作者: Jörn Warnecke , Petri J Käpylä , MJ Mantere , Alel Brandenburg , None
DOI: 10.1017/S1743921313002676
关键词: Solar rotation 、 Dynamo 、 Differential rotation 、 Magnetohydrodynamics 、 Sunspot 、 Convection 、 Geophysics 、 Convection zone 、 Physics 、 Spherical wedge
摘要: We present results of convective turbulent dynamo simulations including a coronal layer in spherical wedge. find an equatorward migration the radial and azimuthal fields similar to behavior sunspots during solar cycle. The field coexist with spoke-like differential rotation anti-solar (clockwise) meridional circulation. Even though extends over whole convection zone, mechanism causing this is not yet fully understood.