Observational features of large-scale structures as revealed by the catastrophe model of solar eruptions
文献类型：期刊论文
| 作者 | Lin J(林隽)1,2
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| 刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2007 |
| 卷号 | 7期号:4页码:457-476 |
| 关键词 | sun : large-scale magnetic structures sun : eruptive processes sun : theory and observations magnetic reconnection and current sheets |
| ISSN号 | 1009-9271 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Lin, J (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | Large-scale magnetic structures are the main carrier of major eruptions in the solar atmosphere. These structures are rooted in the photosphere and are driven by the unceasing motion of the photospheric material through a series of equilibrium configurations. The motion brings energy into the coronal magnetic field until the system ceases to be in equilibrium. The catastrophe theory for solar eruptions indicates that loss of mechanical equilibrium constitutes the main trigger mechanism of major eruptions, usually shown up as solar flares, eruptive prominences, and coronal mass ejections (CMEs). Magnetic reconnection which takes place at the very beginning of the eruption as a result of plasma instabilities/turbulence inside the current sheet, converts magnetic energy into heating and kinetic energy that are responsible for solar flares, and for accelerating both plasma ejecta (flows and CMEs) and energetic particles. Various manifestations are thus related to one another, and the physics behind these relationships is catastrophe and magnetic reconnection. This work reports on recent progress in both theoretical research and observations on eruptive phenomena showing the above manifestations. We start by displaying the properties of large-scale structures in the corona and the related magnetic fields prior to an eruption, and show various morphological features of the disrupting magnetic fields. Then, in the framework of the catastrophe theory, we look into the physics behind those features investigated in a succession of previous works, and discuss the approaches they used. |
| 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 ; II RADIO-BURSTS ; RECONNECTING CURRENT SHEETS ; MAGNETIC-FLUX TRANSPORT ; RAY FLARE EMISSION ; 2002 JULY 23 ; EMERGING FLUX ; ACTIVE REGIONS ; QUIESCENT PROMINENCES ; PARTICLE-ACCELERATION |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1009-9271/7/4/01/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000249365900001 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6113]  |
| 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 2.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA |
| 推荐引用方式 GB/T 7714 | Lin J. Observational features of large-scale structures as revealed by the catastrophe model of solar eruptions[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2007,7(4):457-476. |
| APA | Lin J.(2007).Observational features of large-scale structures as revealed by the catastrophe model of solar eruptions.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,7(4),457-476. |
| MLA | Lin J."Observational features of large-scale structures as revealed by the catastrophe model of solar eruptions".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 7.4(2007):457-476. |
入库方式： OAI收割
来源：云南天文台
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