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Effect of shear and magnetic field on the heat transfer efficiency of convection in rotating spherical shells

MPS-Authors
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Yadav,  R. K.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Gastine,  T.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Christensen,  U. R.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Yadav, R. K., Gastine, T., Christensen, U. R., Duarte, L., V., D., & Reiners, A. (2016). Effect of shear and magnetic field on the heat transfer efficiency of convection in rotating spherical shells. Geophysical Journal International, 204, 1120-1133. doi:10.1093/gji/ggv506.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-B864-3
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