Physical processes in the solar atmosphere associated with flares

B.V. Somov^a, S.I. Syrovatskii
^aLomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

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.

PACS: 96.20.Sh
DOI: 10.1070/PU1976v019n10ABEH005337
URL: https://ufn.ru/en/articles/1976/10/b/
Citation: Somov B V, Syrovatskii S I "Physical processes in the solar atmosphere associated with flares" Sov. Phys. Usp. 19 813–835 (1976)

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PT Journal Article
TI Physical processes in the solar atmosphere associated with flares
AU Somov B V
FAU Somov BV
AU Syrovatskii S I
FAU Syrovatskii SI
DP 10 Oct, 1976
TA Phys. Usp.
VI 19
IP 10
PG 813-835
RX 10.1070/PU1976v019n10ABEH005337
URL https://ufn.ru/en/articles/1976/10/b/
SO Phys. Usp. 1976 Oct 10;19(10):813-835

Оригинал: Сомов Б В, Сыроватский С И «Физические процессы в атмосфере Солнца, вызываемые вспышками» УФН 120 217–257 (1976); DOI: 10.3367/UFNr.0120.197610b.0217