Fluid dynamics and MHD of the solar convection zone and tachocline: Current understanding and unsolved problems - (Invited review)

被引：82

作者：

Gilman, PA ^{[1
]}

机构：

[1] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80301 USA

来源：

SOLAR PHYSICS | 2000年 / 192卷 / 1-2期

关键词：

D O I：

10.1023/A:1005280502744

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review recent progress and define unanswered scientific questions in five related topics: granulation- to supergranulation-scale convection and magnetic structures; global convection and circulation; the rise of magnetic flux tubes to the photosphere, and their injection into the base of the convection zone; tachocline fluid dynamics and MHD; and the solar dynamo. We close with a set of observational 'targets' for helioseismologists to aim for.

引用

页码：27 / 48

页数：22

共 78 条

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