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1976

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October

  

Reviews of topical problems


Physical processes in the solar atmosphere associated with flares

 a,
a Lomonosov 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.

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Fulltext is also available at DOI: 10.1070/PU1976v019n10ABEH005337
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)
BibTexBibNote ® (generic)BibNote ® (RIS)Medline RefWorks
RT Journal
T1 Physical processes in the solar atmosphere associated with flares
A1 Somov,B.V.
A1 Syrovatskii,S.I.
PB Physics-Uspekhi
PY 1976
FD 10 Oct, 1976
JF Physics-Uspekhi
JO Phys. Usp.
VO 19
IS 10
SP 813-835
DO 10.1070/PU1976v019n10ABEH005337
LK https://ufn.ru/en/articles/1976/10/b/

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

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