Session 17. Rings II

Contributed Oral Parallel Session, Tuesday, October 13, 1998, 10:30-11:30am, Madison Ballroom C

17.01 Radar Data Explanation via Superdiamagnetic Model of Saturn's Rings

S.V. Girich (Radiophysics Dept. of Volgograd State Univercity, Russia), A.Yu. Pospelov (General Physics Institute, Russian Academy of Science), V.V. Tchernyi (Moskow State Institute of Electronics and Mathematics, LMIS), CITO MVD Collaboration, GPI RAS Team, MSIEM LMIS Team

17.02 Wavelike Features in Saturn's Cassini Division

L. J. Spilker (formerly Horn) (JPL/Caltech), M. R. Showalter (Stanford)

17.03 Particle Sizes in Saturn's Rings Derived from Stellar Occultation Data.

P. D. Nicholson (Cornell), R. G. French (Wellesley College)

17.04 About the optical depth profile of Saturns E ring

F. Spahn, K. -U. Thiessenhusen, J. Schmidt (University Potsdam, Germany)

17.05 Saturn's ``Gossamer'' Ring: The F Ring's Inner Sheet

M. R. Showalter (Stanford), J. A. Burns (Cornell), D. P. Hamilton (U. Maryland)

17.06 First Infrared Imaging of the Neptune Ring Arcs: HST/Nicmos Results

R. J. Terrile, C. Dumas (JPL), B. A. Smith (Univ. Hawaii), M. Rieke, G. Schneider, R. Thompson (Univ. Arizona), E. Becklin (UCLA), D. Koerner (Univ. Pennsylvania)