Theoretical scaling law of coronal magnetic field and electron power-law index in solarmicrowave burst sources | |
Huang, Y.1,2; Song, Q. W.1,2; Tan, B. L.3,4 | |
刊名 | ASTROPHYSICS AND SPACE SCIENCE |
2018-04-01 | |
卷号 | 363期号:4页码:7 |
关键词 | The Sun: flares The Sun: radio radiation The Sun: corona The Sun: magnetic fields The Sun: energetic particles |
ISSN号 | 0004-640X |
DOI | 10.1007/s10509-018-3301-6 |
英文摘要 | It is first proposed a theoretical scaling law respectively for the coronal magnetic field strength B and electron power-law index delta versus frequency and coronal height in solar microwave burst sources. Based on the non-thermal gyro-synchrotron radiation model (Ramaty in Astrophys. J. 158:753, 1969), B and delta are uniquely solved by the observable optically-thin spectral index and turnover (peak) frequency, the other parameters (plasma density, temperature, view angle, low and high energy cutoffs, etc.) are relatively insensitive to the calculations, thus taken as some typical values. Both of B and delta increase with increasing of radio frequency but with decreasing of coronal height above photosphere, and well satisfy a square or cubic logarithmic fitting. |
资助项目 | NFSC[11203083] ; NFSC[11427803] ; NFSC[U1731241] ; NFSC[11273030] ; Strategic Pioneer Program on Space Science, CAS[XDA15052200] ; Strategic Pioneer Program on Space Science, CAS[XDA15320301] |
WOS关键词 | GYROSYNCHROTRON EMISSION ; MICROWAVE-BURSTS ; PLASMA |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | SPRINGER |
WOS记录号 | WOS:000429130000019 |
资助机构 | NFSC ; NFSC ; Strategic Pioneer Program on Space Science, CAS ; Strategic Pioneer Program on Space Science, CAS ; NFSC ; NFSC ; Strategic Pioneer Program on Space Science, CAS ; Strategic Pioneer Program on Space Science, CAS ; NFSC ; NFSC ; Strategic Pioneer Program on Space Science, CAS ; Strategic Pioneer Program on Space Science, CAS ; NFSC ; NFSC ; Strategic Pioneer Program on Space Science, CAS ; Strategic Pioneer Program on Space Science, CAS |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/37109] |
专题 | 中国科学院国家天文台 |
通讯作者 | Huang, Y. |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Chinese Acad Sci, Key Lab Space Astron & Dark Matter, Nanjing 210008, Jiangsu, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 4.Chinese Acad Sci, Key Lab Solar Activ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Huang, Y.,Song, Q. W.,Tan, B. L.. Theoretical scaling law of coronal magnetic field and electron power-law index in solarmicrowave burst sources[J]. ASTROPHYSICS AND SPACE SCIENCE,2018,363(4):7. |
APA | Huang, Y.,Song, Q. W.,&Tan, B. L..(2018).Theoretical scaling law of coronal magnetic field and electron power-law index in solarmicrowave burst sources.ASTROPHYSICS AND SPACE SCIENCE,363(4),7. |
MLA | Huang, Y.,et al."Theoretical scaling law of coronal magnetic field and electron power-law index in solarmicrowave burst sources".ASTROPHYSICS AND SPACE SCIENCE 363.4(2018):7. |
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