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Remots Sensing and Hydrology 2000 (Proceedings of a s y m p o s i u m held at Santa Fe, N e w M e x i c o , U S A , April 2000). I A H S Publ. no. 267, 2 0 0 1 . 3 Satellite remote sensing of precipitation: progress and problems ERIC C. B A R R E T T Centre for Remote Sensing, Bristol BS8 1SS, UK School of Geographical Sciences, University of Bristol, e - m a i l : c.c,barrett(5ibris.ac,uk Abstract Thirty years after satellite data were first used for assessing rainfall it is appropriate to critically review what has been achieved in this field to date, and what has not. Good progress has been made in developing and understanding the capabilities of satellite sensing systems, the physics of the atmosphere and land surfaces of the Earth, and in the development of computers capable of multiple, high-speed operations for near real-time data processing. However, all types of satellite monitoring of falling precipitation are subject to limitations, and progress is still relatively poor in several regards. To make matters worse, there has been a global trend towards the collection of less, not more, in situ data on precipitation over at least half of the last century. Foci for further research and operations are proposed. Some problems will require concentrated effort and significant expenditure if the recent rate of progress in this field is even to be maintained. K e y w o r d s a p p l i c a t i o n s ; infrared; m i c r o w a v e ; o p e r a t i o n s ; p r e c i p i t a t i o n ; p r o g r e s s ; r e m o t e s e n s i n g ; r e s e a r c h ; satellite; v i s i b l e INTRODUCTION Precipitation is a notoriously difficult parameter to evaluate, first and foremost because of its high spatial and temporal variability. Although most locations on the Earth's surface experience precipitation some time in the course of any one year, and some locations on more days than not, instantaneous precipitation is a rare phenomenon. The area of the globe covered at any one time by falling precipitation has been estimated from surface evidence as being probably below 1% (Barrett & Martin, 1981), and "typically occurs only a very small fraction of the time over any given location ..." (Theon, 1992), though satellite-based studies increasingly suggest that the true frequency of occurrence may be a few percentage points higher then earlier thought, at maybe even about 3 - 4 % in the spatial domain. Meanwhile, at any one instant, precipitation intensities around the globe range from zero to >125 m m h" . Further complicating the measurement problem, rainfall can vary by orders of magnitude of intensity in both space and time over distances of no more than tens of metres, and in a matter of minutes or even seconds. Simultaneously, towards the low end of the rain rate spectrum, gradients of intensity can be quite shallow, and it is never easy by any means to determine no-rain boundaries simply and with confidence. For global weather forecasting purposes rainfall is measured by raingauges, some of whose data are circulated in near real-time via the Global Telecommunication System (GTS) of the World Meteorological Organisation (WMO). For climate analysis purposes supplementary raingauge networks containing several times more gauges are 1 4 E. C. Barrett operated in most countries, though typically these are managed by more than one (and perhaps even several) environmental monitoring agencies within any one country, this often causing severe problems when attempts are made to collect data for "best possible" rainfall studies. As if all this were not difficult enough, still further problems are encountered by anyone seeking to use raingauge data to evaluate rainfall over wide regions and/or the globe as a whole. These include the following (Barrett & Beaumont, 1994): There are many different raingauge types. Different classes or families of raingauges record rainfall for widely different periods of time, ranging from very short intervals (even as short as seconds) in the case of some "hydrographs" (continuously-recording raingauges), up to very long intervals (even as long as months or seasons) in the case of some "accumulating" precipitation gauges. The shapes and sizes of raindrops or other precipitation particles and their behaviour in the vicinity of raingauges, and in relation to local surface conditions, are many and varied. Deficiencies in rainfall station management and data quality control are common place, also seriously affecting both the rainfall data supply and its subsequent utility. Of special significance in the context of extreme events, it may not be possible to obtain "real-time" data related to very high intensity rainfall because of storm disruption of gauges, radar or supporting infrastructures. Rainfall radars are designedly better able to reveal continuous pictures of the spatial distribution of rainfall than the average gauge network, and for the most part provide data used qualitatively, and locally or regionally, for very short-term forecasting ("nowcasting") activities and related research. Collier (1989) has concluded that there are still "... few examples of (radar) systems which produce quantitative (precipitation) data operationally" and that important "... sources of error in radar measurements arise from the characteristics of the precipitation particularly in the vertical". Proportionately more rainfall radars are located in middle latitudes than in the tropics. Existing raingauge and radar densities are not nearly adequate either for global rainfall monitoring, even when quite sophisticated statistical or mathematical proc edures are applied to the resulting scatters of point or local area data in order to extrapolate from them across intervening conventional data remote regions, and so provide spatially-complete inventories of this key variable, or for regional rainfall monitoring in most areas. Theon (1992) commented that "It is remarkable that as important as rain is to us, we really do not know its geographical distribution to within a factor of two over much of the Earth." Rasmusson & Arkin (1992) concluded that "Continuous global monitoring of this variable is a challenging task. Surface-based observations are totally inadequate for estimating rainfall over the ocean areas of the tropics, where surface observations are essentially non-existent except for potentially non-representative island stations, and over most of the continental areas as well". Making the problem of variability much worse, especially where mountainous landfalls are involved, both the temporal and spatial variations of rainfall may approach, and often establish, new global record levels. Satellite remote sensing ofprecipitation: progress and problems 5 Thus, estimation and prediction of rainfall represents one of the biggest scientific challenges in satellite meteorology and climatology, not least because it involves both the upper and lower extremities of the statistical distributions of rainfall rates, totals and variabilities. P R O G R E S S IN SATELLITE R E M O T E SENSING OF PRECIPITATION General comments Historically, satellite meteorology may be said to have begun in April 1960 along with the launch of the first Television and InfraRed Observation Satellite (TIROS-1) designed primarily for global weather monitoring. Since then many "environmental" satellites have been operated for such purposes, providing relatively low spatial resolution data (mostly between 0.5 km and 50 km at the Earth's surface), relatively frequently (mostly between successive images at a given location, between 30-min and 3-day intervals). Through the same period, great advances have been made both in the capacities of the satellite "buses" available to carry Earth-observing instrument payloads into space, and in the capabilities of instruments to provide data of the types, qualities and quantities required by precipitation information end-users. Three types of electromagnetic radiation from the target have proven particularly valuable for the estimation of rainfall from environmental satellites, namely VIS (visible), IR (thermal) and M W (microwave) radiation. To the satellite meteorologist VIS includes short-wave radiation (sunlight) reflected back towards space from the tops of clouds mostly within the 0.4-0.7 urn region of the electromagnetic spectrum; characteristically, the spatial resolution of such data is from about 0.5-2.5 um. Thermal IR is longer wavelength radiation, mostly measured within the 10.6-12.6 um region, the result of absorption of some incoming solar radiation by the Earth and its atmosphere, plus radiation subsequently re-emitted towards space as heat energy; spatial resolutions of IR data are characteristically similar to those of VIS data. M W is even longer wavelength energy, re-emitted or reflected towards space, and mainly exploited for rainfall measurements between wavelengths of about 0.3-3 cm (frequencies ranging from 90-10 GHz); here the spatial resolutions of sensors are lower than with either the VIS or the IR, mostly from about 10 km to 50 km. The principal reason for the relatively poor spatial resolutions of the M W sensors is not the signal-tonoise ratio, as might be supposed, but diffraction. In this case there is a modest additional decrease in resolution owing to the time-integration of the received power. The best spatial resolution cited above for an environmental satellite sensor (0.5 km) relates to a VIS system (part of the Operational Line Scan (OLS) sensor on current U S Defense Meteorological Satellite Program (DMSP) spacecraft), whilst the lowest (about 50 km) relates to a M W sensor (the 19.35 GHz channel on the D M S P SSM/I (Special Sensor Microwave Imager instrument)). VIS and IR data are obtain able from both high-orbiting geostationary satellites ("GEOs") and low-orbiting Earth satellites ("LEOs"). The former are capable of providing very frequent information (every few minutes in some cases) from fixed positions in relation to the Earth, centred on the equator. Meanwhile, since the latter orbit the Earth many times a day, each of 6 E. C. Barrett these satellites is able to provide at best two good observations of any point on the surface during that period. For any particular application the frequency of coverage of the target, the spatial resolution of the data, and the type of spectral information provided, are all co-equally important. For rainfall monitoring, the physical charact eristics and behaviour of cloud particles (including raindrops), the structures and lifecycles of rain cells, and the nature and influence of local precipitation enhancement processes (e.g. convergence, and orography), are important too. Although most satellite rainfall monitoring to date has been based on "passive" remote sensing of the target, i.e. on the collection and measurement of radiation naturally reflected or emitted from the target, it is also possible to use "active" remote sensing for this application, i.e. in respect of radiation artificially generated and propagated towards the target. The first active microwave (AMW) system for rainfall assessment from satellites is the rainfall radar on the recently-launched joint Japanese/US Tropical Rainfall Measuring Mission (TRMM) satellite. This satellite is providing a substantial stimulus to satellite rainfall monitoring not only because of its rainfall radar, but because of the relative ease with which it is possible to intercompare and combine (co-located) data from its Precipitation Radar (PR), Passive Microwave (PMW) (TMI), VIS and ER (VIRS) imaging systems. Analytical approaches Since the early 1970s, much progress has been made with the development of analytical approaches to extract rainfall estimates from satellite and collateral data sets over most regions of the world. Increasingly these methods have become "multisource", and "mature": over the global oceans satellite-based rainfall estimation techniques are now the leading methods for rainfall measurements and monitoring; over land areas, as we shall see later, the challenges are more difficult and demanding. In general, satellite rainfall algorithms seek to: (a) Identify areas of probable precipitation, through recognition of the most likely rain/no-rain boundaries (sometimes referred to as "screening" for no-rain areas). (b) Evaluate associated rain rates (sometimes referred to as "rain rate conversion"). (c) Combine (a) and (b) through time where estimates of total accumulated rainfall are required. This is most reliable where the satellite data collection return period is shortest, i.e. from GEOs rather than from LEOs. Variations on these themes have seen satellite rainfall estimation and monitoring techniques developed for a wide range of applications, from the climatological, through meteorological monitoring, to short period, high-intensity rainstorm identi fication and prediction. In order to achieve reliable results, analyses are often made of the satellite data initially using surface (raingauge and/or radar) data for algorithm "calibration". Often the results will later be compared with independent sets of surface data for algorithm "validation" or "verification". We will go on to see that the object of present day research involves the blending of perhaps even several different types of data from both satellite and nonsatellite sources into a final "best possible" rainfall product. Such activity in respect to multiple-source algorithms is expected to increase further in the foreseeable future. Satellite remote sensing ofprecipitation: progress and problems 7 While three types of electromagnetic radiation have proved particularly valuable for such purposes, namely the visible (VIS), thermal infra-red (IR) and passive microwave (PMW), the Tropical Rainfall Measuring Mission (TRMM), launched in November 1997, carries for the first time an active microwave (AMW) instrument, whose data have been eagerly awaited by scientists interested especially in rainfall processes. In order to achieve best possible results, satellite rainfall estimates are often made in conjunction with surface (raingauge and/or radar) data, meteorological analyses, and increasingly with outputs from numerical weather prediction models (NWPs). Most of today's operational techniques routinely implemented by the Global Precipitation Climatology Centre at monthly, 2 A° lat./long. scales, are relatively simple, deploying fixed rain/no-rain IR temperature thresholds, and constant rain rates for all parts of the globe (Arkin et al., 1994). Others, e.g. the B4 technique (Barrett, 1993) applied to daily estimation over 25 km grid squares or smaller, are much more complicated, deploying spatially and temporally variable IR temperature thresholds and rain rates, related as closely as possible to local morphoclimatic influences, and seasonal weather cycles. Still others are even more complex and take account of very detailed cycles of cloud growth and development, particularly where severe storms are involved. Together, techniques are available to provide a range of results from long-term, broadarea statistics to small basin or even locally-specific statistics. Whilst most operational or quasi-operational techniques today are automatic (or objective), intervention by analysts is still necessary for some special applications, including severe storm monitoring and flash flood forecasting, e.g. the US Weather Service's Interactive Flash Flood Analysis (Scofield, 1987). In the past decade, much effort has also been put into the development of rainfall techniques based on P M W data. Whereas in the VIS/IR regions of the spectrum most rain-related information comes from cloud tops, microwave emissions or reflections received by the satellite emanate from hydrometeors within the clouds themselves. Below about 20 GHz evidence of rain is provided mainly by rainfall absorption/ emission processes, through which areas of active rainfall over water surfaces (e.g. oceans and seas) are warmer than the background radiation; above about 60 GHz evidence of rainfall comes predominately from scattering processes, whereby areas of heavy rainfall are much colder than their backgrounds; meanwhile between about 20 and 60 GHz some combinations of absorption/emission and scattering processes dominate in different situations. Whilst most existing P M W techniques are empirical in the sense that they seek to exploit observed relationships between P M W radiation characteristics and rainfall data from other sources (e.g. raingauge radar) it seems likely that best results may eventually be obtained by physical techniques, through which the observed P M W variations are interpreted in terms of detailed cloud models and understanding of related rainfall processes and patterns. l Application achievements Results of satellite precipitation monitoring operations can therefore be provided to the hydrological user community to meet a wide variety of different needs. Whilst the satellite may provide little additional information of a sufficiently reliable nature in 8 E. C. Barrett areas which are well monitored by more conventional means, satellite-derived estimates may be the only ones available for some types of hydrological activities over large areas of the globe. Increasing opportunities are arising for satellite precipitation estimates to be used for the following hydrometrical applications, amongst others: The incorporation of satellite-derived rainfall estimates into hydrological datasets. The generation of independent sets of precipitation estimates for comparison with existing data types. In support of both point-location and area-wide monitoring and modelling. The estimation and prediction of runoff and stream hydrographs. In these situations, satellites represent a still relatively under-exploited source of data of great potential value in hydrometry, especially in the developing world. However, even in the relatively developed world proper cognizance of the strengths and weaknesses of raingauges, radar and satellites would clearly bring many practical and financial benefits. P R O B L E M S IN SATELLITE R E M O T E SENSING O F P R E C I P I T A T I O N After three decades of research and growing operational use of satellite remote sensing data on precipitation it is clear that limitations on the quality and utility of such data remain, due to numerous factors, including the following: The temporal, spatial and spectral characteristics of the satellite observing systems—which are less than optimal for such a variable phenomena. The varied, and variable, interactions between electromagnetic radiation and its environment—particularly over land areas. The availability and suitability of collateral data for calibration and validation— which are still generally deteriorating. The provision of appropriate infra-structures, systems, personnel and policies to ensure optimum use of all relevant data sources, which are becoming more difficult to sustain as analytical approaches continue to become more complex and demanding. In view of the above, it is unsurprising that progress has been relatively poor in a number of areas, the most significant of which for overland hydrology relate to the following: Convergence of satellite-derived estimates with those from independent (in situ) sources: for example PEP-3 P M W estimates over the western equatorial Pacific and ground-based radar, which initially differed b y approximately a factor of two; and convergence between satellite estimates of different kinds, e.g. IR and P M W estimates over West Africa, which seem to show under-sampling effects from the latter even over unit periods of one month, and different algorithms applied to high-intensity rainfalls. Areas of signal ambiguity remain, e.g. from tropical cyclones in Central America; in respect of cold clouds in the IR which m a y or may not have enough depth to rain heavily; recognition and assessment of low intensity rains over dry, very dry, or frozen land surfaces which may give "false rain" signals in the P M W ; retrieval of "warm rain" by both IR and PMW; and effects of ice in the atmosphere and/or at the surface, which are difficult to discriminate in the P M W or A M W . Satellite remote sensing of precipitation: progress and problems - 9 H o w to calibrate satellite-only techniques in areas whence little or no reliable in situ data are forthcoming (e.g. Nigeria), and how best to combine data from different sources where they are (typically) fragmentary and incomplete. As time has progressed, it seems that local access to satellite data and abilities to use the same have gone full circle: in the early days of satellite meteorology (1960s to mid-1970s) reception facilities were rare, and competence in satellite rainfall retrieval limited to a few global centres; from the mid-1970s to the late 1980s both were more widespread; over the last decade key data have become unavailable to many users, and better techniques have grown more sophisticated and demanding. Thus, state-of-the-art use of satellite remote sensing of precipitation has become restricted, once again, to a relatively small number of centres, in the more developed countries where they can be government supported. FOCI F O R F U T U R E R E S E A R C H AND OPERATIONS Addressing problems of the types listed in the previous section will require concentrated effort, and significant resource expenditure if progress in this field is to be even maintained in relation to the last decade or two. Of paramount importance in research will be the refinement of procedures to retrieve precipitation estimates over drier and colder land surfaces, and from short-period, high-intensity storm situations. Since much precipitation is organized on meso- and local-scales, in operations more attention must be given to rainfall retrieval at space and time scales adequate for effective local use, whether in hydrology or weather and crop forecasting. In this regard, the Global Precipitation Mission (GPM) is promising, though probably still not adequate to give the coverage required. Both research and operations will be challenged particularly b y the overwhelming logic of "multi-sourcing" the solution to the general problem, within flexible systems simultaneously involving gauge and radar data, plus satellite data from different satellites and sensors, and both should be advanced by the development of the Internet, through which—given appropriate international initiatives and encouragement—outputs from advanced methods could be m a d e accessible to all would-be users, maybe preferably in some kind of "proto-results" form, which could then be calibrated better locally, say using datasets not usually disseminated (quickly) outside a particular country, authority or agency. Last but not least, better progress must be made with hydrometric design, to ensure that each available observation unit—whether surface-based or space-borne—can contribute optimally to the monitoring system as a whole. To achieve all this, more interchange is urgently needed between scientists, engineers, planners and politicians, plus the customers for rainfall and related data, and potential sponsors for schemes appropriate to less developed regions of the world and from which the potential benefits of improved rainfall data could be greatest. Perhaps the IAHS might accept the challenge this represents, e.g. through the organization of a colloquium designed to bring together such a wide range of parties with interest in, or responsibility for, the use of water. 10 E. C. Barrett REFERENCES Arkin, P. A. Joyce, R. & J a n o w i a k , J. E. (1994) T h e estimation of global m o n t h l y m e a n rainfall using infrared satellite data: the G O E S Precipitation Index (GPI). Remote Sens. Reviews 11, 619-628 Barrett, E. C. (1993) Satellite rainfall monitoring for agrometeorology: operational p r o b l e m s , practices and prospects. EARSeL Adv. Remote Sens. 2(2-VI), 6 6 - 7 2 . Barrett, E. C. & B e a u m o n t , M . J . (1994) Satellite rainfall monitoring: an o v e r v i e w . Remote Barrett, E. C. & Martin, D . W . (1981) The Use of Satellite Collier, C. G. (1989) Applications Data in Rainfall of Weather Radar Systems. Monitoring. Sens. Reviews 11, 23-48. A c a d e m i c Press, L o n d o n , U K . Ellis H o r w o o d , Chichester, U K . R a s m u s s o n , E. M. & Arkin, P. A. (1992) Observing tropical rainfall from space: a review. In: The Global Role of Tropical Rain (ed. by J. S. T h e o n ) , 1 0 5 - 1 1 8 . Hampton, Virginia, U S A . Scofield, R. A. (1987) T h e N E S D I S operational convective precipitation estimation t e c h n i q u e . Mon. Weath. Rev. 115, 1773-1792. T h e o n , J. S. (1992) T h e tropical rainfall measuring mission ( T R M M ) . In: The Global Role of Tropical Rain (ed. b y J. S. T h e o n ) , 2 0 2 - 2 2 2 . H a m p t o n , Virginia, U S A .