Studying magneto-convection by numerical simulation

被引:45
|
作者
Vögler, A [1 ]
Schüssler, M [1 ]
机构
[1] Max Planck Inst Aeronomie, D-37191 Katlenburg, Germany
关键词
sun; stars : magnetic fields; stars : activity; methods : numerical;
D O I
10.1002/asna.200310146
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Following a brief overview of the two main approaches to investigate the interaction between magnetic fields and convective flows near the solar surface layers by numerical simulation, namely idealized model problems and 'realistic' large-eddy simulations, we present first results obtained with a newly developed MHD code. The first example concerns the realistic simulation of the magnetic field dynamics in a solar plage region while the second example demonstrates small-scale dynamo action in idealized compressible convection.
引用
收藏
页码:399 / 404
页数:6
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