Tracking an Eruptive Intermediate Prominence Originating from the Farside of the Sun
文献类型：期刊论文
| 作者 | Zhang, Qingmin1,2; Pan, Wenwei1,3; Ying, Beili1; Feng, Li1; Li, Yiliang1,3; Yan XL(闫晓理)4,5 ; Yang LH(杨丽恒)4,5; Qiu, Ye6; Chen, Jun1; Ma, Suli2
|
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2025-06-01 |
| 卷号 | 985期号:2 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/add328 |
| 产权排序 | 第5完成单位 |
| 文献子类 | Article |
| 英文摘要 | In this paper, we carry out multiwavelength and multiview observations of the eruption of an intermediate prominence originating from the farside of the Sun on 2023 March 12. The southeast footpoint of the prominence is located in NOAA Active Region 13252. The eruption generates a B7.8 class flare and a partial halo coronal mass ejection (CME). The prominence takes off at 02:00 UT and accelerates for nearly 3 hr. Rotation of the southeast leg of the prominence in the counterclockwise direction is revealed by spectroscopic and imaging observations. The apex of the prominence changes from a smooth loop to a cusp structure during the rising motion, and the northwest leg displays a drift motion after 04:30 UT, implying a writhing motion. Hence, the prominence eruption is most likely triggered by ideal kink instability. For the first time, we apply the Graduated Cylindrical Shell modeling in 3D reconstruction and tracking of the prominence for nearly 2 hr. Both the source region (110 degrees E, 43 degrees N) and northwest footpoint (162 degrees E, 44 degrees N) are located. The edge-on and face-on angular widths of the prominence are similar to 6 degrees and similar to 86 degrees, respectively. The axis has a tilt angle of similar to 70 degrees with the meridian. The heliocentric distance of the prominence leading edge increases from similar to 1.26 R circle dot to similar to 2.27 R circle dot. The true speed of the CME increases from similar to 610 to similar to 849 km s-1. |
| 学科主题 | 天文学 ; 太阳与太阳系 |
| URL标识 | 查看原文 |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| WOS关键词 | CORONAL MASS EJECTIONS ; ALPHA SOLAR TELESCOPE ; ENERGETIC PARTICLE EVENT ; ACTIVE-REGION FILAMENT ; MAGNETIC-FLUX ROPE ; ASO-S MISSION ; KINK INSTABILITY ; 3-DIMENSIONAL RECONSTRUCTION ; MHD SIMULATIONS ; ROLLING MOTION |
| 资助项目 | China National Space Administration (CNSA); Strategic Priority Research Program on Space Science, Chinese Academy of Sciences; Extreme Ultraviolet Imager (EUI); Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000]; National Key R&D Program of China[2021YFA1600500 (2021YFA1600502)]; National Key R&D Program of China[2022YFF0503003]; National Key R&D Program of China[2022YFF0503000]; NSFC[12373065]; NSFC[12203102]; Natural Science Foundation of Jiangsu Province[BK20231510]; Specialized Research Fund for State Key Laboratory of Solar Activity and Space Weather |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001498732500001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | China National Space Administration (CNSA) ; Strategic Priority Research Program on Space Science, Chinese Academy of Sciences ; Extreme Ultraviolet Imager (EUI) ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000] ; National Key R&D Program of China[2021YFA1600500 (2021YFA1600502), 2022YFF0503003, 2022YFF0503000] ; NSFC[12373065, 12203102] ; Natural Science Foundation of Jiangsu Province[BK20231510] ; Specialized Research Fund for State Key Laboratory of Solar Activity and Space Weather |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28328]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 |
| 作者单位 | 1.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Nanjing 210023, People's Republic of China; zhangqm@pmo.ac.cn; 2.State Key Laboratory of Solar Activity and Space Weather, Beijing 100190, People's Republic of China; 3.Department of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China; 4.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, People's Republic of China; 5.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 6.Institute of Science and Technology for Deep Space Exploration, Suzhou Campus, Nanjing University, Suzhou 215163, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Zhang, Qingmin,Pan, Wenwei,Ying, Beili,et al. Tracking an Eruptive Intermediate Prominence Originating from the Farside of the Sun[J]. ASTROPHYSICAL JOURNAL,2025,985(2). |
| APA | Zhang, Qingmin.,Pan, Wenwei.,Ying, Beili.,Feng, Li.,Li, Yiliang.,...&Ma, Suli.(2025).Tracking an Eruptive Intermediate Prominence Originating from the Farside of the Sun.ASTROPHYSICAL JOURNAL,985(2). |
| MLA | Zhang, Qingmin,et al."Tracking an Eruptive Intermediate Prominence Originating from the Farside of the Sun".ASTROPHYSICAL JOURNAL 985.2(2025). |
入库方式： OAI收割
来源：云南天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。