| 3厘米波段太阳射电爆发中精细结构的特征 |
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| 引用本文： | 秦志海,黄光力,姚骑均.3厘米波段太阳射电爆发中精细结构的特征[J].天文学报,1997(1). |
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| 作者姓名： | 秦志海 黄光力 姚骑均 |
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| 作者单位： | 南京大学天文系!南京，210093，中国科学院紫金山天文台!南京，210008，中国科学院紫金山天文台!南京，210008 |
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| 摘 要： | 本文扼要介绍南京大学天文系3厘米波段在1989－1992年间观测射电精细结构的结果，指出该波段存在三种类型的精细结构，并简要讨论它们可能的产生机制．
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| 关 键 词： | 太阳 射电爆发 精细结构 |
CHARACTERISTICS OF THE FINE STRUCTURES IN SOLAR RADIO BURSTS AT 3.2cm |
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| Qin Zhi-hai.CHARACTERISTICS OF THE FINE STRUCTURES IN SOLAR RADIO BURSTS AT 3.2cm[J].Acta Astronomica Sinica,1997(1). |
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| Authors: | Qin Zhi-hai |
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| Abstract: | The obanahonal results of the fine structures in solar radio bursts at 3.2cm by the Observatory of the department of Astronomy of Nanjing University from 1989 to 1992are investigated in this paper.Three kinds of the fine structures in this waveband have been found.Some mechanisms for interpretation have been proposed. |
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| Keywords: | Sun Radio burst Fine structure |
| 本文献已被 CNKI 等数据库收录！ |
