Some issues in diagnostics of solar chromospheric magnetic fields with the Mg b(2) line | |
Bai, Xian-Yong; Deng, Yuan-Yong; Su, Jiang-Tao; Wang, Guo-Ping | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2014 | |
卷号 | 14期号:2页码:193-206 |
关键词 | Sun: chromospheric magnetic fields spectral profiles: radiative transfer |
ISSN号 | 1674-4527 |
通讯作者 | Bai, XY (reprint author), Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China. |
英文摘要 | Up to now, exact measurements of chromospheric magnetic fields have not been as successful as those done in the photosphere. We are currently engaging in diagnostics of chromospheric magnetic fields with the Mg b(2) line by employing the Multi-Channel Solar Telescope at Huairou Solar Observing Station. Therefore, how to improve accuracy in the measurement is the main issue of our present study. To this end, we first study linear calibration coefficients for longitudinal and transverse components of chromospheric fields, which vary with wavelength, in the case of a weak field assumption. Then the polarization crosstalk introduced by instruments is analyzed in detail with two numerical simulation methods. Comparisons of the polarization signals between cases with and without correction are presented. The result indicates that polarization accuracy is greatly improved after crosstalk correction. |
学科主题 | 空间物理 |
收录类别 | SCI |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://ir.nssc.ac.cn/handle/122/2766] |
专题 | 国家空间科学中心_空间科学部 |
推荐引用方式 GB/T 7714 | Bai, Xian-Yong,Deng, Yuan-Yong,Su, Jiang-Tao,et al. Some issues in diagnostics of solar chromospheric magnetic fields with the Mg b(2) line[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2014,14(2):193-206. |
APA | Bai, Xian-Yong,Deng, Yuan-Yong,Su, Jiang-Tao,&Wang, Guo-Ping.(2014).Some issues in diagnostics of solar chromospheric magnetic fields with the Mg b(2) line.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,14(2),193-206. |
MLA | Bai, Xian-Yong,et al."Some issues in diagnostics of solar chromospheric magnetic fields with the Mg b(2) line".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 14.2(2014):193-206. |
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