[PDF.73ts] Convection and Substorms: Paradigms of Magnetospheric Phenomenology (International Series on Astronomy and Astrophysics)

Convection and Substorms: Paradigms of Magnetospheric Phenomenology (International Series on Astronomy and Astrophysics)

[PDF.el39] Convection and Substorms: Paradigms of Magnetospheric Phenomenology (International Series on Astronomy and Astrophysics)

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 | #4799586 in Books |  Charles F Kennel |  1996-02-08 | Original language:English | PDF # 1 |  9.50 x1.32 x6.40l,1.92 | File type: PDF | 432 pages

 | Convection and Substorms Paradigms of Magnetospheric Phenomenology

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The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for ...

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