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Role of Magnetospheric Plasma Physics for Understanding Cosmic Phenomena

Published online by Cambridge University Press:  12 April 2016

Indra Mohan Lal Das
Indra Mohan Lal Das*
Affiliation:
Department of Physics, university of Allahabad, Allahabad-211 002, India

Abstract

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Cosmic phenomena occur in the remote regions of space where in-situ observations are not possible. For proper understanding of these phenomena laboratory experiments are essential, but the in-situ observations of magnetospheric plasma provides even a better background to test various hypothesis of cosmic interest. This is because the ionospheric-magnetospheric plasma and the solar wind are the only cosmic plasmas accessible to extensive in-situ observations and experiments.

Type
2. Magnetic Effects
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 90 - 93
Copyright
Copyright © Cambridge University Press 1990

References

References:

Alfven, H. (1981); Cosmic Plasma, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Falthammer, C-G. (1978); J. Geomag. Geoelectr., 30, 419.Google Scholar
Kennel, C.F. (1975); Comments on Astrophys. Space Sci. 6, 71.Google Scholar
Lehnert, B. (1977); Astrophys. Space Sci., 53, 459.Google Scholar
Spangler, S.R. and Moffett, T.J. (1976); Ap.J., 205, 479.CrossRefGoogle Scholar
Sturrock, P.A. (1971); Ap.J., 164, 529.Google Scholar