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Higher blueshift components in higher-resolution Fe XXV line profiles as evidence of a time-dependent Petschek-type reconnection
Lin J(林隽); Martin, R; Wu, N; Lin, J
Source PublicationASTRONOMY & ASTROPHYSICS
1996-07
Volume311Issue:3Pages:1015-1023
Contribution Rank第1完成单位
Indexed BySCI
KeywordSun Flares Sun X-rays Sun Magnetic Fields
AbstractWe re-investigated the higher blueshift components in higher-resolution Fe XXV line profiles observed during some flares by Antonucci et al. (1990a, b) in detail. The present work was mainly concentrated on the initial part of impulsive phase of the 1984 April 24 flare. The results show that the traditional chromospheric evaporation interpretation seems hardly to be able to account for these higher blueshift components. We tried to ascribe these features to the time-dependent Petschek-type reconnection process. On this basis, some important parameters, such as electron density, temperature, magnetic field in the flare region, etc., were estimated. Our results were found reasonable and consistent with the observations and theoretical estimates obtained by others.
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0004-6361
URL查看原文
WOS IDWOS:A1996UZ29300034
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordX-RAY-SPECTRA ; SOLAR-FLARE TEMPERATURES ; IMPULSIVE PHASE ; CHROMOSPHERIC EVAPORATION ; NUMERICAL SIMULATIONS ; SOFT ; TURBULENCE ; EMISSION ; PLASMA
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6021
Collection太阳物理研究组
Corresponding AuthorLin, J
Recommended Citation
GB/T 7714
Lin J,Martin, R,Wu, N,et al. Higher blueshift components in higher-resolution Fe XXV line profiles as evidence of a time-dependent Petschek-type reconnection[J]. ASTRONOMY & ASTROPHYSICS,1996,311(3):1015-1023.
APA 林隽,Martin, R,Wu, N,&Lin, J.(1996).Higher blueshift components in higher-resolution Fe XXV line profiles as evidence of a time-dependent Petschek-type reconnection.ASTRONOMY & ASTROPHYSICS,311(3),1015-1023.
MLA 林隽,et al."Higher blueshift components in higher-resolution Fe XXV line profiles as evidence of a time-dependent Petschek-type reconnection".ASTRONOMY & ASTROPHYSICS 311.3(1996):1015-1023.
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