Search for Structural Variations of the Near-Surface Layers of the Sun during the Solar Cycle

被引：0
|
作者：
Rabello-Soares, M. C. [1 ]
Korzennik, S. G. [2 ]
机构：
[1] Stanford Univ, HEPL, Stanford, CA 94305 USA
[2] Harvard Smithsonian CfA, Cambridge, MA USA
来源：
SOLAR-STELLAR DYNAMOS AS REVEALED BY HELIO AND ASTEROSEISMOLOGY: GONG 2008/SOHO 21 | 2009年 / 416卷
关键词：
RING-DIAGRAM ANALYSIS; STRUCTURE INVERSION; MODE FREQUENCIES; ACTIVE REGIONS; MDI; PARAMETERS; GONG;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Acoustic mode frequencies, with degree up to 900, observed by Michelson Doppler Imager (MDI) from 1995 to 2005 were analyzed to determine if there are any changes in the near-surface layers of the solar structure with the solar cycle. The inclusion of high-degree modes allowed the determination of the sound speed up to 0.993R(circle dot).
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页码：277 / +
页数：2
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