Gamma-ray continuum and millimeter wave emissions from solar flares.

Details Gamma-ray continuum and millimeter wave emissions from solar flares. Gamma-ray continuum and millimeter wave emissions from solar flares.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cphe.conf...15r&link_type=abstract

Current perspectives in high energy astropyhsics, p. 15 - 21

Astronomy and Astrophysics

Astronomy

Solar Flares: Gamma Rays, Solar Flares: Synchrotron Radiation, Solar Flares: Mm Radiation

Scientific paper

The author presents a theoretical discussion on the methods for correlating gamma-ray continuum and millimeter wave emissions from solar flares. Both of these emissions are produced by electrons of similar energies, typically around 1 MeV, interacting in the solar atmosphere. The gamma-rays are bremsstrahlung and the millimeter waves are gyrosynchrotron radiation. Thin and thick target interaction and radiation models for the accelerated particles are presented. The comparison of the models with observations of gamma-rays and 80 GHz radio emission from the 4 June 1991 flare provides information on a variety of parameters, including the magnetic field in the corona and the variation of the accelerated electron spectrum during the course of the flare.

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