Erratum to "A numerical dynamo benchmark" [Phys. Earth Planet. Int. 128 (1-4) (2001) 25-34] (DOI:10.1016/S0031-9201(01)00275-8);A numerical dynamo benchmark

Physics of the Earth and Planetary Interiors

Volumn 128, Issue 1-4, 2001, Pages 25-34

  Christensen, U R ^a   Aubert, J ^b   Cardin, P ^b   Dormy, E ^c   Gibbons, S ^d   Glatzmaier, G A ^e   Grote, E ^f   Honkura, Y ^g   Jones, C ^d   Kono, M ^h   Matsushima, M ^g   Sakuraba, A ⁱ   Takahashi, F ^g   Tilgner, A ^f   Wicht, J ^a   Zhang, K ^d  

^a UNIVERSITY OF GÖTTINGEN   (Germany)

^b OBSERVATOIRE DE GRENOBLE   (France)

^c INSTITUT DE PHYSIQUE DU GLOBE DE PARIS   (France)

^d UNIVERSITY OF EXETER   (United Kingdom)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f UNIVERSITY OF BAYREUTH   (Germany)

^g TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^h OKAYAMA UNIVERSITY   (Japan)

ⁱ UNIVERSITY OF TOKYO   (Japan)

Author keywords

Geodynamo; Numerical modeling

Indexed keywords

CONVECTION; GEODYNAMO; MAGNETOHYDRODYNAMICS; NUMERICAL MODEL;

EID: 6444245228     PISSN: 00319201     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pepi.2008.09.014     Document Type: Erratum

References (13)

1. On convection driven dynamos in rotating spherical shells
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3. Numerical modelling of the geodynamo: A systematic parameter study
4. MHD flow in a slightly differentially rotating spherical shell, with conducting inner core, in a dipolar magnetic field
5. Numerical simulations of stellar convective dynamos. I. The model and method
6. A three-dimensional convective dynamo solution with rotating and finitely conducting inner core and mantle
7. Regular and chaotic spherical dynamos
8. The complexity simulation group, computer simulation of a magnetohydrodynamic dynamo
9. Some characteristics of magnetic field behavior in a model of MHD dynamo thermally driven in a rotating spherical shell
10. An Earth-like numerical dynamo model
11. Effect of the inner core on the numerical solution of the magnetohydrodynamic dynamo
12. Spectral methods for the simulation of incompressible flow in spherical shells