PMO OpenIR  > 太阳高能及相关物理过程研究团组
An invariable point in the energy spectra of non-thermal electrons of solar flares
Gan, WQ
1998
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
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 keeps 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.
KeywordX-ray Observations Satellite Bursts Models
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordX-RAY OBSERVATIONS ; SATELLITE ; BURSTS ; MODELS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000080922200007
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8343
Collection太阳高能及相关物理过程研究团组
AffiliationAcad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Gan, WQ. An invariable point in the energy spectra of non-thermal electrons of solar flares[J]. ASTROPHYSICS AND SPACE SCIENCE,1998,260(4):515-519.
APA Gan, WQ.(1998).An invariable point in the energy spectra of non-thermal electrons of solar flares.ASTROPHYSICS AND SPACE SCIENCE,260(4),515-519.
MLA Gan, WQ."An invariable point in the energy spectra of non-thermal electrons of solar flares".ASTROPHYSICS AND SPACE SCIENCE 260.4(1998):515-519.
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