OBLATENESS OF THE SUN IN 1983 AND RELATIVITY

被引：22

作者：

DICKE, RH

KUHN, JR

LIBBRECHT, KG

机构：

来源：

NATURE | 1985年 / 316卷 / 6030期

关键词：

D O I：

10.1038/316687a0

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：687 / 690

页数：4

共 18 条

[1]

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DICKE, RH ;

GOLDENBERG, HM .

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[4] DO SOLAR-TYPE STARS HAVE MAGNETIC CORES QUESTIONABLE QUESTION OF STABILITY [J].

DICKE, RH .

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[5]

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[6] SOLAR OBLATENESS AND GRAVITATIONAL QUADRUPOLE MOMENT [J].

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[7] FACULAR INFLUENCES ON THE APPARENT SOLAR SHAPE [J].

DICKE, RH ;

KUHN, JR ;

LIBBRECHT, KG .

NATURE, 1983, 304 (5924) :326-328

[8] OBLATENESS OF SUN [J].

DICKE, RH ;

GOLDENBERG, HM .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1974, 27 :131-182

[9] 12.2 DAY SOLAR ROTATIONAL PERIOD [J].

DICKE, RH .

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[10]

DICKE RH, 1979, NEW SCI, V83, P12

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