A numerical dynamo benchmark

by: UR Christensen, J Aubert, P Cardin, E Dormy, S Gibbons, GA Glatzmaier, E Grote, Y Honkura, C Jones, M Kono, M Matsushima, A Sakuraba, F Takahashi, A Tilgner, J Wicht, K Zhang

Physics of The Earth and Planetary Interiors, Vol. 128, No. 1-4. (10 December 2001), pp. 25-34.

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Abstract

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.

@article{citeulike:2745778, abstract = {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.}, author = {Christensen, U. R. and Aubert, J. and Cardin, P. and Dormy, E. and Gibbons, S. and Glatzmaier, G. A. and Grote, E. and Honkura, Y. and Jones, C. and Kono, M. and Matsushima, M. and Sakuraba, A. and Takahashi, F. and Tilgner, A. and Wicht, J. and Zhang, K. }, citeulike-article-id = {2745778}, doi = {10.1016/S0031-9201(01)00275-8}, journal = {Physics of The Earth and Planetary Interiors}, keywords = {dynamo}, month = {December}, number = {1-4}, pages = {25--34}, posted-at = {2008-05-02 14:23:29}, priority = {2}, title = {A numerical dynamo benchmark}, url = {http://dx.doi.org/10.1016/S0031-9201(01)00275-8}, volume = {128}, year = {2001} }

RIS record

TY - JOUR ID - citeulike:2745778 L3 - citeulike-article-id:2745778 TI - A numerical dynamo benchmark JF - Physics of The Earth and Planetary Interiors VL - 128 IS - 1-4 SP - 25 EP - 34 N2 - 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. KW - dynamo AU - Christensen, UR AU - Aubert, J AU - Cardin, P AU - Dormy, E AU - Gibbons, S AU - Glatzmaier, GA AU - Grote, E AU - Honkura, Y AU - Jones, C AU - Kono, M AU - Matsushima, M AU - Sakuraba, A AU - Takahashi, F AU - Tilgner, A AU - Wicht, J AU - Zhang, K PY - 2001/12/10/ UR - http://dx.doi.org/10.1016/S0031-9201(01)00275-8 ER -

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