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Characteristics of SEP events produced by solar flares during evolution of the active region and their relationship with radio and HXR solar emissionтезисы доклада
- Авторы: Myagkova I.N., Kashapova L.K., Miteva R., Bogomolov A.V.
- Сборник: Abstract book of The 4th RadioSun Workshop and Summer School, Irkutsk, Russia, (8th - 12th June 2015)
- Тезисы
- Год издания: 2015
- Место издания: ИСЗФ РАН Иркутск
- Первая страница: 26
- Аннотация: We present the results of comparative analysis of the solar energetic particles characteristics such as SEP total flux, their maximal energy and spectral index with parameters of X-ray and microwave emission of the solar flares, which were their sources. All studied SEP events were produced by the successive flares occurred in the active region 0069 in August 2002. It was found that during this series of flares the more powerful SEP events with higher energies were observed after those flares in which the delay between microwave and HXR temporal profiles were minimal. Results of study of SEP acceleration and propagation based on the analysis of delays between radio and HXR-rays emission and peculiarities of measured SXR and HXR-emission spectra are discussed.
- Добавил в систему: Мягкова Ирина Николаевна