Formation of transient coronal holes during the eruption of a quiescent filament and its overlying sigmoid
文献类型：期刊论文
| 作者 | Yang LH(杨丽恒)1,2 ; Jiang YC(姜云春)1; Ren DB(任冬柏)1,2
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| 刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2008-06 |
| 卷号 | 8期号:3页码:329-336 |
| 关键词 | Sun : filaments Sun : chromosphere Sun : coronal mass ejections (CMEs) |
| ISSN号 | 1009-9271 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Yang, LH (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | By using Ha, He 110830, EUV and soft X-ray (SXR) data, we examined a filament eruption that occurred on a quiet-sun region near the center of the solar disk on 2006 January 12, which disturbed a sigmoid overlying the filament channel observed by the GOES-12 SXR Imager (SXI), and led to the eruption of the sigmoid. The event was associated with a partial halo coronal mass ejection (CME) observed by the Large Angle and Spectrometric Coronagraphs (LASCO) on board the Solar and Heliospheric Observatory (SOHO), and resulted in the formation of two flare-like ribbons, post-eruption coronal loops, and two transient coronal holes (TCHs), but there were no significantly recorded GOES or Ha flares corresponding to the eruption. The two TCHs were dominated by opposite magnetic polarities and were located on the two ends of the eruptive sigmoid. They showed similar locations and shapes in He I 10830, EUV and SXR observations. During the early eruption phase, brightenings first appeared on the locations of the two subsequent TCHs, which could be clearly identified on He I 10830, EUV and SXR images. This eruption could be explained by the magnetic flux rope model, and the two TCHs were likely to be the feet of the flux rope. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | MASS EJECTIONS ; ACTIVE-REGION ; YOHKOH SXT ; DIMMINGS ; FLARES ; IMAGER ; CME |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1009-9271/8/3/09/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000257222800009 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6123]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 作者单位 | 1.National Astronomical Observatories / Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China 2.Graduate School of Chinese Academy of Sciences, Beijing 100049, China |
| 推荐引用方式 GB/T 7714 | Yang LH,Jiang YC,Ren DB. Formation of transient coronal holes during the eruption of a quiescent filament and its overlying sigmoid[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2008,8(3):329-336. |
| APA | Yang LH,Jiang YC,&Ren DB.(2008).Formation of transient coronal holes during the eruption of a quiescent filament and its overlying sigmoid.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,8(3),329-336. |
| MLA | Yang LH,et al."Formation of transient coronal holes during the eruption of a quiescent filament and its overlying sigmoid".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 8.3(2008):329-336. |
入库方式： OAI收割
来源：云南天文台
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