Source structures of the 1998 November 28 X-class flare and electron acceleration
文献类型：期刊论文
| 作者 | Huang, GL; Nakajima, H; Masuda, S; Kobayashi, K; Kubo, M |
| 刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
 |
| 出版日期 | 2006 |
| 卷号 | 58期号:1页码:37-45 |
| ISSN号 | 0004-6264 |
| 关键词 | sun : flares sun : radio radiation sun : X-rays, gamma rays |
| 英文摘要 | We studied the 1998 November 28 X-class flare, which showed long-duration, two-ribbon H alpha emission. (1) A soft X-ray loop system developed along the major magnetic neutral line in the impulsive phase. Hard X-ray and microwave emissions due to nonthermal electrons were located in some limited regions. While the compact hard X-ray loop was associated with weak, diffuse soft X-ray emission, two large microwave loops did not have soft X-ray counterparts. (2) Time profiles of two large microwave loops were similar to that of hard X-ray total emission, which emanated mostly from the compact Source, even in the fine time Structure in the rising phase. (3) A super-hot thermal hard X-ray source appeared around the impulsive peak and was located along the major magnetic neutral line in the declining phase, coinciding with the bright soft X-ray emission. The thermal component can be explained within the standard reconnection model to the extent that the super-hot thermal plasma was heated in the large soft X-ray loop. However, the nonthermal electrons were accelerated in a localized region where three loops interacted with each other. The inferred configuration may be a more complicated form of the double-loop interaction model proposed by Hanaoka (1996) and Nishio et al. (1997). |
| 学科主题 | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SOLAR-A MISSION ; MAGNETIC RECONNECTION ; RAY TELESCOPE ; MODEL ; YOHKOH ; LOOPS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000235849400006 |
| 公开日期 | 2012-02-07 |
| 源URL | [http://159.226.72.40/handle/332002/3516]  |
| 专题 | 紫金山天文台_太阳活动的多波段观测研究团组 |
| 作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 2.Natl Astron Observ, Nagano 3841305, Japan 3.Nagoya Univ, Solar Terrestrial Environm Lab, Aichi 4428507, Japan 4.NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA 5.Univ Tokyo, Dept Astron, Tokyo 1130033, Japan |
| 推荐引用方式 GB/T 7714 | Huang, GL,Nakajima, H,Masuda, S,et al. Source structures of the 1998 November 28 X-class flare and electron acceleration[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2006,58(1):37-45. |
| APA | Huang, GL,Nakajima, H,Masuda, S,Kobayashi, K,&Kubo, M.(2006).Source structures of the 1998 November 28 X-class flare and electron acceleration.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,58(1),37-45. |
| MLA | Huang, GL,et al."Source structures of the 1998 November 28 X-class flare and electron acceleration".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 58.1(2006):37-45. |
入库方式： OAI收割
来源：紫金山天文台
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