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Some results of model calculations of the solar S‐component radio emission
Author(s) -
Krüger A.,
Hildebrandt J.
Publication year - 1985
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113060312
Subject(s) - sunspot , physics , astrophysics , component (thermodynamics) , stars , microwave , solar radio , computational physics , radiation , solar physics , astronomy , solar flare , magnetic field , optics , quantum mechanics , thermodynamics
Numerical calculations of special characteristics of the solar S‐component microwave radiation are presented on the basis of recent sunspot and plage models. Quantitative results are discussed and can be used for the plasma diagnostics of solar active regions by comparisons with observations with high spatial and spectral resolution. The possibility of generalized applications to magnetic stars and stellar activity is briefly noted.