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Study Guide
... What would the sun look like for a total solar eclipse, partial solar eclipse, and annular solar eclipse? ...
... What would the sun look like for a total solar eclipse, partial solar eclipse, and annular solar eclipse? ...
July 23 2004 - RASC – Mississauga Centre
... Brian Gibson’s showed “The Sky for Pocket PC”, a portable software program with a 64 meg flashcard showing 250,000 stars and an ability to plug into a telescope. Betty Robinson’s the copy editor of “Observer’s Handbook” described this venerable publication with its wealth of astronomical informatio ...
... Brian Gibson’s showed “The Sky for Pocket PC”, a portable software program with a 64 meg flashcard showing 250,000 stars and an ability to plug into a telescope. Betty Robinson’s the copy editor of “Observer’s Handbook” described this venerable publication with its wealth of astronomical informatio ...
ALLAN SACHA BRUN Head of the Laboratory on Dynamics
... - PI of European Research Council Grant STARS2 (www.stars2.eu) for 5 yr on stellar dynamics and magnetism - Co-I of ANR (French funding agency) Grant TOUPIES on rotational history of stars - Co-I of IDEX Paris-Saclay VKSstar project on dynamo studies in VKS2 experiment and stars - Member of Scientif ...
... - PI of European Research Council Grant STARS2 (www.stars2.eu) for 5 yr on stellar dynamics and magnetism - Co-I of ANR (French funding agency) Grant TOUPIES on rotational history of stars - Co-I of IDEX Paris-Saclay VKSstar project on dynamo studies in VKS2 experiment and stars - Member of Scientif ...
May - RASC Hamilton
... and despite the clouds, I had a good view of the entire eclipse. I was also supposed to go on the 1984 trip to the Carolinas for the hybrid eclipse, but the departure time was pushed forward by 24 hours, and it meant I would not be able to celebrate my first wedding anniversary. I chose my bride ove ...
... and despite the clouds, I had a good view of the entire eclipse. I was also supposed to go on the 1984 trip to the Carolinas for the hybrid eclipse, but the departure time was pushed forward by 24 hours, and it meant I would not be able to celebrate my first wedding anniversary. I chose my bride ove ...
Job Description - St Andrews Vacancies
... collaborate on interrelated topics of mutual interest. Professor Ian Bonnell and Dr Vivienne Wild have been awarded major ERC grants in star formation and galaxy evolution respectively, while Professor Keith Horne has been awarded a Leverhulme Fellowship in support of his microlensing searches for c ...
... collaborate on interrelated topics of mutual interest. Professor Ian Bonnell and Dr Vivienne Wild have been awarded major ERC grants in star formation and galaxy evolution respectively, while Professor Keith Horne has been awarded a Leverhulme Fellowship in support of his microlensing searches for c ...
Take time to understand it now
... Galactic open clusters are laboratories, provided by nature, for us to study stellar evolution. Using 1m-, 4m- and 8m-class telescopes, I will show how spectroscopic and photometric observations of solar-type stars in open clusters allow us to establish a stellar chronometer, and create an age-ranki ...
... Galactic open clusters are laboratories, provided by nature, for us to study stellar evolution. Using 1m-, 4m- and 8m-class telescopes, I will show how spectroscopic and photometric observations of solar-type stars in open clusters allow us to establish a stellar chronometer, and create an age-ranki ...
WOMEN-ASTRONOMERS OF FORMER USSR L.V. RYKHLOVA
... Tamara Ruzmaikina (1945) works in the field of cosmology and origin of the solar system, molecular astrophysics and star formation. This list of outstanding women-astronomers in the former USSR and the present Russia is far from being complete. We have included only those women who have achieved the ...
... Tamara Ruzmaikina (1945) works in the field of cosmology and origin of the solar system, molecular astrophysics and star formation. This list of outstanding women-astronomers in the former USSR and the present Russia is far from being complete. We have included only those women who have achieved the ...
talk
... Discover significant patterns from the analysis of statistically rich and unbiased image/catalog databases Understand complex astrophysical systems via confrontation between data and sophisticated numerical simulation ...
... Discover significant patterns from the analysis of statistically rich and unbiased image/catalog databases Understand complex astrophysical systems via confrontation between data and sophisticated numerical simulation ...
“A wide-field astronomer in King Malcolm’s court” or
... R5. A mechanism should be sought whereby the peer-reviewed publication of datasets can be made part of the standard scientific process. R8. A set of tutorials should be created and maintained, for introducing application scientists to new key concepts in e-science. ...
... R5. A mechanism should be sought whereby the peer-reviewed publication of datasets can be made part of the standard scientific process. R8. A set of tutorials should be created and maintained, for introducing application scientists to new key concepts in e-science. ...
How can you get involved in research?
... “Arcs” of light from background galaxies bent by the gravitational mass of the galaxy cluster in the foreground. This is evidence for ...
... “Arcs” of light from background galaxies bent by the gravitational mass of the galaxy cluster in the foreground. This is evidence for ...
Asteroseismology with the Whole Earth Telescope
... Aperture Photometry Monitor variable star Monitor “comparison” stars ...
... Aperture Photometry Monitor variable star Monitor “comparison” stars ...
HEIC0619: EMBARGOED UNTIL: 19:30 (CET)/01:30 PM EST 11
... or maybe even more – tend to be born in multiple systems that can easily disguise themselves as single very heavy stars. Moreover, these stellar heavyweights are so rare that only a few are close enough to the Sun to be examined in detail. One of the top candidates for the title of “Milky Way stella ...
... or maybe even more – tend to be born in multiple systems that can easily disguise themselves as single very heavy stars. Moreover, these stellar heavyweights are so rare that only a few are close enough to the Sun to be examined in detail. One of the top candidates for the title of “Milky Way stella ...
DUST FROM EVOLVED STARS TO PROTOSTARS. A. K. Speck
... molecules [e.g. 5]. Furthermore, dust has been observed at higher redshifts than expected, and understanding this phenomenon is vital to our understanding of the cosmos at large and its evolution [e.g. 6, 7].Such a crucial and ubiquitous constituent of our Universe needs to be well understood in its ...
... molecules [e.g. 5]. Furthermore, dust has been observed at higher redshifts than expected, and understanding this phenomenon is vital to our understanding of the cosmos at large and its evolution [e.g. 6, 7].Such a crucial and ubiquitous constituent of our Universe needs to be well understood in its ...
Remote Observatory Atacama Desert
... and started a time series at August 2.844 UT, just 1.34 hours after the initial discovery. A first analysis of the data of G. Masi by the Kyoto team (Ohshima et al. 2011) showed that the star is probably an SU UMa type dwarf nova with a superhump period of about 1.54 hours. The present outburst seem ...
... and started a time series at August 2.844 UT, just 1.34 hours after the initial discovery. A first analysis of the data of G. Masi by the Kyoto team (Ohshima et al. 2011) showed that the star is probably an SU UMa type dwarf nova with a superhump period of about 1.54 hours. The present outburst seem ...
Introduction to Astronomy Lab
... measuring stellar magnitudes, spectral lines, motions of the sun, moon and planets. Prerequisite/Corequisite: Astronomy 1, 10, or 20. 3 hours laboratory. [Typical contact hours: 52.5] Prerequisite Skills: None Expected Outcomes for Students: Upon completion of the course, the student should be able ...
... measuring stellar magnitudes, spectral lines, motions of the sun, moon and planets. Prerequisite/Corequisite: Astronomy 1, 10, or 20. 3 hours laboratory. [Typical contact hours: 52.5] Prerequisite Skills: None Expected Outcomes for Students: Upon completion of the course, the student should be able ...
05 Feb: The "Nature of Things" in the Solar System
... • The obliquity is 23.5 degrees, and changes over time by about +/- 1.5 degrees • This is a mild variation, and allows moderate, but not extreme seasonal variations. • It is conjectured that this modest variation is a consequence of the Earth having a relatively large moon, which may be a low-probab ...
... • The obliquity is 23.5 degrees, and changes over time by about +/- 1.5 degrees • This is a mild variation, and allows moderate, but not extreme seasonal variations. • It is conjectured that this modest variation is a consequence of the Earth having a relatively large moon, which may be a low-probab ...
PPT file
... More 25 years of H2O space masers monitoring at 22 GHz in PRAO. It’s the most long set observations. 125 sources are in the modern list for observation once in the month. Here two type sources: super compact (~1au) gaze clouds in star formation regions and envelopes of variable late spectra classes ...
... More 25 years of H2O space masers monitoring at 22 GHz in PRAO. It’s the most long set observations. 125 sources are in the modern list for observation once in the month. Here two type sources: super compact (~1au) gaze clouds in star formation regions and envelopes of variable late spectra classes ...
Session 1: Structure and dynamics of the solar chromosphere
... chromosphere (cell interior, network, spicules etc.) as well as other features seen at the chromospheric level or having the properties of plasmas at chromospheric temperatures: sunspots chromosphere, plages, chromospheric flares, filaments etc. The relation of such plasmas to other atmospheric laye ...
... chromosphere (cell interior, network, spicules etc.) as well as other features seen at the chromospheric level or having the properties of plasmas at chromospheric temperatures: sunspots chromosphere, plages, chromospheric flares, filaments etc. The relation of such plasmas to other atmospheric laye ...
Gravity Simulation - National Schools` Observatory
... •Open up a web browser containing the NSO Gravity Simulator. •To carry out the experiment you will also need a stopwatch. ...
... •Open up a web browser containing the NSO Gravity Simulator. •To carry out the experiment you will also need a stopwatch. ...
The sodium D-lines Why and What are D
... The Fraunhofer lines are a set of spectral lines named for the German physicist Joseph von Fraunhofer (1787– 1826). The lines were originally observed as dark features (absorption lines) in the optical spectrum of the Sun. He labeled the lines with letters from A to K. ...
... The Fraunhofer lines are a set of spectral lines named for the German physicist Joseph von Fraunhofer (1787– 1826). The lines were originally observed as dark features (absorption lines) in the optical spectrum of the Sun. He labeled the lines with letters from A to K. ...
Lots of free resources!
... Karen Sorensen, Portland Community College Presentation at Quality Matters 2016 Conference ...
... Karen Sorensen, Portland Community College Presentation at Quality Matters 2016 Conference ...
Viktor Ambartsumian International Prize 2014 goes to Felix
... Institute. After the Ph.D. degree received from the same institute in 1979, he joined Yerevan Physics Institute, where he conducted his research until 1991. In 1987, he received a degree of Doctor of Sciences. In 1991-1992 he was invited to the University of Chicago, USA, as a visiting researcher. I ...
... Institute. After the Ph.D. degree received from the same institute in 1979, he joined Yerevan Physics Institute, where he conducted his research until 1991. In 1987, he received a degree of Doctor of Sciences. In 1991-1992 he was invited to the University of Chicago, USA, as a visiting researcher. I ...
Indian Institute of Astrophysics
![](https://en.wikipedia.org/wiki/Special:FilePath/IIA_logo.png?width=300)
The Indian Institute of Astrophysics (IIA), with its headquarters in Bangalore (Karnataka state), India, is a premier national institute of India for the study of and research into topics pertaining to astronomy, astrophysics and related subjects.The Institute has a network of laboratories and observatories located in various places in India, including Kodaikanal (the Kodaikanal Solar Observatory), Kavalur (the Vainu Bappu Observatory), Gauribidanur, Hanle (the Indian Astronomical Observatory) and Hosakote.