xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)
xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)
xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)
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IAGA NEWS N0.29<br />
GAM4 . 9 Comets<br />
Konrad Schwingenschuh, Space Research Institute,<br />
Austrian Academy of Sciences, Inffeldgasse 12, A-8010<br />
Graz, <strong>AUSTRIA</strong>.<br />
Tatsuki Ogino<br />
A P Remizov<br />
The main objective will be to discuss new results about the<br />
solar wind interaction with ·comets, cometary dust and neutral<br />
gas environments, and comparisons between comets and other<br />
outgassing solar system bodies. Papers will describe<br />
investigations using the results of in situ or Earth-based<br />
observations, computer simulations or theoretical conclusions.<br />
GAM4 .10 The Interplanetary Magnetic Field: Observations and<br />
Models<br />
I S Veselovsky, Institute of Nuclear Physics, Moscow<br />
State University, Moscow 119899, USSR.<br />
N U Crooker<br />
T Saito<br />
The following topics will be covered: 3D time-dependent and<br />
averaged IMF; Heliospheric current sheet structure; Largescale<br />
magnetic fields. Observational and theoretical papers<br />
will be welcome.<br />
GAM4. 11 From the Bow Shock to the Magnetopause: the<br />
Magnetos heath<br />
David G Sibeck, Applied Physics Laboratory, The Johns<br />
Hopkins University, Johns Hopkins Road, Laurel MD<br />
20707-6099, USA.<br />
Mark A Saunders<br />
Stephen A Fuselier<br />
Oleg L Vaisberg<br />
Consideration will be given to case studies and statistical<br />
observational studies of transient events and the steady state<br />
magnetosheath structure in the context of new and existing<br />
magnetosheath models. Bow shock and magnetopause studies with<br />
emphasis upon t he magnetosheath are also invited.<br />
GAM4.12 The Microphysics of Shocks and Other Discontinuities<br />
Michelle F Thomsen, Los Alamos National Laboratory,<br />
Mail Stop D438, Los Alamos NM 87545, USA.<br />
Steven J Schwartz<br />
V G Es e levich<br />
Stephen H Brecht<br />
Transitions in plasmas are in r ealit y ne ve r discontinuous but<br />
occ ur t hrough finite spatial scalele ngths. Properties like<br />
transport and dissipation depe nd crucia lly upon the<br />
microphysics of the transition . Rece nt research on the shocks,<br />
tange ntial discontinuities, contact discontinuities etc. will<br />
be t he focus of this symposium.<br />
34