NAOC Open IR
太阳存在脉动不稳定的低球谐阶p1模吗?
熊大闰1; 邓李才2
2012
Source Publication天文学报
ISSN0001-5245
Volume053Issue:006Pages:500
Abstract利用一种非局部和非定常的恒星对流理论,计算了太阳中低球谐阶(?〈25)模的非绝热脉动.结果表明,低阶(0〈f〈6)非径向p1模是脉动不稳定的,而与之相邻的g模、f模和p2.p5模都是脉动稳定的.根据累积功图的分析,发现振荡的激发来自对流区底部区域.太阳是否存在不稳定的低球谐阶p1模对判断太阳5min振荡的激发机制有重要意义.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/41897
Collection中国科学院国家天文台
Affiliation1.中国科学院紫金山天文台
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
熊大闰,邓李才. 太阳存在脉动不稳定的低球谐阶p1模吗?[J]. 天文学报,2012,053(006):500.
APA 熊大闰,&邓李才.(2012).太阳存在脉动不稳定的低球谐阶p1模吗?.天文学报,053(006),500.
MLA 熊大闰,et al."太阳存在脉动不稳定的低球谐阶p1模吗?".天文学报 053.006(2012):500.
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