The Long-term Dynamics of the Solar Radiative Zone: New Results from the Solar and Heliospheric Observatory (SoHO) and Young Solar Analogs

被引：0

作者：

Turck-Chieze, Sylvaine ^{[1
]}

Couvidat, Sebastien ^{[2
]}

Eff-Darwich, Antonio ^{[3
]}

Duez, Vincent ^{[4
]}

Garcia, Rafael A. ^{[1
]}

Mathis, Stephane ^{[1
]}

Mathur, Savita ^{[5
]}

Piau, Laurent ^{[6
]}

Salabert, David ^{[7
]}

机构：

[1] CE Saclay, CEA DSM IRFU SAp AIM, F-91191 Gif Sur Yvette, France

[2] Stanford Univ, W Hansen P L, Stanford, CA 94305 USA

[3] IAC, San Cristobal la Laguna, Spain

[4] Univ Bonn, Argelander Inst Astron, Bonn, Germany

[5] NCAR, High Altitude Observ, Boulder, CO 80307 USA

[6] LATMOS, Paris, France

[7] Univ Nice Sophia Antipolis, CNRS, Observ Cote dAzur, F-06304 Nice 4, France

来源：

PROGRESS IN SOLAR/STELLAR PHYSICS WITH HELIO- AND ASTEROSEISMOLOGY | 2012年 / 462卷

关键词：

MAGNETIC-FIELDS; OSCILLATIONS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Standard Solar Model (SSM) is no longer sufficient to interpret all the observations of the radiative zone obtained with the SoHO satellite. We recall our present knowledge of this internal region and compare recent results with models beyond the SSM assumptions. Then we discuss the missing processes and quantify some of them in using observations of young solar analogs to build a more realistic view of the Sun. This progress will be useful for understanding solar-like stars observed by CoRoT and Kepler.

引用

页码：366 / +

页数：2

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