Variations of microwave emission from solar active regions

Variations of microwave emission from solar active regions

Based on observational data obtained with the RT-22 Crimean Astrophysical Observatory radio telescope at frequencies of 8.6 and 15.4 GHz, we investigate the quasi-periodic variations of microwave emission from solar active regions with periods T^sub p^

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Veröffentlicht in:Astronomy letters 2004-07, Vol.30 (7), p.489-495
Hauptverfasser: Gelfreikh, G B, Tsap, Yu T, Kopylova, Yu G, Goldvarg, T B, Nagovitsyn, Yu A, Tsvetkov, L I
Format: Artikel
Sprache:eng
Schlagworte:
Emissions
Sun
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Zusammenfassung:Based on observational data obtained with the RT-22 Crimean Astrophysical Observatory radio telescope at frequencies of 8.6 and 15.4 GHz, we investigate the quasi-periodic variations of microwave emission from solar active regions with periods T^sub p^
ISSN:1063-7737
1562-6873
DOI:10.1134/1.1774401