Some results of model calculations of the solar S‐component radio emission
- 1 January 1985
- journal article
- Published by Wiley in Astronomische Nachrichten
- Vol. 306 (3) , 157-166
- https://doi.org/10.1002/asna.2113060312
Abstract
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.Keywords
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