A brief history of the solar oblateness. A review

被引：30

作者：

Damiani, C. ^{[2
]}

Rozelot, J. P. ^{[1
]}

Lefebvre, S. ^{[3
,4
,5
]}

Kilcik, A. ^{[6
,7
]}

Kosovichev, A. G. ^{[8
]}

机构：

[1] Univ Nice, Fizeau OCA Dpt, CNRS, UMR6525, F-06130 Grasse, France

[2] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy

[3] Univ Versailles St Quentin, F-75252 Paris 05, France

[4] Univ Paris 06, F-75252 Paris 05, France

[5] IPSL, CNRS, INSU, LATMOS, F-75252 Paris 05, France

[6] Bogazici Univ, Kandilli Observ, Istanbul, Turkey

[7] Earthquake Res Inst, Istanbul, Turkey

[8] Stanford Univ, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA

来源：

JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS | 2011年 / 73卷 / 2-3期

关键词：

Sun: characteristic and properties; Solar physics; Solar activity; Solar interior; Relativistic astrophysics; QUADRUPOLE-MOMENT; SUN; FIGURE; DIAMETER; SURFACE; VARIABILITY; ROTATION; ASTROLABE;

D O I：

10.1016/j.jastp.2010.02.021

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

We hereby present a review on solar oblateness measurements. By emphasizing historical data, we illustrate how the discordance between experimental results can lead to substantial improvements in the building of new technical apparatus as well as to the emergence of new ideas to develop new theories. We stress out the need to get accurate data from space to enhance our knowledge of the solar core in order to develop more precise ephemerids and ultimately build possible new gravitational theories. (C) 2010 Elsevier Ltd. All rights reserved.

引用

页码：241 / 250

页数：10

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