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Direct observations of the magnetic reconnection site of an eruption on 2003 November 18
文献类型：期刊论文
| 作者 | Lin, J1 ; Ko, YK1; Sui, L2; Raymond, JC1; Stenborg, GA2; Jiang YC(姜云春)3; Zhao, S3; Mancuso, S1,4
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2005-04-01 |
| 卷号 | 622期号:2页码:1251-1264 |
| 关键词 | Sun : coronal mass ejections (CMEs) Sun : flares Sun : magnetic fields |
| ISSN号 | 0004-637X |
| 产权排序 | 第三完成单位 |
| 通讯作者 | Lin, J (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. |
| 英文摘要 | We report direct observations of the magnetic reconnection site during an eruptive process that occurred on 2003 November 18. The event started with a rapid expansion of a few magnetic arcades located over the east limb of the Sun and developed an energetic partial-halo coronal mass ejection (CME), a long current sheet, and a group of bright flare loops in the wake of the CME. It was observed by several instruments, both in space and on the ground, including the EUV Imaging Telescope, Ultraviolet Coronagraph Spectrometer, and Large Angle Spectrometric Coronagraph experiment on board the Solar and Heliospheric Observatory, the Reuven Ramaty High Energy Solar Spectroscopic Imager, and the Mauna Loa Solar Observatory Mark IV K-Coronameter. We combine the data from these instruments to investigate various properties of the eruptive process, including those around the current sheet. The maximum velocities of the CME leading edge and the core were 1939 and 1484 km s(-1), respectively. The average reconnection inflow velocities near the current sheet over different time intervals ranged from 10.5 to 106 km s(-1), and the average outflow velocities ranged from 460 to 1075 km s(-1). This leads to a corresponding rate of reconnection in terms of the Alfven Mach number MA ranging from 0.01 to 0.23. The composite of images from different instruments specifies explicitly how the different objects developed by a single eruptive process are related to one another. |
| 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] | CORONAL MASS EJECTIONS ; CURRENT SHEET ; SOLAR-FLARES ; FLUX ROPES ; FIELD ; EVOLUTION ; RHESSI ; MOTION ; LOOPS |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/0004-637X/622/2/1251/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000228093400044 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6076]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 作者单位 | 1.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 2.Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064 3.Yunnan Observatory, National Astronomical Observatories, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, China 4.Osservatorio Astronomico di Torino, INAF, 20 Strada Osservatorio, I-10025 Pino Torinese, Italy |
| 推荐引用方式 GB/T 7714 | Lin, J,Ko, YK,Sui, L,et al. Direct observations of the magnetic reconnection site of an eruption on 2003 November 18[J]. ASTROPHYSICAL JOURNAL,2005,622(2):1251-1264. |
| APA | Lin, J.,Ko, YK.,Sui, L.,Raymond, JC.,Stenborg, GA.,...&Mancuso, S.(2005).Direct observations of the magnetic reconnection site of an eruption on 2003 November 18.ASTROPHYSICAL JOURNAL,622(2),1251-1264. |
| MLA | Lin, J,et al."Direct observations of the magnetic reconnection site of an eruption on 2003 November 18".ASTROPHYSICAL JOURNAL 622.2(2005):1251-1264. |
入库方式： OAI收割
来源：云南天文台
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