Large Flares (M1–X7) in Solar Activity Cycle 24
- 作者: Bruevich E.A.1, Kazachevskaya T.V.2, Yakunina G.V.1
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隶属关系:
- Sternberg Astronomical Institute
- Fedorov Institute of Applied Geophysics
- 期: 卷 57, 编号 8 (2017)
- 页面: 1077-1085
- 栏目: Article
- URL: https://journal-vniispk.ru/0016-7932/article/view/156592
- DOI: https://doi.org/10.1134/S0016793217080059
- ID: 156592
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详细
The large (X-ray class > M1) and very large (X-ray class > X1) flares (according to the observations of GOES-15 and Preliminary data from Current Catalog of Flare Events) in solar activity cycle 24 were analyzed. The monthly average values of optical Flare Index for 2010–2016 were calculated. The values of the total energy of the flare E (J m–2) in the 0.1–0.8 nm range at the level of the earth’s atmosphere were estimated. The energy spectrum (the dependence of the number of flares with the full energy E from the value of this full energy) for 115 flares of M5–X7 classes was built. The comparative study of monthly average values of several indices of solar activity in current cycle 24–the relative sunspot numbers (SSN), the 10.7 cm radio flux (F10.7), the radiation flux in the Lyman-alpha line (FLy-α), the solar constant (TSI) and the Flare Index (FI)–was made.
作者简介
E. Bruevich
Sternberg Astronomical Institute
编辑信件的主要联系方式.
Email: red-field@yandex.ru
俄罗斯联邦, Moscow, 119992
T. Kazachevskaya
Fedorov Institute of Applied Geophysics
Email: red-field@yandex.ru
俄罗斯联邦, Moscow, 129128
G. Yakunina
Sternberg Astronomical Institute
Email: red-field@yandex.ru
俄罗斯联邦, Moscow, 119992
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