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JOURNALS // Uspekhi Fizicheskikh Nauk // Archive

UFN, 1976 Volume 120, Number 2, Pages 217–257 (Mi ufn9887)

This article is cited in 101 papers

REVIEWS OF TOPICAL PROBLEMS

Physical processes in the solar atmosphere associated with flares

B. V. Somov, S. I. Syrovatsky

P. N. Lebedev Physical Institute, the USSR Academy of Sciences, Moscow

Abstract: Flares on the sun release an enormous amount of energy in the form of accelerated particles, heat fluxes, matter fluxes, and radiation. The relative importance of each of these energy channels is reviewed and the reaction of the solar atmosphere to the corresponding energy fluxes is considered. The possibility of determining the characteristics of the primary process of the flare from its secondary manifestations in the atmosphere of the sun is discussed.

UDC: 523.75

PACS: 96.20.Sh

DOI: 10.3367/UFNr.0120.197610b.0217


 English version:
Physics–Uspekhi, 1976, 19:10, 813–835


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