Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse
文献类型：期刊论文
| 作者 | Chen,Yajie1; Tian,Hui1; Su,Yingna2,3 ; Qu,Zhongquan4; Deng,Linhua4; Jibben,Patricia R.5; Yang,Zihao1; Zhang,Jingwen1; Samanta,Tanmoy1; He,Jiansen1
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| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2018-03-21 |
| 卷号 | 856期号:1 |
| ISSN号 | 0004-637X |
| 关键词 | Sun: corona Sun: filaments, prominences Sun: magnetic fields |
| DOI | 10.3847/1538-4357/aaaf68 |
| 英文摘要 | Abstract We present an investigation of a coronal cavity observed above the western limb in the coronal red line Fe x 6374 ? using a telescope of Peking University and in the green line Fe xiv 5303 ? 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 3.1π, 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 ? 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 ?, 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 ? and Fe x 6374 ?. |
| 语种 | 英语 |
| 出版者 | The American Astronomical Society |
| WOS记录号 | IOP:0004-637X-856-1-AAAF68 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/22400]  |
| 专题 | 中国科学院紫金山天文台 |
| 作者单位 | 1.School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China 2.Key Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, CAS, Nanjing 210008, People's Republic of China; huitian@pku.edu.cn 3.School of Astronomy and Space Science, University of Science and Technology of China, Hefei, Anhui 230026, People's Republic of China 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People's Republic of China 5.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA |
| 推荐引用方式 GB/T 7714 | 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]. The Astrophysical Journal,2018,856(1). |
| 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.The Astrophysical Journal,856(1). |
| MLA | Chen,Yajie,et al."Diagnosing the Magnetic Field Structure of a Coronal Cavity Observed during the 2017 Total Solar Eclipse".The Astrophysical Journal 856.1(2018). |
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来源：紫金山天文台
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