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The broadening cause of the CaXIX resonace line in solar flares
Li, YP ; Gan, WQ
2002
Source PublicationSOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT
Volume14Pages:173—174
AbstractWe distinguish different broadening mechanisms of the CaXIX resonance line by studying the influence of the loop orientation, based on the data observed with SXT and BCS on Yohkoh. The results seem to support that the broadening of the CaXIX resonance line is caused by the nonthermal turbulence, rather than by the velocity dispersion.
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7914
Collection太阳高能及相关物理过程研究团组
Recommended Citation
GB/T 7714
Li, YP,Gan, WQ. The broadening cause of the CaXIX resonace line in solar flares[J]. SOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT,2002,14:173—174.
APA Li, YP,&Gan, WQ.(2002).The broadening cause of the CaXIX resonace line in solar flares.SOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT,14,173—174.
MLA Li, YP,et al."The broadening cause of the CaXIX resonace line in solar flares".SOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT 14(2002):173—174.
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