
None
None
None
scutes
Abdominal
No
No
No
No
No
No
No
No
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
No
No
No
No
No
No
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
Species
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.05
Kwonkan sp.01
Kwonkan sp.06
Yilgarnia sp.04
Cavisternum sp.07
Grymeus sp.04
Grymeus sp.09
Myrmopopaea sp.01
Myrmopopaea sp.05
Myrmopopaea sp.08
Myrmopopaea sp.14
Myrmopopaea sp.15
Opopaea sp.02
Opopaea sp.03
Opopaea sp.06
Opopaea sp.12
Opopaea sp.13
Opopaea sp.16
Xestaspis sp.10
Xestaspis sp.11
Oxyopes sp.01
Oxyopes sp.02
Oxyopes dingo Strand, 1913
Family
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oxyopidae
Oxyopidae
Oxyopidae
Appendix S2 cont.
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Yes
Yes
Yes
Yes
Yes
221
3.0
2.6
2.0
1.1
1.3
0.5
0.6
0.5
0.9
0.6
0.6
0.8
0.6
0.5
0.8
0.7
0.9
1.0
0.5
4.5
4.5
5.2
6.3
5.4
3.4
length (mm)
behaviour
Yes
Carapace
Burrowing
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Heavy
Heavy
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
None
None
None
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
Full
None
None
None
None
None
None
scutes
Abdominal
Yes
Yes
Yes
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
long
long
long
long
long
long
maturity
Time to
No
No
Genus 1 sp.01
Genus 1 sp.02
Trichocyclus arabana Huber, 2001
Trichocyclus nigropunctatus Simon, 1908
Cryptoerithus halli Platnick & Baehr, 2006
Cryptoerithus occultus Rainbow, 1915
Molycria vokes Platnick & Baehr, 2006
Nomindra sp.01 (cf. cooma)
Nomindra sp.02
Nomindra leeuweni Platnick & Baehr, 2006
Wesmaldra learmonth Platnick & Baehr, 2006
Wydundra kennedy Platnick & Baehr, 2006
Wydundra sp.03
Wydundra sp.04
‘Clynotis albobarbatus grp.' sp.10
Damoetas sp.13
Damoetas sp.17
Genus 1 sp.23
Genus 1 sp.02 'big embolus grp.'
Genus 1 sp.27 'big embolus grp.'
Grayenulla sp.01
Holoplatys sp.07 (cf. planissima)
Holoplatys sp.14
Lycidas chlorophthalmus (Simon, 1909)
Philodromidae
Philodromidae
Pholcidae
Pholcidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Oxyopes rubicundus L. Koch, 1878
222
3.2
1.9
1.9
1.7
1.9
1.5
1.6
1.9
2.2
2.7
2.0
2.8
1.7
1.4
0.9
0.9
0.8
1.8
1.2
1.4
1.0
1.0
1.3
2.5
2.0
length (mm)
behaviour
Oxyopidae
Carapace
Burrowing
Species
Family
Appendix S2 cont.
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
Some
Some
Some
Some
Some
Some
Some
Some
Full
Some
None
Some
Some
None
Some
Full
None
None
None
Some
Some
Some
None
None
None
scutes
Abdominal
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
No
No
No
No
No
No
No
No
No
No
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
No
No
No
No
No
Lycidas grp. sp.11
Lycidas grp. sp.12
‘Neon' sp.15
Ocrisiona yakatunyae Żabka, 1990
Paraplatoides sp.03
Paraplatoides sp.06
Pellenes bitaeniata (Keyserling, 1882)
Zebraplatys keyserlingi Żabka, 1992
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.07
Genus 1 sp.08
Genus 1 sp.12
Genus 1 sp.13
Hadrotarsus sp.10
Hadrotarsus sp.11
Latrodectus sp.09
Steatoda sp.01
Steatoda sp.02
Steatoda sp.03
Steatoda sp.04
Steatoda sp.05
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Segestriidae
Segestriidae
Sparassidae
Sparassidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Yes
Yes
No
No
No
No
Lycidas sp.08
223
1.1
1.0
1.3
1.2
0.9
1.1
0.6
0.5
0.6
0.7
0.9
0.9
4.9
3.1
2.9
2.5
1.8
1.5
2.9
2.8
3.7
0.7
1.7
3.2
1.5
length (mm)
behaviour
Salticidae
Carapace
Burrowing
Species
Family
Appendix S2 cont.
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
Some
Some
Some
Some
Some
Some
Full
Full
Some
Some
Some
None
None
None
None
None
Some
None
Some
Some
Some
Full
Some
Some
Full
scutes
Abdominal
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
No
No
No
No
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
Species
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Stephanopis sp.03
Fissarena castanea (Simon, 1908)
Australutica quaerens Jocqué, 1995
Australutica sp.01 (cf. quaerens)
Cavasteron sp.32 (cf. crassicalcar)
Genus 1 sp.31
Genus 1 sp.33
Genus 1 sp.34
Habronestes bicornis Baehr, 2003
Habronestes sp.13 (cf. longiconductor)
Habronestes sp.16 (cf. grahami)
Habronestes sp.18 (cf. hamatus)
Habronestes sp.21
Habronestes sp.30
Masasteron piankai Baehr, 2004
Neostorena sp.02
Neostorena sp.03
Neostorena sp.05
Spinasteron cavasteroides Baehr & Churchill, 2003
Family
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Trochanteriidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Appendix S2 cont.
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
224
2.3
4.3
6.4
2.5
3.3
3.0
2.6
3.3
2.1
3.0
2.6
1.8
2.6
2.6
2.6
2.3
2.4
4.2
4.2
2.3
3.7
1.5
1.8
1.2
length (mm)
behaviour
No
Carapace
Burrowing
Normal
Heavy
Heavy
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
Some
Some
Some
Some
Some
Some
Some
Some
Some
Some
Some
Some
Some
Some
None
Some
Some
None
Some
Some
None
None
None
None
scutes
Abdominal
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Yes
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
short
maturity
Time to
Species
Argoctenus sp.01
Argoctenus sp.02
Argoctenus sp.03
Argoctenus sp.04
Argoctenus sp.05
Argoctenus sp.08
Genus 1 sp.10
Family
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Appendix S2 cont.
No
No
No
No
No
No
225
2.7
3.0
1.8
2.0
2.5
2.8
2.6
length (mm)
behaviour
No
Carapace
Burrowing
Normal
Normal
Normal
Normal
Normal
Normal
Normal
carapace
Sclerotisation of
None
None
None
None
None
None
None
scutes
Abdominal
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Ballooning
short
short
short
short
short
short
short
maturity
Time to
Species
Cheiracanthium sp.05
Clubiona sp.01
Clubiona sp.02
Clubiona sp.03
Clubiona sp.04
Battalus sp.04
Genus 1 sp.01
Poecilipta sp.02
Poecilipta sp.03
Supunna funerea Simon, 1896
Supunna picta (L. Koch, 1873)
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Phryganoporus sp.01
Genus 1 sp.01
Genus 1 sp.02
Ceryerda cursitans Simon, 1909
Eilica sp.07
Eilica sp.11
Encoptarthria sp.01
Encoptarthria sp.08
Encoptarthria sp.15
Encoptarthria sp.33
Family
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Clubionidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Corinnidae
Desidae
Desidae
Desidae
Desidae
Dictynidae
Dictynidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Appendix S2 cont.
226
Three
Three
Six
Three
Nine
Nine
Nine
Three
Six
Nine
Three
Three
Three
Nine
Three
Nine
Six
Three
Six
Six
Three
Three
Nine
Three
Phenology
Active
Active
Active
Active
Active
Active
Active
TerrWeb
TerrWeb
TerrWeb
TerrWeb
TerrWeb
TerrWeb
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
Yes
No
No
No
No
No
diet on ants
strategy
Active
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
II
II
II
II
I
I
I
I
I
I
I
I
I
II
II
II
IV
IV
III
I
I
I
I
I
group
Emergent
Gnap_Enco_33
Gnap_Enco_15
Gnap_Enco_08
Gnap_Enco_01
Gnap_Eili_11
Gnap_Eili_07
Gnap_Cery_curs
Dict_Gen01_02
Dict_Gen01_01
Desi_Phry_01
Desi_Gen01_04
Desi_Gen01_03
Desi_Gen01_02
Cori_Supu_pict
Cori_Supu_fune
Cori_Poec_03
Cori_Poec_02
Cori_Gen01_01
Cori_Batt_04
Club_Club_04
Club_Club_03
Club_Club_02
Club_Club_01
Club_Chei_01
for cluster analysis
Abbreviated names
Species
Encoptarthria sp.34
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Genus 1 sp.09
Genus 1 sp.10
Genus 1 sp.12
Genus 1 sp.13
Genus 1 sp.16
Genus 1 sp.17
Genus 1 sp.18
Genus 1 sp.21
Genus 1 sp.22
Genus 1 sp.24
Genus 1 sp.25
Genus 1 sp.27
Genus 1 sp.28
Genus 1 sp.29
Genus 1 sp.30
Genus 1 sp.31
Genus 1 sp.32
Hemicloea sp.20
Hemicloea sp.23
Family
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Gnaphosidae
Appendix S2 cont.
Three
Three
Three
Three
Three
Three
Three
Three
Six
Six
Six
Three
Six
Three
Three
Three
Three
Nine
Six
Six
Nine
Six
Nine
Nine
Three
227
Phenology
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
diet on ants
strategy
Active
Specialized
Hunting
Flat
Flat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
II
II
IV
I
I
II
I
I
I
II
I
I
I
II
II
II
II
II
II
I
I
II
II
II
II
group
Emergent
Gnap_Hemi_23
Gnap_Hemi_20
Gnap_Gen01_32
Gnap_Gen01_31
Gnap_Gen01_30
Gnap_Gen01_29
Gnap_Gen01_28
Gnap_Gen01_27
Gnap_Gen01_25
Gnap_Gen01_24
Gnap_Gen01_22
Gnap_Gen01_21
Gnap_Gen01_18
Gnap_Gen01_17
Gnap_Gen01_16
Gnap_Gen01_13
Gnap_Gen01_12
Gnap_Gen01_10
Gnap_Gen01_09
Gnap_Gen01_06
Gnap_Gen01_05
Gnap_Gen01_04
Gnap_Gen01_03
Gnap_Gen01_02
Gnap_Enco_34
for cluster analysis
Abbreviated names
Three
Three
Three
Three
Laronius sp.19
Asadipus banjiwarn Platnick, 2000
Lamponina asperrima (Hickman, 1950)
Lamponata daviesae Platnick, 2000
Lamponina elongata Platnick, 2000
Lampona quinqueplagiata Simon, 1908
Lamponina scutata (Strand, 1913)
Erigone prominens Bösenberg & Strand, 1906
Genus 1 sp.01
Hoggicosa alfi Langlands & Framenau, 2010
Hoggicosa bicolor (Hogg, 1905)
Knoelle clara (L. Koch, 1877)
‘Pexa grp.' sp.04
‘Yalkara grp.' sp.02
‘Yalkara grp.' sp.03
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.03
Genus 1 sp.04
Genus 1 sp.06
Genus 1 sp.08
Miturga sp.05
Miturga sp.07
Genus 1 sp.02
Gnaphosidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Lamponidae
Linyphiidae
Liocranidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Lycosidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Miturgidae
Nemesiidae
Six
Six
Six
Six
Three
Three
Three
Nine
Six
Six
Six
Three
Six
Six
Nine
Three
Nine
Three
Three
Three
Three
Hemicloea sp.26
Gnaphosidae
228
Phenology
Species
Family
Appendix S2 cont.
Burrow
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Burrow
Burrow
Burrow
Burrow
Active
TerrWeb
Active
Active
Active
Active
Active
Active
Active
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
diet on ants
strategy
Active
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
Flat
body
Flattened
V
I
I
I
I
I
I
I
I
I
I
V
V
V
V
IV
I
III
III
III
III
III
IV
I
II
group
Emergent
Neme_Gen01_02
Mitu_Mitu_07
Mitu_Mitu_05
Mitu_Mitu_08
Mitu_Mitu_06
Mitu_Mitu_04
Mitu_Mitu_03
Mitu_Mitu_02
Mitu_Mitu_01
Lyco_Yalk_03
Lyco_Yalk_02
Lyco_Pexa_04
Lyco_Knoe_clar
Lyco_Hogg_bico
Lyco_Hogg_alfi
Lioc_Gen01_01
Liny_Erig_prom
Lamp_Lamp_scut
Lamp_Lamp_quin
Lamp_Lamp_elon
Lamp_Lamp_davi
Lamp_Lamp_aspe
Lamp_Asad_banj
Gnap_Laro_19
Gnap_Hemi_26
for cluster analysis
Abbreviated names
Species
Genus 1 sp.03
Genus 1 sp.05
Kwonkan sp.01
Kwonkan sp.06
Yilgarnia sp.04
Cavisternum sp.07
Grymeus sp.04
Grymeus sp.09
Myrmopopaea sp.01
Myrmopopaea sp.05
Myrmopopaea sp.08
Myrmopopaea sp.14
Myrmopopaea sp.15
Opopaea sp.02
Opopaea sp.03
Opopaea sp.06
Opopaea sp.12
Opopaea sp.13
Opopaea sp.16
Xestaspis sp.10
Xestaspis sp.11
Oxyopes sp.01
Oxyopes sp.02
Oxyopes dingo Strand, 1913
Oxyopes rubicundus L. Koch, 1878
Family
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Nemesiidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oonopidae
Oxyopidae
Oxyopidae
Oxyopidae
Oxyopidae
Appendix S2 cont.
Nine
Nine
Three
Six
Three
Nine
Nine
Nine
Three
Nine
Nine
Three
Three
Six
Three
Nine
Nine
Nine
Six
Nine
Three
Three
Three
Three
Three
229
Phenology
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Burrow
Burrow
Burrow
Burrow
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
diet on ants
strategy
Burrow
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
I
I
I
I
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
IV
V
V
V
V
V
group
Emergent
Oxyo_Oxyo_rubi
Oxyo_Oxyo_ding
Oxyo_Oxyo_02
Oxyo_Oxyo_dess
Oono_Xest_11
Oono_Xest_10
Oono_Opop_16
Oono_Opop_13
Oono_Opop_12
Oono_Opop_06
Oono_Opop_03
Oono_Opop_02
Oono_Myrm_15
Oono_Myrm_14
Oono_Myrm_08
Oono_Myrm_05
Oono_Myrm_01
Oono_Grym_09
Oono_Grym_04
Oono_Cavi_07
Neme_Yilg_04
Neme_Kwon_06
Neme_Kwon_01
Neme_Gen01_05
Neme_Gen01_03
for cluster analysis
Abbreviated names
Three
Three
Genus 1 sp.02
Trichocyclus arabana Huber, 2001
Trichocyclus nigropunctatus Simon, 1908
Cryptoerithus halli Platnick & Baehr, 2006
Cryptoerithus occultus Rainbow, 1915
Molycria vokes Platnick & Baehr, 2006
Nomindra sp.01 (cf. cooma)
Nomindra sp.02
Nomindra leeuweni Platnick & Baehr, 2006
Wesmaldra learmonth Platnick & Baehr, 2006
Wydundra kennedy Platnick & Baehr, 2006
Wydundra sp.03
Wydundra sp.04
‘Clynotis albobarbatus grp.' sp.10
Damoetas sp.13
Damoetas sp.17
Genus 1 sp.23
Genus 1 sp.02 'big embolus grp.'
Genus 1 sp.27 'big embolus grp.'
Grayenulla sp.01
Holoplatys sp.07 (cf. planissima)
Holoplatys sp.14
Lycidas chlorophthalmus (Simon, 1909)
Lycidas sp.08
Philodromidae
Pholcidae
Pholcidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Prodidomidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Nine
Three
Three
Three
Nine
Nine
Nine
Three
Three
Three
Three
Six
Three
Nine
Six
Nine
Three
Three
Six
Nine
Nine
Three
Three
Genus 1 sp.01
Philodromidae
230
Phenology
Species
Family
Appendix S2 cont.
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
TerrWeb
TerrWeb
Sit&Wait
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
diet on ants
strategy
Sit&Wait
Specialized
Hunting
NotFlat
NotFlat
Flat
Flat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
IV
II
II
II
II
II
II
II
II
IV
II
I
III
III
I
III
IV
I
I
I
III
II
II
I
I
group
Emergent
Salt_Lyci_08
Salt_Lyci_chlo
Salt_Holo_14
Salt_Holo_07
Salt_Gray_01
Salt_Gen01_27
Salt_Gen01_02
Salt_Gen01_23
Salt_Damo_17
Salt_Damo_13
Salt_Clyn_10
Prod_Wydu_04
Prod_Wydu_03
Prod_Wydu_kenn
Prod_Wesm_lear
Prod_Nomi_leeu
Prod_Nomi_02
Prod_Nomi_01
Prod_Moly_voke
Prod_Cryp_occu
Prod_Cryp_hall
Phol_Tric_nigr
Phol_Tric_arab
Phil_Gen01_02
Phil_Gen01_01
for cluster analysis
Abbreviated names
Six
Three
Six
Six
Three
Lycidas grp. sp.12
‘Neon' sp.15
Ocrisiona yakatunyae Żabka, 1990
Paraplatoides sp.03
Paraplatoides sp.06
Pellenes bitaeniata (Keyserling, 1882)
Zebraplatys keyserlingi Żabka, 1992
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.01
Genus 1 sp.02
Genus 1 sp.07
Genus 1 sp.08
Genus 1 sp.12
Genus 1 sp.13
Hadrotarsus sp.10
Hadrotarsus sp.11
Latrodectus sp.09
Steatoda sp.01
Steatoda sp.02
Steatoda sp.03
Steatoda sp.04
Steatoda sp.05
Genus 1 sp.01
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Salticidae
Segestriidae
Segestriidae
Sparassidae
Sparassidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Theridiidae
Thomisidae
Three
Nine
Six
Nine
Nine
Nine
Three
Three
Nine
Six
Nine
Six
Three
Nine
Three
Six
Six
Three
Three
Six
Lycidas grp. sp.11
Salticidae
231
Phenology
Species
Family
Appendix S2 cont.
Sit&Wait
TerrWeb
TerrWeb
TerrWeb
TerrWeb
TerrWeb
TerrWeb
Active
Active
TerrWeb
TerrWeb
TerrWeb
TerrWeb
Sit&Wait
Sit&Wait
Burrow
Burrow
Active
Active
Active
Active
Active
Active
Active
No
No
No
No
No
No
No
Yes
Yes
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
No
diet on ants
strategy
Active
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
Flat
NotFlat
NotFlat
Flat
NotFlat
Flat
Flat
Flat
NotFlat
NotFlat
NotFlat
body
Flattened
I
II
II
II
II
II
II
IV
IV
II
II
II
I
I
I
V
V
II
I
II
II
II
IV
II
II
group
Emergent
Thom_Gen01_01
Ther_Stea_05
Ther_Stea_04
Ther_Stea_03
Ther_Stea_02
Ther_Stea_01
Ther_Latr_09
Ther_Hadr_11
Ther_Hadr_10
Ther_Gen01_13
Ther_Gen01_12
Ther_Gen01_08
Ther_Gen01_07
Spar_Gen01_02
Spar_Gen01_01
Sege_Gen01_02
Sege_Gen01_01
Salt_Zebr_keys
Salt_Pell_bita
Salt_Para_06
Salt_Para_03
Salt_Ocri_yaka
Salt_Gen01_15
Salt_Lyci_12
Salt_Lyci_11
for cluster analysis
Abbreviated names
Species
Genus 1 sp.02
Genus 1 sp.04
Genus 1 sp.05
Genus 1 sp.06
Stephanopis sp.03
Fissarena castanea (Simon, 1908)
Australutica quaerens Jocqué, 1995
Australutica sp.01 (cf. quaerens)
Cavasteron sp.32 (cf. crassicalcar)
Genus 1 sp.31
Genus 1 sp.33
Genus 1 sp.34
Habronestes bicornis Baehr, 2003
Habronestes sp.13 (cf. longiconductor)
Habronestes sp.16 (cf. grahami)
Habronestes sp.18 (cf. hamatus)
Habronestes sp.21
Habronestes sp.30
Masasteron piankai Baehr, 2004
Neostorena sp.02
Neostorena sp.03
Neostorena sp.05
Spinasteron cavasteroides Baehr & Churchill, 2003
Argoctenus sp.01
Family
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Thomisidae
Trochanteriidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zodariidae
Zoridae
Appendix S2 cont.
Six
Six
Three
Three
Three
Three
Six
Three
Three
Three
Three
Three
Three
Three
Three
Three
Three
Three
Six
Three
Three
Three
Three
Three
232
Phenology
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Active
Sit&Wait
Sit&Wait
Sit&Wait
Sit&Wait
No
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
Yes
No
No
No
No
No
No
diet on ants
strategy
Sit&Wait
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
Flat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
I
III
III
III
III
III
III
III
III
III
III
III
III
III
III
III
III
III
I
I
I
I
I
I
group
Emergent
Zori_Argo_01
Zoda_Spin_cava
Zoda_Neos_05
Zoda_Neos_03
Zoda_Neos_02
Zoda_Masa_pian
Zoda_Habr_30
Zoda_Habr_21
Zoda_Habr_18
Zoda_Habr_16
Zoda_Habr_13
Zoda_Habr_bico
Zoda_Gen01_34
Zoda_Gen01_33
Zoda_Gen01_31
Zoda_Cava_32
Zoda_Aust_01
Zoda_Aust_quae
Troc_Fiss_cast
Thom_Step_03
Thom_Gen01_06
Thom_Gen01_05
Thom_Gen01_04
Thom_Gen01_02
for cluster analysis
Abbreviated names
Species
Argoctenus sp.02
Argoctenus sp.03
Argoctenus sp.04
Argoctenus sp.05
Argoctenus sp.08
Genus 1 sp.10
Family
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Zoridae
Appendix S2 cont.
Three
Three
Three
Three
Three
Three
233
Phenology
Active
Active
Active
Active
Active
No
No
No
No
No
No
diet on ants
strategy
Active
Specialized
Hunting
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
NotFlat
body
Flattened
I
I
I
I
I
I
group
Emergent
Zori_Gen01_10
Zori_Argo_08
Zori_Argo_05
Zori_Argo_04
Zori_Argo_03
Zori_Argo_02
for cluster analysis
Abbreviated names
Appendix S3
Flow diagram of statistical analyses. Squares represent rows by columns matrices, and
triangles are pair-wise similarity half-matrices.
Fourth-corner
see a)
Fourth-corner
see c)
Principal
coordinate
Analysis (PCoA)
see b)
Emergent groups
see d)
a) Fourth-corner on individual traits
sites
traits
species
L
Q
post-fire
age
R
two stage fourth-corner analysis
(permutation model 2 followed by model 4)
b) Linked traits
traits
species
Q
PCoA axes
species
Gower
coefficient
species
s
species
Principal
coordinate
analysis (PCoA)
Q2
c) Combined traits (PCoA) in fourth-corner
sites
traits
L
species
post-fire
age
Q2
two stage fourth-corner analysis
(permutation model 2 followed by model 4)
R
d) Emergent groups (EGs)
dendrogram
sites
species
species
S
Cluster analysis,
Ward’s method
Select
EGs
EGs
Euclidean
distance
PERMANOVAs on
post-fire age for each EG
234
sites
sites
Appendix S4
Non-metric multidimensional scaling (nMDS) of species composition of spiders based
on Bray-Curtis similarity from fourth root transformed data. Each number represents a
site and indicates the post-fire age in years.
2D Stress: 0.23
8
20
8
20
20
20
5
8
5
3
5
5
20
0.5
8
8
5
0.5
0
3
0.5
0
3
0
3
3
0
235
Appendix S5
The loadings of ten traits on the first three PCoA axes . Loadings > 0.5 are bolded.
PCoA Axes
PCoA 1
PCoA 2
PCoA 3
-0.272
-0.841
0.228
0.530
0.259
-0.030
Hunting strategy- Terrestrial Web
-0.168
-0.497
-0.081
Hunting strategy- Burrowing
-0.433
0.236
-0.050
Hunting strategy- Sit & wait
-0.274
-0.064
0.218
0.495
0.377
0.313
Phenology- 3mths
-0.152
0.349
0.861
Phenology- 6mths
-0.104
-0.106
-0.568
Phenology- 9mths
0.285
-0.311
-0.460
Burrowing
-0.433
0.236
-0.050
Body Length
-0.238
0.354
0.321
0.368
0.257
-0.031
Time to maturity
-0.304
0.311
0.025
Flattened body
-0.023
-0.161
0.300
Abdominal scutes- Absent
-0.860
0.081
-0.075
Abdominal scutes- Partial
0.671
-0.204
0.288
Abdominal scutes- Full
0.272
0.167
-0.292
Total variation (%)
37.5
32.3
21.9
Cumulative variation (%)
37.5
69.8
91.7
Ballooning
Hunting strategy- Active
Diet specialization (Ants)
Heavy sclerotisation of carapace
236
Appendix S6
Cluster dendrogram used to define the five emergent groups (Group I – V). A similarity
matrix of ten traits based on the Gower coefficient was used to create the dendrogram
with Ward‟s method. For electronic copy see enclosed CD.
237
Synthesis of Ecological Results and Future Research
I was interested in examining the long-term pattern of response of spiders to fire in
spinifex habitat in the arid zone of Australia. Consistent with previous studies in other
habitats, I found a clear successional pattern. With increasing post-fire age there were
considerable differences in the number of species, evenness and the composition of
species in the spider assemblage (Chapter 2). Based on these parameters, the spider
assemblage seems strongly deterministic, converging on long-unburnt conditions over
time. Also consistent with our current understanding of spider assemblages, post-fire
changes in the species composition and habitat structure of the vegetation explained the
greatest proportions of the variation in richness and composition of the spiders (Chapter
3). Given these results, I anticipated that there would be strong links between the traits
of species and environmental conditions. However, when I tested this, the results were
equivocal (Chapter 4). This incongruence is a little puzzling. Perhaps the traits that I
used are not functional for survival in the post-fire environment, or perhaps they are
divergent traits (traits that allow species to coexist under similar environmental
conditions). Clearly, this requires further investigation, and one potential avenue is to
look at changes in trait space. This approach has recently been applied to post-fire
changes in bee and beetle assemblages using functional diversity (FD) or community
weighted mean (CWM) trait values (e.g. Moretti et al. 2009, Moretti et al. in press).
Another possible avenue to explore these results, particularly the importance of habitat
structure, might be to conduct experimental manipulations of the habitat. The amount of
ground cover, specifically spinifex, could be reduced manually, to see how this
influences the spider assemblage. Does it cause a retrogression of succession as shown
for mammals in heath habitat (Fox et al. 2003)? Masters et al. (2003) conducted a study
in central Australia, where they manually reduced spinifex cover to study the impact on
a carnivorous small marsupial (Dasycercus cristicauda). They found no change in the
total biomass of the invertebrates; however, they did not analyse the species
composition of the invertebrate fauna (Masters et al. 2003).
Although changes in vegetation best explained the changes in the spider assemblage,
rainfall and the presence of predators also explained a significant amount of variation.
Although technically and practically more difficult, the mechanisms behind how these
variables might influence spiders in arid Australia could also be investigated by
238
manipulative experiments. The influence of rainfall via the addition of water could be
studied using the numerous bores on Lorna Glen and most stations. I am unaware of any
study on fauna that has manipulated rainfall in the arid zone of Australia. Variation in
predation pressure by vertebrate predators (lizards and small mammals) could be
examined by exclusion experiments using cages or barriers (see for example Spiller and
Schoener 1998, Manicom et al. 2008).
The spatial location of sites and spatial processes also clearly play a part in structuring
the spider assemblage (Chapter 3). Unfortunately, with the available fire histories, it
was not possible to intersperse completely all fire ages. To account for this, I included a
spatial variable into the permutational analysis of variance as a covariate. Although the
results of pair-wise comparisons were slightly different, this did not result in any major
change (Chapter 2 Appendix B vs Chapter 3 Table 1 and 3). From six to ten of the 15
comparisons were still significant, something which is extremely unlikely to occur by
chance alone (Moran 2003). Therefore, the interpretation of results was not altered.
The available fire histories also restricted the number of true replicates (sensu Hurlbert
1984). I spent many weeks examining the fire histories via satellite images with the aid
of GIS researchers and then „ground truthing‟ potential sites to confirm the fire age,
correct vegetation type and the patchiness or completeness of the historic fires. In
addition to satellite images, I aged the sites by dendrochronology of mallee (Eucalyptus
kingsmillii and E. lucasii). Mallee is a common term given to species that regrow from
underground lignotubers following disturbance. This subsequently proved to be an
unreliable method, so I relied on the satellite data to come up with the best possible
design given the fire histories available on the station. Unfortunately, there were not
enough individual fires to avoid nesting sites in a single fire. However, when this was
the case, I selected sites several kilometres apart, with roads between, in the hope of
collecting independent samples of spiders.
The limitations of my experimental design must also be acknowledged. While some
studies have demonstrated the validity of the chronosequence or space-for-time
approach for certain situations (Twigg et al. 1989, Knops and Tilman 2000), there have
also been several critical assessments over the years (Collins and Adams 1983, Pickett
1989, Johnson and Miyanishi 2008). It can be difficult to assess the assumptions of the
chronosequence approach; that all sites had similar initial conditions, experienced a
239
similar disturbance, and have received similar conditions since disturbance. In the case
of my study, with current techniques, I had little chance of testing these assumptions.
Indeed, with the benefit of hindsight, it seems that the characteristics of the arid zone,
including extreme variability in rainfall in both time and space (Stafford-Smith and
Morton 1990), might make meeting the assumptions required for a chronosequence
difficult. Additionally, the inclusion of sites that received experimental burns that were
smaller than natural fires is a clear violation of these assumptions. However, a space for
time approach provides a snapshot, and one that is achievable within the period of a
Ph.D. program. For this reason, chronosequence studies are still used commonly for
ecological research (Jeffries et al. 2006, Shipley et al. 2006, Wardle et al. 2008, Aubin
et al. 2009), and it is considered a useful approach for fire studies (Clarke 2008).
Ideally, to test the patterns I have found, a long-term study of the spiders is required,
particularly monitoring over the first three years post-fire.
Ultimately, our overall understanding of how the flora and fauna of arid Australia,
including spiders, respond to fire will be advanced most rapidly through a long-term,
large scale, replicated, multidisciplinary study, along the lines of the Kalpaga fire
experiment (Andersen et al. 1998). This however, requires a considerable long-term
input of resources and a commitment to maintain experimental fire regimes. In addition,
to examine aspects of the fire regime that are difficult to replicate, such as mosaics,
another approach would be to conduct a large scale, multidisciplinary chronosequence
study, similar to that currently underway in the mallee region of Eastern Australia
(Clarke et al. 2006). Along with the need to manage biodiversity, the challenge of
anthropogenic climate change adds urgency to such research. Understanding how
increased temperatures and changes in rainfall will further alter the fire regimes of
inland Australia and the consequences for biodiversity and carbon fluxes will be vital
for conservation in the future.
240
References
Andersen, A. N., Braithwaite, R. W., Cook, G. D., Corbett, L. K., Williams, R. J.,
Douglas, M. M., Gill, A. M., Setterfield, S. A. & Muller, W. J. (1998) Fire
research for conservation management in tropical savannas: Introducing the
Kapalga fire experiment. Australian Journal of Ecology, 23, 95-110.
Aubin, I., Ouellette, M.-H., Legendre, P., Messier, C. & Bouchard, A. (2009)
Comparison of two plant functional approaches to evaluate natural restoration
along an old-field - deciduous forest chronosequence. Journal of Vegetation
Science, 20, 185-198.
Clarke, M. F. (2008) Catering for the needs of fauna in fire management: science or just
wishful thinking? Wildlife Research, 35, 385-394.
Clarke, M. F., Bennett, A., Callister, K., Ferguson, S., Kelly, L., Kenny, S., Nimmo, D.,
Spence-Bailey, L., Taylor, R. & Watson, S. (2006) Mallee Fire and Biodiversity
Project: Determining appropriate fire regimes in the Murray Mallee.
Collins, S. L. & Adams, D. E. (1983) Succession in grasslands: Thirty-two years of
change in a central Oklahoma tallgrass prairie. Plant Ecology, 51, 181-190.
Fox, B. J., Taylor, J. E. & Thompson, P. T. (2003) Experimental manipulation of habitat
structure: a retrogression of the small mammal succession. Journal of Animal
Ecology, 72, 927-940.
Hurlbert, S. H. (1984) Pseudoreplication and the design of ecological experiments.
Ecological Monographs, 54, 187-211.
Jeffries, J. M., Marquis, R. J. & Forkner, R. E. (2006) Forest age influences oak insect
herbivore community structure, richness, and density. Ecological Applications,
16, 901-912.
Johnson, E. A. & Miyanishi, K. (2008) Testing the assumptions of chronosequences in
succession. Ecology Letters, 11, 419-431.
Knops, J. M. H. & Tilman, D. (2000) Dynamics of soil nitrogen and carbon
accumulation for 61 years after agricultural abandonment. Ecology, 81, 88-98.
Manicom, C., Schwarzkopf, L., Alford, R. A. & Schoener, T. W. (2008) Self-made
shelters protect spiders from predation. Proceedings of the National Academy of
Sciences, 105, 14903-14907.
Masters, P., Dickman, C. R. & Crowther, M. (2003) Effects of cover reduction on
mulgara Dasycercus cristicauda (Marsupialia: Dasyuridae), rodent and
invertebrate populations in central Australia: implications for land management.
Austral Ecology, 28, 658-665.
241
Moran, M. D. (2003) Arguments for rejecting the sequential Bonferroni in ecological
studies. Oikos, 100, 403-405.
Moretti, M., De Bello, F., Roberts, S. & Potts, S. G. (2009) Taxonomical vs. functional
responses of bee communities to fire in two contrasting climatic regions.
Journal of Animal Ecology, 78, 98-108.
Moretti, M., De Cáceres, M., Pradella, C., Obrist, M. K., Wermelinger, B., Legendre, P.
& Duelli, P. (in press) Fire-induced taxonomic and functional changes in
saproxylic beetle communities in fire sensitive regions. Ecography.
Pickett, S. T. A. (1989) Space-for-time substitution as an alternative to long-term
studies. Long-Term Studies in Ecology: Approaches and Alternatives (ed G. E.
Likens), pp. 110-135. Springer-Verlag, New York.
Shipley, B., Vile, D. & Garnier, E. (2006) From plant traits to plant communities: a
statistical mechanistic approach to biodiversity. Science, 314, 812-814.
Spiller, D. A. & Schoener, T. W. (1998) Lizards reduce spider species richness by
excluding rare species. Ecology, 79, 503-516.
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Australia. Journal of Arid Environments, 18, 255-278.
Twigg, L. E., Fox, B. J. & Jia, L. (1989) The modified primary succession following
sand mining: a validation of the use of chronosequence analysis. Australian
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Wardle, D. A., Bardgett, R. D., Walker, L. R., Peltzer, D. A. & Lagerstrom, A. (2008)
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242
CONCLUSION
Fire is a common disturbance in many ecosystems and an integral part of arid Australia.
The displacement of Aboriginal peoples in recent history led to a change in fire regimes
in spinifex habitats of arid Australia. To conserve Australia‟s arid biodiversity it is
crucial to fill in the many gaps in our current knowledge of how the fauna and flora
respond to fire. This is particularly true for spiders, where there are several obstacles to
successful biodiversity conservation, including the taxonomic impediment and a better
understanding of post-fire response patterns. I set out to improve our knowledge for the
conservation of spiders in arid Australia by removing part of this taxonomic
impediment and examining the long-term response of spiders to fire.
To help remove the taxonomic impediment and facilitate my investigations of the postfire response of spiders, I revised the taxonomy and systematics of a charismatic and
common genus of wolf spiders. The Australian wolf spider genus Hoggicosa Roewer,
1960 now includes ten species and a phylogenetic analysis supports the monophyly of
Hoggicosa. My analysis found that an unusual sexual dimorphism for wolf spiders
(females more colourful than males), evident in four species of Hoggicosa, has evolved
multiple times. Hoggicosa are large, burrowing lycosids, which will prove ideal models
for further evolutionary and ecological studies.
In my ecological studies, using a chronosequence approach, I found significant nonlinear changes in species richness and evenness, as well as marked changes in the
species composition of spiders with increasing post-fire age. However, there was no
difference in multivariate dispersion within ages. While it appears that all sites converge
towards long unburnt sites, a longitudinal study would be required to confirm these
findings and shed light on the changes within the first three years following disturbance
by fire. This could also test the two alternative hypotheses that I propose to explain the
return trajectory of sites burnt experimentally. Sampling regularly over this period could
uncover a lag in the full impact of disturbance by fire (inertia) or a rapid recolonization
from the surrounding areas.
243
Although only correlative, for the first time, I have quantified the ability of seven
different variables (Fire, Rainfall, Soil, Habitat, Floristics, Predators and Space) to
explain post-fire changes in a spider assemblage. These results now focus attention and
highlight future manipulative experiments that can further develop our understanding of
the post-fire response of spiders in the Australian arid zone.
Finally, I have attempted to develop a predictive understanding of how spiders respond
to fire by adapting an approach from plant ecologists. The development of a traits-based
approach, which is highly novel, was less successful than hoped. However, the
development of such a mechanistic approach still deserves considerable attention. I
therefore consider this thesis makes a substantial contribution of new knowledge to
assist with conservation of spiders in the arid zone of Australia.
244