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.
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.