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Beam-return current systems in nonthermal solar flare models (1989)

Larosa, T. N. ; Emslie, A. Gordon

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Publication Date: 2019-07-12

Description: It is shown here that the generation of return current in large-scale astrophysical plasmas such as solar flares is quite different from the laboratory environment. Whereas in the laboratory the return current is established inductively and subsequently decays on a resistive timescale, the return current in a solar flare is established electrostatically and therefore does not decay. An explanation of the difference is given in terms of the characteristics of the laboratory circuit.

Keywords: SOLAR PHYSICS

Type: Solar Physics (ISSN 0038-0938); 120; 2 19

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