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Physics Of Solar System Plasmas

Author: Thomas E. Cravens
Publisher: Cambridge University Press
ISBN: 9780521611947
Size: 42.36 MB
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A comprehensive introduction to the ionised gases of the solar-terrestrial environment.

Plasma Turbulence In The Solar System

Author: Yasuhito Narita
Publisher: Springer Science & Business Media
ISBN: 364225666X
Size: 69.75 MB
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Dynamics of astrophysical systems is often described by plasma physics, yet understanding the nature of plasma turbulence remains as a challenge. This book presents a summary and review of recent results in research on waves and turbulence in near-Earth space plasma turbulence, obtained by Cluster, the multi-spacecraft mission.

Solar System Magnetic Fields

Author: E.R. Priest
Publisher: Springer Science & Business Media
ISBN: 9400954824
Size: 18.87 MB
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In September 1984 a Summer School on Solar System Plasmas was held at Imperial College with the support of the Science and Engineering Research Council. An excellent group of lecturers was assembled to give a series of basic talks on the various aspects of the subject, aimed at Ph. D. students or researchers from related areas wanting to learn about the plasma physics of the solar system. The students were so appreciative of the lectures that it was decided to write them up as the present book. Traditionally, different areas of solar system science, such as solar and magnetospheric physics, have been studied by separate communities with little contact. However, it has become clear that many common themes cut right across these distinct topics, such as magnetohydrodynamic instabilities and waves, magnetic reconnect ion , convection, dynamo activity and particle acceleration. The plasma parameters may well be quite different in the Sun's atmosphere, a cometary tailor Jupiter's magnetosphere, but many of the basic processes are similar and it is by studying them in different environments that we come to understand them more deeply. Furthermore, direct in situ measurements of plasma properties at one point in the solar wind or the magnetosphere complement the more global view by remote sensing of a similar phenomenon at the Sun.