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 18. Titan Posters
Displayed, 1:00pm, Monday - 1:00pm, Friday,
Highlighted Tuesday, 3:30-6:30pm, C101-C105, C211
- 18.01 Adaptive Optics Observations of Titan from the W.M. Keck Telescope
- S.G. Gibbard, B. Macintosh, C.E. Max (Lawrence Livermore National Lab), H. Roe, I. de Pater (University of California, Berkeley), E.F. Young (Southwest Research Institute, Boulder), C.P. McKay (NASA Ames)
- 18.02 High Spectral Resolution Imaging of Titan
- N. J. Chanover (New Mexico State University), D. A. Glenar (NASA/Goddard Space Flight Center)
- 18.03 On the Abundance of Ethane in Titan's Stratosphere
- T. A. Livengood, J. J. Goldstein (Challenger Ctr.), T. Hewagama, K. E. Fast (U of MD), Th. Kostiuk, F. Espenak, D. Buhl (NASA's GSFC)
- 18.04 Simulation of Titan Haze Formation Using a Photochemical Flow Reactor. Optical Constants of the Simulated Haze
- B. N. Tran, J. C. Joseph, J. P. Ferris (Renssealaer Polytechnic Institute)
- 18.05 Seasonality and differential mixing of trace species by waves in Titan's stratosphere
- D. Luz (Observatório Astronómico de Lisboa, Portugal), F. Hourdin (Laboratoire de Météorologie Dynamique du CNRS, Paris)
- 18.06 Titan's Seasonal Photochemistry - A Two-dimensional Model
- J. R. Dire (U.S. Coast Guard Academy)
- 18.07 O+ bombardment of an O and O2 Thermosphere
- M. McKeown, R.E. Johnson (University of Virginia)
- 18.08 Basic Physical Properties of Ammonia-Rich Ice
- S. E. Shandera, R. D. Lorenz (Lunar and Planetary Lab, University of Arizona)
- 18.09 Saturnian satellite chemistry: Titan as polluter of the Saturn system
- M.L. Delitsky, A.L. Lane (Jet Propulsion Laboratory)
- 18.10 A Turbulent model of the Saturn subnebula: Implications for the origin of methane in Titan's atmosphere
- O. Mousis (Obs. Paris, University of Nantes), D. Gautier (Obs. Paris), D. Bockelée-Morvan (Obs. Paris), B. Dubrulle (CEA Saclay), F. Hersant (Obs. Paris and CEA Saclay)
- 18.11 Observing Titan's Surface by Bistatic-Scattering: Cassini's Potential
- E. Marouf (San Jose State University), R. French (Wellesely College), N. Rappaport, A. Kliore (JPL)
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