Comments on "Full-sphere simulations of circulation-dominated solar dynamo: Exploring the parity issue"

被引:12
作者
Dikpati, M [1 ]
Rempel, M [1 ]
Gilman, PA [1 ]
MacGregor, KB [1 ]
机构
[1] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
关键词
sun : magnetic fields; methods : numerical;
D O I
10.1051/0004-6361:20042435
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using two distinct simulation codes that respectively apply semi-implicit and fully explicit schemes, we perform calculations of a 2D kinematic Babcock-Leighton type flux-transport dynamo with Chatterjee et al.'s parameter settings. We show that their solutions are diffusion-dominated, rather than circulation-dominated as their title implies. We also have been unable to reproduce several properties of their dynamo solutions, namely we obtain a much faster cycle with similar to 4 times shorter period than theirs, with highly overlapping cycles; a polar field value of similar to 2 kG if one has to produce a similar to 100 kG toroidal field at convection zone base; and quadrupolar parity as opposed to Chatterjee et al.'s dipolar parity solutions.
引用
收藏
页码:699 / 702
页数:4
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