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Dynamics of the Hard X-ray, Gamma-ray, and Microwave Emission of Solar Flares Produced by the Active Region NOAA 0069 in August 2002статья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 13 мая 2014 г.
- Авторы: Bogomolov A.V., Kashapova L.K., Myagkova I.N., Tsap Yu T.
- Журнал: Astronomy Reports
- Том: 58
- Номер: 3
- Год издания: 2014
- Издательство: Maik Nauka/Interperiodica Publishing
- Местоположение издательства: Russian Federation
- Первая страница: 156
- Последняя страница: 166
- DOI: 10.1134/S1063772914030020
- Аннотация: Regularities have been searched for in the dynamics of characteristics of flare solar radiation during the development of the active region NOAA 0069 in the interval of August 14–24, 2002. The SONG (Solar Neutrons and Gamma rays) instrument onboard the Russian CORONAS-F Solar Observatory recorded hard X-ray and gamma-ray radiation in nine of the 30 flares of class above C5 in this active region within the indicated time interval. It was obtained that, in accordance with the development of the active region, the X- and gamma-ray flux tended to increase at the flare maxima while the hard X-ray spectral index tended to decrease; flares with a harder radiation spectrum occurred in the sunspot umbra, i.e., in the region with the strongest magnetic fields.
- Добавил в систему: Мягкова Ирина Николаевна