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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