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太阳p模振动的激发机制
毕少兰; 李如凤
1998
Source Publication天体物理学报
ISSN0253-2379
Volume018Issue:001Pages:68
Abstract本文估计了激发单个太阳p模振动需要的能量输入率E≡ET,其中谱线宽度Г假设是振动模能量衰减率的观测值,在改进后的对流湍流三维时空分离描述的基础上,利用太阳对流区的混合长流模型计算了振动模的激发率,认为太阳P模振动主要是由雷诺应力扰动激发的,即P模激发对应着地流湍流运动引起声波发射,对于频率v〈3mHz,振动模的激发率为E∝v^7频率v〉3mHz,振动模的激发率为E∝v^-5,理论计算的振动能谱与观
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37566
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
毕少兰,李如凤. 太阳p模振动的激发机制[J]. 天体物理学报,1998,018(001):68.
APA 毕少兰,&李如凤.(1998).太阳p模振动的激发机制.天体物理学报,018(001),68.
MLA 毕少兰,et al."太阳p模振动的激发机制".天体物理学报 018.001(1998):68.
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