The Sun as a Climate Driver: Modelling the Variability of the Solar Interior Structure

被引:0
|
作者
Spada, F. [1 ]
Li, L. H. [1 ]
Sofia, S. [1 ]
Ventura, P. [2 ]
机构
[1] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA
[2] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
来源
ADVANCES IN COMPUTATIONAL ASTROPHYSICS: METHODS, TOOLS AND OUTCOMES | 2012年 / 453卷
关键词
STELLAR EVOLUTION CODE; ROTATION; STARS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The interior of the Sun undergoes variations on intermediate time scales (i.e. years or longer), which affect the luminosity output and the total amount of radiation received by the Earth (the Total Solar Irradiance, or TSI). Modelling these variations is currently beyond the capabilities of conventional stellar codes. The main goal of this project is to put meaningful constraints on the effect of the solar variability on climate change.
引用
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页码:395 / +
页数:2
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