Collective plasma effects associated with the continuous injection model of solar flare particle streams

Details Collective plasma effects associated with the continuous injection model of solar flare particle streams Collective plasma effects associated with the continuous injection model of solar flare particle streams

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...233..717v&link_type=abstract

Astrophysical Journal, Part 1, vol. 233, Oct. 15, 1979, p. 717-726. Navy-supported research;

Astronomy and Astrophysics

Astrophysics

56

Magnetohydrodynamics, Solar Corona, Solar Flares, Electron Beams, Electron Energy, Mathematical Models, Maxwell-Boltzmann Density Function, Velocity Distribution

Scientific paper

A modified continuous injection model for impulsive solar flares that includes self-consistent plasma nonlinearities based on the concept of marginal stability is presented. A quasi-stationary state is established, composed of a hot truncated electron Maxwellian distribution confined by acoustic turbulence on the top of the loop and energetic electron beams precipitating in the chromosphere. It is shown that the radiation properties of the model are in accordance with observations.

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