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磁能和磁复杂性向日冕的传输
汪景
1995
Source Publication天体物理学报
ISSN0253-2379
Volume015Issue:003Pages:261
Abstract本文讨论了从太阳光球向日冕传输磁能和磁复杂性的过程。活动日冕,作为由电磁场和粒子组成的系统,其唯一的开场表面是太阳光球,光球层等离子体的运动和磁场的相互作用,是造成磁能和磁复杂性向日冕传输的主要根据;同时,光球上的耗散过程也对日冕磁能和磁复杂性的积累有不可忽视的贡献。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47416
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
汪景. 磁能和磁复杂性向日冕的传输[J]. 天体物理学报,1995,015(003):261.
APA 汪景.(1995).磁能和磁复杂性向日冕的传输.天体物理学报,015(003),261.
MLA 汪景."磁能和磁复杂性向日冕的传输".天体物理学报 015.003(1995):261.
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