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Hard X-Ray Emission of Solar Flares Measured by Lomonosov Space Missionстатья
Информация о цитировании статьи получена из
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 29 июля 2020 г.
- Авторы: Myagkova Irina N., Bogomolov Andrey V., Bogomolov Vitaly V., Svertilov Sergey I., Bobrovnikov Sergey Yu, Yashin Ivan V., Panasyuk Mikhail I., Kalegaev Vladimir V., Petrov Vasily L., Shishkova Svetlana S.
- Журнал: Proceedings of the International Astronomical Union
- Том: 13
- Номер: S335
- Год издания: 2018
- Первая страница: 29
- Последняя страница: 31
- DOI: 10.1017/S1743921317008821
- Аннотация: Solar hard X-ray and gamma-ray emission was measured by BDRG instrument, the part of set of instruments operated on board the Russian satellite Lomonosov from April 2016 until now (solar-synchronous orbit with altitude 490 km, inclination of 97.6 degrees). Lomonosov measurements (11 flares with the X-ray energy more than 10 keV, and more than half of them have class in soft X-rays less than C2) were compared to the data obtained by RHESSI and Fermi space observatories as well as the Nobeyama Radioheliograph operating at the same time. The quasi-periodicity with different periods were found in some of them.
- Добавил в систему: Богомолов Андрей Владимирович