Effect of electron beams during solar flares

Details Effect of electron beams during solar flares Effect of electron beams during solar flares

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..243a&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Physics

8

Electron Beams, Hydrogen Recombinations, Opacity, Solar Atmosphere, Solar Flares, Flare Stars, Radiation Absorption, Solar Flux, Stellar Flares

Scientific paper

Electron bombardment of the solar atmosphere has two effects: one is to enhance hydrogen recombination emission, the other is to increase the opacity via an increase of H(-) population. The first effect is the most important in the upper part of the atmosphere, and the second in the lower part. It is predicted that, when enhanced absorption dominates in the part of the atmosphere where radiation originates, there will be a decrease in the white-light emission, leading to a 'negative flare', or 'black-light flare' short duration, not more than about 20 sec.

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