Global seismology of the Sun

被引：100

作者：

Basu, Sarbani ^{[1
]}

机构：

[1] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA

来源：

LIVING REVIEWS IN SOLAR PHYSICS | 2016年 / 13卷

关键词：

Sun: interior; Sun: helioseismology; Sun: rotations; Stars: asteroseismology; SOLAR-LIKE OSCILLATIONS; EQUATION-OF-STATE; P-MODE FREQUENCIES; MICHELSON DOPPLER IMAGER; NONASYMPTOTIC HELIOSEISMIC INVERSION; STELLAR ACOUSTIC-OSCILLATIONS; RADIAL DIFFERENTIAL ROTATION; CONVECTION-ZONE DYNAMICS; TOROIDAL MAGNETIC-FIELD; CHEMICAL-COMPOSITION;

D O I：

10.1007/s41116-016-0003-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The seismic study of the Sun and other stars offers a unique window into the interior of these stars. Thanks to helioseismology, we know the structure of the Sun to admirable precision. In fact, our knowledge is good enough to use the Sun as a laboratory. We have also been able to study the dynamics of the Sun in great detail. Helioseismic data also allow us to probe the changes that take place in the Sun as solar activity waxes and wanes. The seismic study of stars other than the Sun is a fairly new endeavour, but we are making great strides in this field. In this review I discuss some of the techniques used in helioseismic analyses and the results obtained using those techniques. I focus on results obtained with global helioseismology, i.e., the study of the Sun using its normal modes of oscillation. I also briefly touch upon asteroseismology, the seismic study of stars other than the Sun, and discuss how seismic data of others stars are interpreted.

引用

页数：126

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