Non-stationary heating of solar flare plasma by non-thermal electrons

Details Non-stationary heating of solar flare plasma by non-thermal electrons Non-stationary heating of solar flare plasma by non-thermal electrons

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..347g&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 3, Dec. 1976, p. 347-354.

Astronomy and Astrophysics

Astrophysics

6

Electron Energy, Kinetic Heating, Plasma Heating, Solar Flares, Solar X-Rays, Absorption Spectra, Energy Transfer, Green'S Functions, Particle Acceleration, Particle Collisions, Plasma Density, Radiant Flux Density, Solar Heating, Thermal Conductivity

Scientific paper

A general solution of the energy-transfer equation for nonthermal particles in an absorbing medium at constant density is obtained by the Green's function method. The derived particle distributions are used to compute the collisional heating of the high-temperature region of solar flares. The space and time dependence of the energy deposition is determined for a variety of nonthermal-particle sources. The results are discussed on the basis of presently available flare observations, and suggestions are given for the use of the computed energy-deposition functions in the investigation of flare models.

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