The 'standard' Sun -: Modelling and helioseismology

被引：43

作者：

Christensen-Dalsgaard, J ^{[1
]}

机构：

[1] Aarhus Univ, Inst Fys & Astron, DK-8000 Aarhus C, Denmark

[2] Danmarks Grundforskningsfond, Teoretisk Astrofys Ctr, DK-8000 Aarhus C, Denmark

来源：

SPACE SCIENCE REVIEWS | 1998年 / 85卷 / 1-2期

关键词：

Sun; structure; composition; helioseismology;

D O I：

10.1023/A:1005116132024

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 'standard' solar model is based on a number of simplifying assumptions and depends on knowledge of the physical properties of matter in the Sun. Given these assumptions, the constraint that the model have the observed surface luminosity provides an estimate of the initial solar helium abundance. From helioseismic analyses further information can be obtained about the present composition, including a fairly precise measure of the envelope helium abundance and an estimate of the hydrogen profile in the radiative interior. It must be emphasized, however, that these inferences may suffer from systematic error arising from incomplete knowledge about the equation of state and opacity of the solar interior.

引用

页码：19 / 36

页数：18

共 50 条

[21]

DAPPEN W, 1986, SEISMOLOGY SUN DISTA, P275

[22] A DISPERSION LAW FOR SOLAR OSCILLATIONS [J].

DUVALL, TL .

NATURE, 1982, 300 (5889) :242-243

[23]

DZIEMBOWSKI WA, 1990, MON NOT R ASTRON SOC, V244, P542

[24] HELIUM CONTENT IN THE SOLAR CONVECTIVE ENVELOPE FROM HELIOSEISMOLOGY [J].

DZIEMBOWSKI, WA ;

PAMYATNYKH, AA ;

SIENKIEWICZ, R .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1991, 249 (04) :602-605

[25]

ELLIOTT JR, 1998, UNPUB ASTROPHYS J

[26] SOLAR P-MODE FREQUENCIES AND THEIR DEPENDENCE ON SOLAR-ACTIVITY - RECENT RESULTS FROM THE BISON NETWORK [J].

ELSWORTH, Y ;

HOWE, R ;

ISAAK, GR ;

MCLEOD, CP ;

MILLER, BA ;

NEW, R ;

SPEAKE, CC ;

WHEELER, SJ .

ASTROPHYSICAL JOURNAL, 1994, 434 (02) :801-806

[27] SEISMIC OBSERVATIONS OF THE SOLAR INTERIOR [J].

GOUGH, D ;

TOOMRE, J .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1991, 29 :627-685

[28]

Gough D. O., 1984, Memorie della Societa Astronomica Italiana, V55, P13

[29] CALIBRATION OF STELLAR CONVECTION THEORIES [J].

GOUGH, DO ;

WEISS, NO .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 176 (03) :589-607

[30] The seismic structure of the sun [J].

Gough, DO ;

Kosovichev, AG ;

Toomre, J ;

Anderson, E ;

Antia, HM ;

Basu, S ;

Chaboyer, B ;

Chitre, SM ;

ChristensenDalsgaard, J ;

Dziembowski, WA ;

EffDarwich, A ;

Elliott, JR ;

Giles, PM ;

Goode, PR ;

Guzik, JA ;

Harvey, JW ;

Hill, F ;

Leibacher, JW ;

Monteiro, MJPFG ;

Richard, O ;

Sekii, T ;

Shibahashi, T ;

Takata, M ;

Thompson, MJ ;

Vauclair, S ;

Vorontsov, SV .

SCIENCE, 1996, 272 (5266) :1296-1300

← 1 2 3 4 5 →