Beam heating in solar flares - Electrons or protons?

Details Beam heating in solar flares - Electrons or protons? Beam heating in solar flares - Electrons or protons?

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..343b&link_type=abstract

(NASA and University of New Hampshire, Workshop on Impulsive Solar Flares, 2nd, Durham, NH, Sept. 26-28, 1988) Astrophysical Jou

Astronomy and Astrophysics

Astrophysics

29

Electron Beams, Proton Beams, Solar Flares, Solar Heating, Electrostatic Waves, Gamma Rays, Solar Atmosphere, Solar X-Rays, Spatial Distribution

Scientific paper

The current status of electron and proton beam models as candidates for the impulsive phase heating of solar flares is discussed in relation to observational constants and theoretical difficulties. It is concluded that, while the electron beam model for flare heating still faces theoretical and observational problems, the problems faced by low and high energy proton beam models are no less serious, and there are facets of proton models which have not yet been studied. At the present, the electron beam model remains the most viable and best developed of heating model candidates.

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