Transition from axi- to nonaxisymmetric dynamo modes in spherical convection models of solar-like stars

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机构：
[1] Viviani, M.
[2] 1,Warnecke, J.
[3] 1,Käpylä, M.J.
[4] 1,2,3,Käpylä, P.J.
[5] Olspert, N.
[6] Cole-Kodikara, E.M.
[7] 1,Lehtinen, J.J.
[8] 4,6,7,Brandenburg, A.
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| 1600年 / EDP Sciences卷 / 616期
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All Open Access; Bronze; Green;
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摘要：
Magnetohydrodynamics
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