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The plasma wake field excited by solar energetic flare electrons through the corona
Huang YN(黄永年); Wang XY(王学英); Int Union, Pure; Appl, Phys
Department空间天气学国家重点实验室
Source Publication24th international cosmic ray conference, vol 4 - sh sessions - contributed papers
1995
Pages1-4
Language英语
AbstractThe plasma wake fields (PWFs) excited by the interaction of high-energy electron beams with a cold and hot plasma are calculated. We have studied tau-profiles of the PWFs resulted from the interaction of high energy electron beams from solar impulsive hares with the coronal ground plasma, and the acceleration of lower energy electrons in the hares by this PWFs. The tau = omega(p)(t - x/v(b)), where omega(p) is the plasma frequency.
Conference Name24th International Cosmic Ray Conference (XXIV ICRC)
Conference Date1995
Conference PlaceRome, Italy
Indexed ByCPCI
Document Type会议论文
Identifierhttp://ir.nssc.ac.cn/handle/122/919
Collection空间科学部
Recommended Citation
GB/T 7714
Huang YN,Wang XY,Int Union, Pure,et al. The plasma wake field excited by solar energetic flare electrons through the corona[C]. URBINO:Argalia Editore Delle Arti Grafiche Editoriali Srl,1995:1-4.
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