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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Published in | Geophysical journal international Vol. 197; no. 1; pp. 119 - 134 |
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Main Authors | , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Oxford University Press
01.04.2014
Oxford University Press (OUP) |
Subjects | |
Online Access | Get full text |
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