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A numerical dynamo benchmark

被引：246
作者：
Christensen, UR
Aubert, J
Cardin, P
Dormy, E
Gibbons, S
Glatzmaier, GA
Grote, E
Honkura, Y
Jones, C
Kono, M
Matsushima, M
Sakuraba, A
Takahashi, F
Tilgner, A
Wicht, J
Zhang, K
机构：
[1] Univ Gottingen, Inst Geophys, D-37075 Gottingen, Germany
[2] Univ Grenoble, Observ Sci, LGIT, F-38041 Grenoble 09, France
[3] Inst Phys Globe, F-75252 Paris 05, France
[4] Univ Exeter, Dept Math, Exeter EX4 4QE, Devon, England
[5] Univ Calif Santa Cruz, Earth Sci Dept, Santa Cruz, CA 95064 USA
[6] Univ Bayreuth, D-95440 Bayreuth, Germany
[7] Tokyo Inst Technol, Dept Earth & Planetary Sci, Meguro Ku, Tokyo 1528551, Japan
[8] Okayama Univ, Inst Study Earths Interior, Misasa, Tottori 6820193, Japan
[9] Univ Tokyo, Dept Earth & Planetary Sci, Bunkyo Ku, Tokyo 1130033, Japan
来源：
PHYSICS OF THE EARTH AND PLANETARY INTERIORS | 2001年 / 128卷 / 1-4期
关键词：
geodynamo; numerical modeling;
D O I：
10.1016/S0031-9201(01)00275-8
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
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.
引用
收藏
页码：25 / 34
页数：10
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