Magnetoconvection and the Solar Dynamo

Journal of astrophysics and astronomy

Ã…. Nordlund1²  R. F. Stein3¹  S. B. F. Dorch2³ 

[1]Dept. of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA$$

[2]Astronomical Observatory & Theoretical Astrophysics Center, Juliane Maries Vej 30, 2100 Copenhagen ɸ, Denmark$$

[3]The Royal Swedish Academy of Sciences, Stockholm Observatory, SE-13336 Saltsjöbaden, Sweden$$

关键词: Magnetic fields;    convection;    dynamo;    Sun.;   

DOI  :  

学科分类：天文学(综合)

来源: Indian Academy of Sciences

【 摘 要 】

We review current understanding of the interaction of magnetic fields with convective motions in stellar convection zones. Among the most exciting recent results is the discovery that magnetic fields need not primarily be confined to the stable layer below the convection zone; numerical simulations have shown that surprisingly, strong magnetic fields can be maintained in the interior of the convection zone.

【 授权许可】

Unknown