The electrodynamics of beam/return current systems in the solar corona

Details The electrodynamics of beam/return current systems in the solar corona The electrodynamics of beam/return current systems in the solar corona

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..496v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 496-518. Research supported by EEC.

Astronomy and Astrophysics

Astrophysics

60

Electrodynamics, Electron Beams, Solar Corona, Solar Flares, Solar X-Rays, Space Plasmas, Beam Currents, Ohms Law

Scientific paper

The response of a uniform plasma to the propagation of a prescribed electron beam in the approximation of decoupled solenoidal and irrotational fields is studied. It is shown that the electrostatic and inductive response of a plasma are governed by two independent sets of equations and that both are important for the current neutralization process. It is also found that the electrostatic response accounts for neutralization of the irrotational part of the beam current while the inductive response leads to neutralization of the solenoidal part of the beam current.

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