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An invariable point in the energy spectra of non-thermal electrons of solar flares
Gan, W.Q.
1999
Source PublicationAstrophysics and Space Science
Volume260Issue:4Pages:515-519
AbstractThe power-law energy spectra of non-thermal electrons for each 1.024 second have been drawn together during the flare. For some flares, it is discovered that the energy spectra taken at different times present a roughly fixed crossing point, at which point the flux of non-thermal electrons remains the same during the flare. The possible significance of this phenomenon is discussed. We conjecture that there may be a flux saturation at the low-energy cutoff in the process of electron acceleration
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8310
Collection太阳高能及相关物理过程研究团组
Recommended Citation
GB/T 7714
Gan, W.Q.. An invariable point in the energy spectra of non-thermal electrons of solar flares[J]. Astrophysics and Space Science,1999,260(4):515-519.
APA Gan, W.Q..(1999).An invariable point in the energy spectra of non-thermal electrons of solar flares.Astrophysics and Space Science,260(4),515-519.
MLA Gan, W.Q.."An invariable point in the energy spectra of non-thermal electrons of solar flares".Astrophysics and Space Science 260.4(1999):515-519.
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