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- W1561426887 abstract "Magnetic fields dominate most solar activities, there exist direct relations between solar flare and the distributions of magnetic field, and also its corresponding magnetic energy. In this paper, the statistical results about the relationships between the spatial magnetic field and solar flare are given basing on vector magnetic field observed by the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station (HSOS). The spatial magnetic fields are obtained by extrapolated photosphere vector magnetic field observed by SMFT. There are 23 active regions with flare eruption are chosen as data samples, which were observed from 1997 to 2007. The results are as follows: 1. Magnetic field lines become lower after flare for 16(69%) active regions; 2. The free energy are decreased after flare for 17 (74%) active regions. It can conclude that for most active regions the changes of magnetic field after solar flare are coincident with the previous observations and studies." @default.
- W1561426887 created "2016-06-24" @default.
- W1561426887 creator A5031731992 @default.
- W1561426887 date "2014-06-01" @default.
- W1561426887 modified "2023-10-18" @default.
- W1561426887 title "A statistical study on property of spatial magnetic field for solar active region" @default.
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- W1561426887 doi "https://doi.org/10.1007/s10509-014-1852-8" @default.
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