THE SOLAR INTERIOR

被引：164

作者：

TURCKCHIEZE, S

DAPPEN, W

FOSSAT, E

PROVOST, J

SCHATZMAN, E

VIGNAUD, D

机构：

[1] UNIV SO CALIF, DEPT ASTRON, LOS ANGELES, CA 90089 USA

[2] UNIV NICE, DEPT ASTROPHYS, NICE 06, FRANCE

[3] OBSERV NICE, F-06304 NICE 04, FRANCE

[4] OBSERV MEUDON, DASGAL, F-92195 MEUDON, FRANCE

[5] CE SACLAY, SERV PHYS PARTICULES, DAPNIA, F-91191 GIF SUR YVETTE, FRANCE

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 1993年 / 230卷 / 2-4期

关键词：

D O I：

10.1016/0370-1573(93)90020-E

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

This report confronts the different aspects of the solar interior from the experimental and theoretical points of view, discussing photospheric abundances, neutrinos and acoustic mode measurements. The theoretical approach mainly concerns the classical framework of stellar evolution, nevertheless, particle interpretation of the data and astrophysical solutions invoked in the last 10 years are coherently examined.

引用

收藏

页码：57 / 235

页数：179

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