Full sphere hydrodynamic and dynamo benchmarks

Convection in planetary cores can generate fluid flow and magnetic fields, and a number of sophisticated codes exist to simulate the dynamic behaviour of such systems. We report on the first community activity to compare numerical results of computer codes designed to calculate fluid flow within a w...

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Bibliographic Details
Published inGeophysical journal international Vol. 197; no. 1; pp. 119 - 134
Main Authors Marti, P., Schaeffer, N., Hollerbach, R., Cébron, D., Nore, C., Luddens, F., Guermond, J.-L., Aubert, J., Takehiro, S., Sasaki, Y., Hayashi, Y.-Y., Simitev, R., Busse, F., Vantieghem, S., Jackson, A.
Format Journal Article
LanguageEnglish
Published Oxford University Press 01.04.2014
Oxford University Press (OUP)
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