Microwave & hard X-ray emission during solar flare of 19 Oct. 1981

Details Microwave & hard X-ray emission during solar flare of 19 Oct. 1981 Microwave & hard X-ray emission during solar flare of 19 Oct. 1981

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ijrsp..13..159v&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 13, Oct. 1984, p. 159-163.

Physics

Space Physics

1

Electron Energy, H Alpha Line, Microwave Emission, Solar Flares, Solar X-Rays, Temporal Distribution, Correlation Coefficients, Kinetic Energy, Magnetic Flux, Photons, Spectrum Analysis, Stellar Spectrophotometry

Scientific paper

Time correlation study of a double ribbon flare, observed on Oct. 19, 1981, in the light of H-alpha, microwave, and hard X-ray data is presented. The kinetic energy of electrons required to emit hard X-rays is nearly 10,000 times that of those electrons which produce microwave emission. The magnetic field and source size of the microwave emission region are found to be 375 gauss and 7 arcsec, respectively, and the kinetic energy involved in flare strand separation turns out to be 6.2 x 10 to the 27th erg/sec.

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