Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT
文献类型：期刊论文
| 作者 | Trottet, G.; Correia, E.; Karlicky, M.; Aulanier, G.; Yan, Y. ; Kaufmann, P.
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| 刊名 | SOLAR PHYSICS
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| 出版日期 | 2006-06-01 |
| 卷号 | 236期号:1页码:75-95 |
| 英文摘要 | This paper deals with a detailed analysis of spectral and imaging observations of the November 5, 1998 (H alpha 1B, GOES M1.5) flare obtained over a large spectral range, i.e., from hard X-rays to radiometric wavelengths. These observations allowed us to probe electron acceleration and transport over a large range of altitudes that is to say within small-scale (a few 10(3) km) and large-scale (a few 10(5) km) magnetic structures. The observations combined with potential and linear force-free magnetic field extrapolations allow us to show that: (i) Flare energy release and electron acceleration are basically driven by loop-loop interactions at two independent, low lying, null points of the active region magnetic field; (ii) < 300 keV hard X-ray-producing electrons are accelerated by a different process (probably DC field acceleration) than relativistic electrons that radiate the microwave emission; and (iii) although there is evidence that hard X-ray and decimetric/metric radio-emitting electrons are produced by the same accelerator, the present observations and analysis did not allow us to find a clear and direct magnetic connection between the hard X-ray emitting region and the radio-emitting sources in the middle corona. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000239087300005 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/7082]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | 1.Observ Paris, Sect Meudon, LESIA, F-92190 Meudon, France 2.Univ Presbiteriana Mackenzie, INPE, CRAAM, BR-01302907 Sao Paulo, Brazil 3.Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic 4.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Trottet, G.,Correia, E.,Karlicky, M.,et al. Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT[J]. SOLAR PHYSICS,2006,236(1):75-95. |
| APA | Trottet, G.,Correia, E.,Karlicky, M.,Aulanier, G.,Yan, Y.,&Kaufmann, P..(2006).Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT.SOLAR PHYSICS,236(1),75-95. |
| MLA | Trottet, G.,et al."Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT".SOLAR PHYSICS 236.1(2006):75-95. |
入库方式： OAI收割
来源：国家天文台
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