Does the tachocline show solar cycle related changes?

被引：11

作者：

Basu, S

Schou, J

机构：

[1] Inst Adv Study, Princeton, NJ 08540 USA

[2] Yale Univ, Dept Astron, New Haven, CT 06520 USA

[3] Stanford Univ, Stanford, CA 94305 USA

来源：

SOLAR PHYSICS | 2000年 / 192卷 / 1-2期

关键词：

D O I：

10.1023/A:1005231509224

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The tachocline at the base of the convection zone is generally believed to be the seat of the solar dynamo. Here we investigate whether the tachocline shows any detectable change using several 72 day time-series of the Michelson Doppler Imager (MDI) Medium-l data. We do not find any clear evidence of change with time.

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页码：481 / 486

页数：6

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