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Escaping near-relativistic electron beams from the solar corona

โœ Scribed by D.K. Haggerty; E.C. Roelof; G.M. Simnett


Book ID
108426794
Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
576 KB
Volume
32
Category
Article
ISSN
0273-1177

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โœ K. G. McClements ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 432 KB

The conditions required for the stability of a steady-state electron beam propagating in the solar corona are determined using the quasi-linear theory. The growth rate for electron plasma waves in a magnetized plasma is evaluated, with the electron distribution function being given by an analytic so