NAOC Open IR
太阳分米波尖峰辐射最小带宽的探讨
汪敏1; 王昆山2; 许春1; 施硕彪1; 李维华1
2003
Source Publication云南天文台台刊
ISSN1001-7526
Volume000Issue:002Pages:29
Abstract云南天文台0.6~1.5GHz太阳射电快速动态频谱仪,在2001年6月24日的射电爆发中观测到大量尖峰。由于观测仪器有相当高的频率分辨率,使我们可以对尖峰的绝对带宽进行更精细的统计分析。由于尖峰数量很大,特别编制了识别尖峰并测量其带宽的软件来进行统计工作。结果发现76%的尖峰的绝对带宽达到仪器频率分辨率1.4MHz,其相对带宽达到0.1%。这比以前关于尖峰辐射带宽的统计结果要小很多。统计结果支持用ECM机制解释尖峰辐射。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46906
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.云南省计算中心
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
汪敏,王昆山,许春,等. 太阳分米波尖峰辐射最小带宽的探讨[J]. 云南天文台台刊,2003,000(002):29.
APA 汪敏,王昆山,许春,施硕彪,&李维华.(2003).太阳分米波尖峰辐射最小带宽的探讨.云南天文台台刊,000(002),29.
MLA 汪敏,et al."太阳分米波尖峰辐射最小带宽的探讨".云南天文台台刊 000.002(2003):29.
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