Planetary magnetospheric physics II; Proceedings of Symposium 5 and the Topical Meetings of the Interdisciplinary Scientific Commission B (Meetings B1 and B6) of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990

Details Planetary magnetospheric physics II; Proceedings of Symposium 5 and the Topical Meetings of the Interdisciplinary Scientific Commission B (Meetings B1 and B6) of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990 Planetary magnetospheric physics II; Proceedings of Symposium 5 and the Topical Meetings of the Interdisciplinary Scientific Commission B (Meetings B1 and B6) of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992adspr..12.....k&link_type=abstract

Symposium and Meetings sponsored by COSPAR, IAU, and IAGA. Advances in Space Research (ISSN 0273-1177), vol. 12, no. 8, Aug. 199

Physics

Atmospheric Physics, Conferences, Planetary Magnetospheres, Comets, Energy Transfer, Exosphere, Gas Giant Planets, Magnetospheric Instability, Mars Atmosphere, Neutral Gases, Particle Acceleration, Planetary Magnetic Fields, Plasma Dynamics, Plasma Waves, Solar Planetary Interactions, Space Plasmas, Transport Properties, Venus Atmosphere

Scientific paper

The present conference on planetary magnetospheric physics encompasses magnetospheres of the outer planets, the magnetic fields of planets and other bodies of the solar system, and energy-transfer processes in planetary exospheres and extended neutral clouds. Specific areas addressed include the sources, transport, and acceleration of energetic particles, magnetic boundaries and MHD disturbances, the transport of plasma, plasma-wave and radio emission, and time variability. Also addressed are radio observations of the Jovian magnetic field, the question of a Martian planetary magnetic field, dynamo theory, energy transfer in Mars, Venus, and comets, remote sensing of solar system plasmas by means of UV and IR wavelengths, observations of Io's sodium cloud and torus, and plasma-neutral interactions in the magnetosphere of Saturn.

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