KMS of Xinjiang Astronomical Observatory, CAS
| Magnetic Field Extrapolation in Active Region Well Comparable to Observations in Multiple Layers | |
Yu, Fu1,2,3; Zhao, Jie1,3; Su, Yang1,2; Zhu, Xiaoshuai3; Guo, Yang4,5; Shen, Jinhua6 ; Li, Hui1,2
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| 2023-07-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 951Issue:1Pages:54 |
| Contribution Rank | 5 |
| Abstract | Magnetic field extrapolation is a fundamental tool to reconstruct the three-dimensional magnetic field above the solar photosphere. However, the prevalently used force-free field model might not be applicable in the lower atmosphere with non-negligible plasma & beta;, where the crucial process of flux rope formation and evolution could happen. In this work, we perform extrapolation in active region 12158, based on a recently developed magnetohydrostatic (MHS) method that takes plasma forces into account. By comparing the results with those from the force-free field extrapolation methods, we find that the overall properties, which are characterized by the magnetic free energy and helicity, are roughly the same. The major differences lie in the magnetic configuration and the twist number of the magnetic flux rope (MFR). Unlike previous works either obtained sheared arcades or one coherent flux rope, the MHS method derives two sets of MFR, which are highly twisted and slightly coupled. Specifically, the result in the present work is more comparable to the high-resolution observations from the chromosphere, through the transition region to the corona, such as the filament fibrils, pre-eruptive braiding characteristics, and the eruptive double-J-shaped hot channel. Overall, our work shows that the newly developed MHS method is more promising to reproduce the magnetic fine structures that can well match the observations at multiple layers, and future data-driven simulation based on such extrapolation will benefit in understanding the critical and precise dynamics of flux rope before eruption. |
| DOI | 10.3847/1538-4357/acd112 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | FLUX ROPES ; HELICITY ESTIMATIONS ; MAGNETOSTATIC ATMOSPHERES ; 3-DIMENSIONAL STRUCTURES ; KINK INSTABILITY ; SOLAR ERUPTIONS ; ENERGY-RELEASE ; MHD SIMULATION ; MODELS ; STABILITY |
| Funding Project | NJIT ; US NSF[AGS-1821294] ; Korea Astronomy and Space Science Institute, Seoul National University ; Key Laboratory of Solar Activities of the Chinese Academy of Sciences (CAS) ; Operation, Maintenance, and Upgrading Fund of CAS for Astronomical Telescopes and Facility Instruments ; National Natural Science Foundation of China[11820101002] ; National Natural Science Foundation of China[U1731241] ; National Natural Science Foundation of China[2023333] ; Youth Innovation Promotion Association CAS[12233012] ; Chinese Academy of Science Strategic Pioneer Program on Space Science[XDA15052200] ; Chinese Academy of Science Strategic Pioneer Program on Space Science[XDA15320103] ; Chinese Academy of Science Strategic Pioneer Program on Space Science[XDA15320301] ; Sino-German Science Center[M-0068] ; National Key Ramp ; D Program of China[2021YFA1600503] ; NSFC[11773016] ; NSFC[11961131002] ; NSFC[11533005] ; NSFC[2020YFC2201201] ; NSFC[12273101] ; Open Research Program of the CAS Key Laboratory of Solar Activity[KLSA202112] ; International Space Science Institute (ISSI) in Bern and the ISSI-BJ in Beijing, through ISSI International Team[55] ; International Space Science Institute (ISSI) in Bern and the ISSI-BJ in Beijing, through ISSI International Team[568] ; [2022YFF0503001] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001022148000001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | NJIT ; US NSF ; Korea Astronomy and Space Science Institute, Seoul National University ; Key Laboratory of Solar Activities of the Chinese Academy of Sciences (CAS) ; Operation, Maintenance, and Upgrading Fund of CAS for Astronomical Telescopes and Facility Instruments ; National Natural Science Foundation of China ; Youth Innovation Promotion Association CAS ; Chinese Academy of Science Strategic Pioneer Program on Space Science ; Sino-German Science Center ; National Key Ramp ; D Program of China ; NSFC ; Open Research Program of the CAS Key Laboratory of Solar Activity ; International Space Science Institute (ISSI) in Bern and the ISSI-BJ in Beijing, through ISSI International Team |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5296 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Zhao, Jie |
| Affiliation | 1.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210023, Peoples R China 2.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China 3.Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing 100190, Peoples R China 4.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China 5.Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China 6.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China |
| Recommended Citation GB/T 7714 | Yu, Fu,Zhao, Jie,Su, Yang,et al. Magnetic Field Extrapolation in Active Region Well Comparable to Observations in Multiple Layers[J]. ASTROPHYSICAL JOURNAL,2023,951(1):54. |
| APA | Yu, Fu.,Zhao, Jie.,Su, Yang.,Zhu, Xiaoshuai.,Guo, Yang.,...&Li, Hui.(2023).Magnetic Field Extrapolation in Active Region Well Comparable to Observations in Multiple Layers.ASTROPHYSICAL JOURNAL,951(1),54. |
| MLA | Yu, Fu,et al."Magnetic Field Extrapolation in Active Region Well Comparable to Observations in Multiple Layers".ASTROPHYSICAL JOURNAL 951.1(2023):54. |
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| Yu-2023-Magnetic Fie（7685KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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