NAOC Open IR
类太阳恒星耀斑光变轮廓特征分析
云多; 王华宁; 贺晗
2016
Source Publication天文学报
ISSN0001-5245
Volume057Issue:001Pages:9
Abstract太阳耀斑是由于在太阳黑子附近磁场能量的突然释放所引起的爆发现象.人们发现在许多类太阳恒星上也有类似的耀斑(称类太阳恒星耀斑)出现.主要采用开普勒太空望远镜获取的数据,从中选取SC(Short Cadence)数据进行分析,找出类太阳恒星上耀斑光变轮廓的特征参数并做统计,总结耀斑的活动特点.分析结果表明:类太阳恒星耀斑的光变轮廓和爆发的特征时间与太阳耀斑的相似,这可以说明两种耀斑的物理机制相同.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/44113
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
云多,王华宁,贺晗. 类太阳恒星耀斑光变轮廓特征分析[J]. 天文学报,2016,057(001):9.
APA 云多,王华宁,&贺晗.(2016).类太阳恒星耀斑光变轮廓特征分析.天文学报,057(001),9.
MLA 云多,et al."类太阳恒星耀斑光变轮廓特征分析".天文学报 057.001(2016):9.
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