硬X射线爆发的Hα特征 |
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引用本文: | 史忠先,汪景琇.硬X射线爆发的Hα特征[J].空间科学学报,1986,6(4):243-251. |
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作者姓名: | 史忠先 汪景琇 |
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作者单位: | 中国科学院北京天文台 |
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摘 要: | 对50个Ha耀斑检查表明:1.有硬X射线爆发(HXRBS)的耀斑,其Ha的线宽均超过4?,HXRBS对应的Ha耀斑核(在Ha+2?处,J耀斑核/I背景≥1.15)至少有两个,它们分处于磁场正负极性区;2.Ha耀斑开始较早, Ha耀斑核(kernel)的强度峰落后HXRBS的峰(spike)数秒,峰与峰之间有很好的对应关系; 3.Ha耀斑核,当HXRBS峰值计数率大于1000时,掩盖黑子半影,峰值计数率小于200时,不掩盖黑子半影。
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收稿时间: | 1986-01-08 |
The Ha Characteristics of Hard X-ray Bursts |
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Institution: | Beijing Astronomical Observatory, Academia Sinica |
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Abstract: | The following results are obtained from the examination of 50 Ha flares. (1) all flares with HXRBS are detectabe from the emission of Hα±2A. They have at least two Ha kernels (I flare/I bac. >1.15 on Hα + 2?) located in the opposite polarity regions; (2) the Ha brigh-tenings start earlier than HXRBS, while the Ha peaks, which correspond to the spikes of HXRBS very well, come later than that of HXRBS by several seconds; (3) if the count rates of HXRBS are more than 1000, the kernels of Hα+2A cover the penumbra, if the count rates are less than 200, the kernels do not cover the penumbra. |
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