Drifting bands of solar radio spikes
文献类型：期刊论文
| 作者 | Xu FuYing1,2; Wu HongAo1,2 |
| 刊名 | CHINESE SCIENCE BULLETIN
 |
| 出版日期 | 2008-02-01 |
| 卷号 | 53期号:4页码:638-640 |
| 关键词 | sun solar microwave burst spike activity |
| ISSN号 | 1001-6538 |
| 英文摘要 | The solar flare (1N/C5.3) occurred in NOAA 8742 on October 27, 1999, and the accompanied complex radio burst was observed by the spectrometer with both high temporal (5 ms) and frequency (10 MHz) resolutions at Purple Mountain Observatory (PMO). It started at 04:27:42 UT, peaked at 04:28:42 UT and ended at 04:29:18 UT. The most significant feature of the event might be the sequential spikes in both time and frequency to form three slow drift bands over the frequency range of similar to 5 to >= 7.5 GHz with almost the same drift rate about 2.7 GHz/s. The relative bandwidth for the individual spikes varied from 1.6% to 4.9%, typically 3.3%. Based on electron cyclotron maser action driven by loss-cone anisotropy, the rare phenomena of slow drift band consisting of spikes were interpreted by spike source moving back and forth along the magnetic loop. Also, the estimations of the narrow bandwidths of spike given by electron cyclotron maser theory coincided well with the observations. |
| WOS标题词 | Science & Technology |
| 学科主题 | Astronomy & Astrophysics; Physics |
| 类目[WOS] | Multidisciplinary Sciences |
| 研究领域[WOS] | Science & Technology - Other Topics |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000252974500021 |
| 公开日期 | 2011-12-30 |
| 源URL | [http://159.226.72.40/handle/332002/2035]  |
| 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.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Xu FuYing,Wu HongAo. Drifting bands of solar radio spikes[J]. CHINESE SCIENCE BULLETIN,2008,53(4):638-640. |
| APA | Xu FuYing,&Wu HongAo.(2008).Drifting bands of solar radio spikes.CHINESE SCIENCE BULLETIN,53(4),638-640. |
| MLA | Xu FuYing,et al."Drifting bands of solar radio spikes".CHINESE SCIENCE BULLETIN 53.4(2008):638-640. |
入库方式： OAI收割
来源：紫金山天文台
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