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Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse
Chen, Yajie; Tian, Hui; Su, Yingna; Qu, Zhongquan; Deng, Linhua; Jibben, Patricia R.; Yang, Zihao; Zhang, Jingwen; Samanta, Tanmoy; He, Jiansen; Wang, Linghua; Zhu, Yingjie; Zhong, Yue; Liang, Yu
2018
发表期刊ASTROPHYSICAL JOURNAL
卷号856期号:1页码:21
摘要We present an investigation of a coronal cavity observed above the western limb in the coronal red line Fe X 6374 angstrom using a telescope of Peking University and in the green line Fe XIV 5303 angstrom using a telescope of Yunnan Observatories, Chinese Academy of Sciences, during the total solar eclipse on 2017 August 21. A series of magnetic field models is constructed based on the magnetograms taken by the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory (SDO) one week before the eclipse. The model field lines are then compared with coronal structures seen in images taken by the Atmospheric Imaging Assembly on board SDO and in our coronal red line images. The best-fit model consists of a flux rope with a twist angle of 3.1 pi, which is consistent with the most probable value of the total twist angle of interplanetary flux ropes observed at 1 au. Linear polarization of the Fe XIII 10747 angstrom line calculated from this model shows a "lagomorphic" signature that is also observed by the Coronal Multichannel Polarimeter of the High Altitude Observatory. We also find a ring-shaped structure in the line-of-sight velocity of Fe XIII 10747 angstrom, which implies hot plasma flows along a helical magnetic field structure, in the cavity. These results suggest that the magnetic structure of the cavity is a highly twisted flux rope, which may erupt eventually. The temperature structure of the cavity has also been investigated using the intensity ratio of Fe XIII 10747 angstrom and Fe X 6374 angstrom.
语种英语
WOS记录号WOS:000428455800007
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文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/18042
专题太阳高能及相关物理过程研究团组
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Chen, Yajie,Tian, Hui,Su, Yingna,et al. Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse[J]. ASTROPHYSICAL JOURNAL,2018,856(1):21.
APA Chen, Yajie.,Tian, Hui.,Su, Yingna.,Qu, Zhongquan.,Deng, Linhua.,...&Liang, Yu.(2018).Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse.ASTROPHYSICAL JOURNAL,856(1),21.
MLA Chen, Yajie,et al."Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse".ASTROPHYSICAL JOURNAL 856.1(2018):21.
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