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太阳大气铍丰度的衰减
熊大闰; 邓李才
2003
Source Publication天文学报
ISSN0001-5245
Volume0Issue:1Pages:42006
AbstractLi和Be轻元素在温度仅几百万度时就因核反应而遭毁坏,因此它们是恒星演化过程的外层对流混合延伸程度很好的一种示踪。基于这种考虑,我们曾计算过太阳包层模型Li的衰减,得到一个同时满足日震学太阳对流区深度和太阳Li丰度观测要求的非局部太阳对流包层模型[1].Li丰度给出了一个非局部对流混合延伸程度的上限。
Keyword太阳 丰度 恒星 丰度 对流
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11153
Collection院士文集_熊大闰
Recommended Citation
GB/T 7714
熊大闰,邓李才. 太阳大气铍丰度的衰减[J]. 天文学报,2003,0(1):42006.
APA 熊大闰,&邓李才.(2003).太阳大气铍丰度的衰减.天文学报,0(1),42006.
MLA 熊大闰,et al."太阳大气铍丰度的衰减".天文学报 0.1(2003):42006.
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