| 从太阳硬X射线和微波爆发频谱推断总电子数 |
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| 引用本文： | 于兴凤,姚金兴.从太阳硬X射线和微波爆发频谱推断总电子数[J].中国天文和天体物理学报,1999(1). |
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| 作者姓名： | 于兴凤 姚金兴 |
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| 作者单位： | 中国科学院紫金金山天文台 |
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| 基金项目： | 国家自然科学重点基金,江苏省基金 |
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| 摘 要： | 用非均匀模型，对１９８１年４月２７日０８００１Ｔ大耀斑进行了分析。从硬Ｘ射线和微波爆发的观测频谱出发，在假定周围离子密度ｎｉ＝３×１０１０／ｃｍ３的情况下，计算得到两者的总电子数ＮＸ和ＮＲ是近似相等的。这表明，至少对这个耀斑，两者的非热电子可能有同样的分布。此外，文中也分析了ＮＲ提高了１０３－１０４倍的原因可能在于磁场的非均匀性和源中的磁场值较小。
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| 关 键 词： | 太阳耀斑─硬X射线─微波爆发频谱─非热电子数 |
Electron Numbers Inferred from Solar Microwave andX-ray Bursts |
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| YU Xing-feng, YAO Jin-xing.Electron Numbers Inferred from Solar Microwave andX-ray Bursts[J].Chinese Journal of Astronomy and Astrophysics,1999(1). |
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| Authors: | YU Xing-feng YAO Jin-xing |
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| Abstract: | The question of whether the numbers of X-ray and radio-producing electrons in solar flares are the same has been discussed in this paper. Calculation shows that the number of radio-producing electrons NR estimated with nonhomogeneous radio source is approximately equal to the number of X-ray-producing electrons NX for the 1981 April 27 flare. It seems that they have a common population. In addition, the causes of NR increased by a factor of 103 - 104 have been analysed. |
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| Keywords: | Sun - solar microwave - X-ray bursts |
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