Natural spectral bandwidth of electron cyclotron maser emission
文献类型：期刊论文
| 作者 | Fleishman, GD |
| 刊名 | ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS
 |
| 出版日期 | 2004-09-01 |
| 卷号 | 30期号:9页码:603-614 |
| 关键词 | Sun |
| ISSN号 | 1063-7737 |
| 英文摘要 | We studied the spectral properties of the electron cyclotron maser emission generated by anisotropic distributions of fast electrons with power-law Magnitude distributions in solar flares. The 19 natural bandwidth of the generated spectral line depends significantly on the angle between the direction of the wave emission and the direction of the magnetic field in the Source. In addition, the line bandwidth depends on the parameters of the momentum and pitch-angle distribution functions for fast electrons. The 14 typical spectral bandwidths are shown to lie within the range 0.1-0.4%, in agreement with the minimum observable bandwidths of millisecond solar radio spikes. (C) 2004 MAIK"Nauka/lnterperiodica". |
| 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] | AURORAL KILOMETRIC RADIATION ; MILLISECOND RADIO SPIKES ; LOSS-CONE ; WAVES |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000224036000003 |
| 公开日期 | 2012-12-22 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/7764]  |
| 专题 | 紫金山天文台_期刊（老文献） |
| 作者单位 | 1.Purple Mt Observ, Nanjing 210008, Peoples R China 2.Russian Acad Sci, AF Ioffe Physicotech Inst, St Petersburg 194021, Russia |
| 推荐引用方式 GB/T 7714 | Fleishman, GD. Natural spectral bandwidth of electron cyclotron maser emission[J]. ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS,2004,30(9):603-614. |
| APA | Fleishman, GD.(2004).Natural spectral bandwidth of electron cyclotron maser emission.ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS,30(9),603-614. |
| MLA | Fleishman, GD."Natural spectral bandwidth of electron cyclotron maser emission".ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS 30.9(2004):603-614. |
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来源：紫金山天文台
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