期刊
PHYSICS OF THE EARTH AND PLANETARY INTERIORS
卷 128, 期 1-4, 页码 25-34出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/S0031-9201(01)00275-8
关键词
geodynamo; numerical modeling
We present the results of a benchmark study for a convection-driven magnetohydrodynamic dynamo problem in a rotating spherical shell. The solutions are stationary aside from azimuthal drift. One case of non-magnetic convection and two dynamos that differ in the assumptions concerning the inner core are studied. Six groups contributed numerical solutions which show good agreement. This provides an accurate reference standard with high confidence. (C) 2001 Elsevier Science B.V. All rights reserved.
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