Planetary magnetospheric physics II : proceedings of Symposium 5, and the Topical Meetings of the COSPAR Interdisciplinary Scientific Commission B (Meetings B1 and B6) of the COSPAR Twenty-eighth Plenary Meeting held in The Haque, The Netherlands, 25 June - 6 July 1990

Bibliographic Information

Planetary magnetospheric physics II : proceedings of Symposium 5, and the Topical Meetings of the COSPAR Interdisciplinary Scientific Commission B (Meetings B1 and B6) of the COSPAR Twenty-eighth Plenary Meeting held in The Haque, The Netherlands, 25 June - 6 July 1990

edited by M.G. Kivelson (Symp. 5), S.K. Runcorn (Mtg B1), N.F. Ness (Mtg B1) and W.-H. Ip (Mtg B6)

(Advances in space research, vol. 12, no. 8)

Published for the Committee on Space Research by Pergamon Press, 1992

Available at  / 3 libraries

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Includes bibliographies and index

Description and Table of Contents

Description

Magnetospheres of the Outer Planets, the first chapter in this volume, presents an overview of comparative magnetospheres with an emphasis on basic processes that are common to all planets but that vary in importance among the bodies of the solar system because of the different parameter regimes that they represent. The Magnetic Fields of the Planets and Other Bodies covers topical theories in connection with the magnetic fields. From 1600 to the middle of this century, only one planet was known to have a magnetic field. It is now known that all the terrestrial planets have iron cores. The major planets, Jupiter and Saturn have metallic hydrogen cores and Uranus and Neptune shells, outside Earth-like cores, of an electrolyte-ammonia and water. The Moon is now widely accepted as having an iron core of 500km in radius. Energy Transfer Processes in Planetary Exospheres and Extended Neutral Clouds provides papers covering interesting results from past observations of the plasma-neutral interaction effects but also acts as a forerunner for the exciting developments in the field of space plasma physics and the missions of Giotto, Ulysses, Galileo and Casini in future years.

Table of Contents

  • Chapter headings and selected sections and papers: Magnetospheres of the Outer Planets. Sources, transport and acceleration of energetic particles. Heavy ion dynamics and auroral arc formation in the Jovian Magnetosphere, D D Barbosa. Magnetic boundaries, magnetospheric structure, and MHD disturbances. ULF waves in the outer magnetosphere of Uranus, C T Russell & R P Leppi
  • g. Transport of plasma: sources, convection and rotation. Phase space densities in the Uranian plasma sheet, C M Hammond et al . Plasma wave and radio emission: observations and interpretations. Comparative observations of plasma waves at the outer planets, W S Kurth. Uranus smooth low frequency emission, G K F Rabl et al . Time variability. Variability in the outer planet aurorae, J T Clarke. The Magnetic Fields of the Planets and Other Bodies of the Solar System. Radio observations of the Jovian magnetic field, C H Barrow & T D Carr.
  • Palaeomagnetism in the solar system, D W Collinson. A new scaling law of the planetary magnetic fields, H Mizutani et al . Energy Transfer Processes in Planetary Exospheres and Extended Neutral Clouds. Mars, Venus and comets. Solitary vortex type motions of the mass loaded magnetized plasma flow, A A Galeev et al . Bulk parameters of water group ions at comet Giacobini-Zinner, K Staines et al . The Jovian and Saturnian system. Neutral cloud distribution in the Jovian system, W H Smyth. UV, IR and radio-wave remote-sensing of solar system plasmas. The UV and IR Jovian aurorae, R Prange. Author Index.

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Details

  • NCID
    BA1409560X
  • ISBN
    • 0080418546
  • Country Code
    uk
  • Title Language Code
    eng
  • Text Language Code
    eng
  • Place of Publication
    Oxford
  • Pages/Volumes
    viii, 406 p.
  • Size
    28 cm
  • Parent Bibliography ID
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