Why Does the Sun's Torsional Oscillation Begin before the Sunspot Cycle?

被引:26
作者
Chakraborty, Sagar [1 ]
Choudhuri, Arnab Rai [2 ]
Chatterjee, Piyali [2 ]
机构
[1] SN Bose Ctr Basic Sci, Dept Theoret Sci, Kolkata 700098, India
[2] Indian Inst Sci, Dept Phys, Bangalore 560012, Karnataka, India
关键词
SOLAR CONVECTION-ZONE; MERIDIONAL CIRCULATION; DYNAMO MODEL; DIFFERENTIAL ROTATION; FLUX TUBES; FLOWS; PENETRATION; SURFACE; REGIONS; FORCE;
D O I
10.1103/PhysRevLett.102.041102
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Although the Sun's torsional oscillation is believed to be driven by the Lorentz force associated with the sunspot cycle, this oscillation begins 2-3 yr before the sunspot cycle. We provide a theoretical explanation of this with the help of a solar dynamo model having a meridional circulation penetrating slightly below the bottom of the convection zone, because only in such dynamo models does the strong toroidal field form a few years before the sunspot cycle and at a higher latitude.
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页数:4
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