LIMITS ON THE SUNS CORE MAGNETISM FROM SOLAR OSCILLATIONS

被引：8

作者：

DZIEMBOWSKI, W

GOODE, PR

机构：

[1] UNIV ARIZONA,ARIZONA RES LABS,TUCSON,AZ 85721

[2] UNIV ARIZONA,DEPT PHYS,TUCSON,AZ 85721

来源：

NATURE | 1983年 / 305卷 / 5929期

关键词：

D O I：

10.1038/305039a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

引用

页码：39 / 42

页数：4

共 10 条

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[2]

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[3] THE 5-MIN OSCILLATIONS OF THE SUN ARE INCOMPATIBLE WITH A RAPIDLY-ROTATING CORE [J].

DICKE, RH .

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[4]

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[5]

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[7] EVIDENCE FOR AN OBLIQUE MAGNETIC SOLAR ROTATOR [J].

GOUGH, DO .

NATURE, 1982, 298 (5872) :350-354

[8] PRELIMINARY DETERMINATION OF THE SUNS GRAVITATIONAL QUADRUPOLE-MOMENT FROM ROTATIONAL SPLITTING OF GLOBAL OSCILLATIONS AND ITS RELEVANCE TO TESTS OF GENERAL-RELATIVITY [J].

HILL, HA ;

BOS, RJ ;

GOODE, PR .

PHYSICAL REVIEW LETTERS, 1982, 49 (24) :1794-1797

[9] MODELS OF ROTATING MAGNETIC STARS [J].

MESTEL, L ;

MOSS, DL .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1977, 178 (01) :27-49

[10]

ULRICH RK, 1982, PREPRINT U CALIFORNI

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