Three-dimensional distribution of the escape photons of H alpha flares | |
Sun MG(孙明国)1,3; Qu ZQ(屈中权)1; Xu Z(徐稚)2; Zhang XY(张霄宇)1; Xu CL(胥成林)1,3; Wang S(王帅)1,3; Jin CL(金春兰)1,3; Sun, MG (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, Kunming 650011, Peoples R China. | |
发表期刊 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS |
2006 | |
卷号 | 6期号:1页码:87-95 |
DOI | 10.1088/1009-9271/6/1/010 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Line : Formation Radiative Transfer Sun : Flares |
摘要 | A technique for obtaining a three-dimensional distribution of received photons in Ha flares in the solar atmosphere is presented. It is well known that during flares hydrogen atoms in the chromosphere and photosphere are excited (even ionized) by the downward heating of non-thermal particles and then emit Ha. photons. We trace back these Ha photons to their original layers by use of the contribution function in the theory of spectral line formation, and so acquire their three-dimensional (3D) distribution. This technique is applied to the two-ribbon flare of 2002 January 20. The atmospheric models are obtained by fitting the "quasi-profiles" with the help of the generally used model atmospheres. Since the variety of the 3D images reflects the response of the atmospheric layers to the impact of energy transport, an analysis of the development of the flare is given through a comparison of the 3D images with the 2D temperature distribution. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 1009-9271 |
URL | 查看原文 |
归档日期 | 2006-03-03 |
WOS记录号 | WOS:000235501700010 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | LINE FORMATION PROCESS ; WHITE-LIGHT FLARE ; SOLAR CHROMOSPHERE ; NONTHERMAL ELECTRONS ; SEMIEMPIRICAL MODELS ; OPTICAL-SPECTRA ; ATMOSPHERES ; DIAGNOSTICS ; IONIZATION ; SIGNATURES |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6094 |
专题 | 太阳物理研究组 |
通讯作者 | Sun, MG (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.Yunnan Astronomical Observatory/National Astronomical Observatories, Chinese Academy of Sciences, Kunming 650011 2.Astronomical Department of Astronomy, Nanjing University, Nanjing 210093 3.Graduate University of the Chinese Academy of Sciences, Beijing 100049 |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Sun MG,Qu ZQ,Xu Z,et al. Three-dimensional distribution of the escape photons of H alpha flares[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2006,6(1):87-95. |
APA | Sun MG.,Qu ZQ.,Xu Z.,Zhang XY.,Xu CL.,...&Sun, MG .(2006).Three-dimensional distribution of the escape photons of H alpha flares.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,6(1),87-95. |
MLA | Sun MG,et al."Three-dimensional distribution of the escape photons of H alpha flares".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 6.1(2006):87-95. |
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