DPS Pasadena Meeting 2000, 23-27 October 2000
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All findings are embargoed until the time of presentation at the
meeting.
Session 64. Venus Posters
Displayed, 1:00pm, Monday - 1:00pm, Friday,
Highlighted Thursday, 3:30-6:30pm, C101-C105, C211
- 64.01 Venus's airglow as observed by the Cassini Ultraviolet Imaging Spectrometer
- A.I.F. Stewart, L.W. Esposito, W.R. Pryor (LASP, Univ. of Colorado at Boulder), J.L. Fox (Physics Dept, Wright State Univ., Dayton, Ohio), UVIS Team
- 64.02 The terms ``Arachnoids" and ``Novae" are valid in the Venusian context.
- V-P. Kostama, M. Aittola, J. Raitala (University of Oulu)
- 64.03 Cloud Top Water Vapour Abundance on Venus
- M. E. Koukouli, P. G. J. Irwin, F. W. Taylor (Atmospheric, Oceanic and Planetary Physics, Oxford University)
- 64.04 The Solar and Thermal Radiation Field Below the Venus Clouds
- D. Crisp (Jet Propulsion Laboratory, California Institute of Technology)
- 64.05 High precision Wind measurements in the upper Venus atmosphere
- F. Schmuelling (NRC at NASA/GSFC), J. Goldstein (CCSSE), T. Kostiuk (GSFC), T. Hewagama (UMD/GSFC), D. Zipoy (UMD)
- 64.06 High Resolution 3D Simulations of the Impacts of Asteroids into the Venusian Atmosphere
- D. G. Korycansky, K. J. Zahnle, M.-M. Mac Low (AAS)
- 64.07 The 3 Final States of Venus
- A.C.M. Correia, J. Laskar (ASD/IMC-CNRS)
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