Millimeter and X-ray emissions from the Solar flare of 31 october 1991

Details Millimeter and X-ray emissions from the Solar flare of 31 october 1991 Millimeter and X-ray emissions from the Solar flare of 31 october 1991

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002kfnt...18....3t&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 18, no. 1, p. 3-17

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The solar flare of 31 October 1991 is analyzed on the basis of the millimeter and X-ray observations obtained with the RT-22 radio telescope of the Crimean Astrophysical Observatory and the GOES, BATSE, and Yohkoh space stations. Arguments in favor of the non-thermal nature of the millimeter emission are given. The magnetic field strength, the temperature, and the emission measure of the flare plasma as well as the quantity of accelerated electrons and their spectral index are estimated. It was found that thermal particles rather than accelerated ones contain the major part of the flare energy. The peculiarities of the millimeter and hard X-ray emissions are interpreted within the frame-work of the coronal magnetic trap model with developed plasma turbulence.

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