Beam-return current systems in nonthermal solar flare models

Details Beam-return current systems in nonthermal solar flare models Beam-return current systems in nonthermal solar flare models

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..343l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 343-349.

Physics

12

Beam Currents, Solar Flares, Electron Beams, Electrostatics, Magnetic Fields

Scientific paper

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.

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