| A FLUX ROPE ERUPTION TRIGGERED BY JETS | |
Guo, J1 ; Liu Y(刘煜)2; Zhang, HQ1; Deng, YY1; Lin, JB1; Su, JT1; Guo, J (reprint author), Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China.
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| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2010-03-10 | |
| 卷号 | 711期号:2页码:1057-1061 |
| DOI | 10.1088/0004-637X/711/2/1057 |
| 产权排序 | 第2完成单位 |
| 收录类别 | SCI |
| 关键词 | Sun: Activity Sun: Coronal Mass Ejections (Cmes) Sun: Filaments Prominences |
| 摘要 | We present an observation of a filament eruption caused by recurrent chromospheric plasma injections (surges/jets) on 2006 July 6. The filament eruption was associated with an M2.5 two-ribbon flare and a coronal mass ejection (CME). There was a light bridge in the umbra of the main sunspot of NOAA 10898; one end of the filament was terminated at the region close to the light bridge, and recurrent surges were observed to be ejected from the light bridge. The surges occurred intermittently for about 8 hr before the filament eruption, and finally a clear jet was found at the light bridge to trigger the filament eruption. We analyzed the evolutions of the relative darkness of the filament and the loaded mass by the continuous surges quantitatively. It was found that as the occurrence of the surges, the relative darkness of the filament body continued growing for about 3-4 hr, reached its maximum, and kept stable for more than 2 hr until it erupted. If suppose 50% of the ejected mass by the surges could be trapped by the filament channel, then the total loaded mass into the filament channelwill be about 0.57x10(16) g with a momentum of 0.57x10(22) g cm s(-1) by 08:08 UT, which is a non-negligible effect on the stability of the filament. Based on the observations, we present a model showing the important role that recurrent chromospheric mass injection play in the evolution and eruption of a flux rope. Our study confirms that the surge activities can efficiently supply the necessary material for some filament formation. Furthermore, our study indicates that the continuous mass with momentum loaded by the surge activities to the filament channel could make the filament unstable and cause it to erupt. |
| 项目资助者 | National Natural Science Foundation of China [10733020, 10911120051, 0911181001, 10933003] ; National Basic Research Program of China [2006CB806301] ; National Astronomical Observatories, Chinese Academy of Sciences |
| 语种 | 英语 |
| 学科领域 | Astronomy & Astrophysics |
| 文章类型 | Article |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000274848100007 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | X-RAY JETS ; H-ALPHA SURGES ; CORONAL MASS EJECTIONS ; MAGNETIC RECONNECTION ; ACTIVE REGION ; EMERGING FLUX ; TELESCOPE |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/7174 |
| 专题 | 选址与日冕观测组 |
| 通讯作者 | Guo, J (reprint author), Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China. |
| 作者单位 | 1.Key Laboratory of Solar Activity, National Astronomical Observatories, Beijing 100012, China 2.Yunnan Astronomical Observatory, National Astronomical Observatories, Kunming 650011, China |
| 推荐引用方式 GB/T 7714 | Guo, J,Liu Y,Zhang, HQ,et al. A FLUX ROPE ERUPTION TRIGGERED BY JETS[J]. ASTROPHYSICAL JOURNAL,2010,711(2):1057-1061. |
| APA | Guo, J.,Liu Y.,Zhang, HQ.,Deng, YY.,Lin, JB.,...&Guo, J .(2010).A FLUX ROPE ERUPTION TRIGGERED BY JETS.ASTROPHYSICAL JOURNAL,711(2),1057-1061. |
| MLA | Guo, J,et al."A FLUX ROPE ERUPTION TRIGGERED BY JETS".ASTROPHYSICAL JOURNAL 711.2(2010):1057-1061. |
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| A FLUX ROPE ERUPTION（1058KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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