NAOC Open IR
乌鲁木齐天文站的耀斑预报
宋淑敏
1999
Source Publication紫金山天文台台刊
ISSN1000-3681
Volume018Issue:002Pages:154
Abstract鉴于预报太阳耀斑的重要性和难度,我们在文中介绍了怎样用太阳色球望远镜观测太阳色球层的耀斑先兆(现象),并且根据太阳活动特点和十几年的观察经验及观测资料,综合分析,判断出太阳色球耀斑将要产生的大概时间,大致规模及耀斑在日面上的可能位置。通过第22周峰年资料验证,准确率可达70%。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51456
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
宋淑敏. 乌鲁木齐天文站的耀斑预报[J]. 紫金山天文台台刊,1999,018(002):154.
APA 宋淑敏.(1999).乌鲁木齐天文站的耀斑预报.紫金山天文台台刊,018(002),154.
MLA 宋淑敏."乌鲁木齐天文站的耀斑预报".紫金山天文台台刊 018.002(1999):154.
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