NAOC Open IR
太阳耀斑的行星引潮力触发
董士化; 郑乐平
2001
Source Publication空间科学学报
ISSN0254-6124
Volume021Issue:001Pages:92
Abstract阐述了太阳潮波动力学的概况,依据实际资料的统计结果指出;行星引潮力触发耀斑的效应随耀斑级别的增大而增强;对于3级及其以上耀斑,强潮汐触发较之弱触发的耀斑产出率之比高达9.33;这个重要事实在预报地球和日地空间灾害性扰动方面,会有相当大的实际价值。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46838
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
董士化,郑乐平. 太阳耀斑的行星引潮力触发[J]. 空间科学学报,2001,021(001):92.
APA 董士化,&郑乐平.(2001).太阳耀斑的行星引潮力触发.空间科学学报,021(001),92.
MLA 董士化,et al."太阳耀斑的行星引潮力触发".空间科学学报 021.001(2001):92.
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