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.
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页码：27 / 48
页数：22
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