HELIUM CONTENT IN THE SOLAR CONVECTIVE ENVELOPE FROM HELIOSEISMOLOGY

被引：54

作者：

DZIEMBOWSKI, WA ^{[1
]}

PAMYATNYKH, AA ^{[1
]}

SIENKIEWICZ, R ^{[1
]}

机构：

[1] MOSCOW ASTRON COUNCIL,MOSCOW 109017,USSR

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1991年 / 249卷 / 04期

关键词：

D O I：

10.1093/mnras/249.4.602

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using measured frequencies of the solar p-modes we determined the fractional mass content of helium in the Sun's envelope. We found that its value lies between 0.23 and 0.24. This result appears to be unaffected by the uncertainties in the treatment of the atmosphere and the outer convective zone, but it relies in a sensitive way on calculation of thermodynamical quantities.

引用

页码：602 / 605

页数：4

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