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 30. Io Posters
Displayed, 1:00pm, Monday - 1:00pm, Friday,
Highlighted Thursday, 3:30-6:30pm, C101-C105, C211
- 30.01 Photometric Mapping of Io
- P.E. Geissler, A.S. McEwen (University of Arizona), C. Phillips (SETI Institute), D.P. Simonelli (Cornell University), R. Lopes-Gautier (J.P.L.), S. Douté (U.C.L.A.)
- 30.02 Regolith Variations on Io: Implications for Bolometric Albedos
- D.P. Simonelli, C. Dodd, J. Veverka (Cornell U.), Galileo SSI Team
- 30.03 Infrared Spectral Signatures For Io's Dark Spots
- J.C. Granahan, J. Sweet (BAE SYSTEMS), F.P. Fanale (University of Hawaii), R.W. Carlson, W.D. Smythe (Jet Propulsion Laboratory), Galileo NIMS Team, Galileo SSI Team
- 30.04 The Thermal State of Io's Interior
- W. B. Moore, G. Schubert (Dept. of Earth and Space Sciences, UCLA)
- 30.05 Actual and future monitoring of Io's hot spots by used of Adaptive Optics systems
- F. Marchis (ESO), R. Prange (IAS), T. Fusco (ONERA)
- 30.06 Reflectance Spectra of Impure Sulfur: Io and New Lab Results
- T. MacIntyre (Northern Arizona University), J.S. Kargel, B. Dalton, R. Clark (U.S. Geological Survey)
- 30.07 Are Prometheus-Type Plumes on Io Produced by Lava-SO2 Interactions at the Flow Fronts?
- M. P. Milazzo, L. P. Keszthelyi, A. S. McEwen (University of Arizona), Galileo SSI Team
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