Shell-to-shell energy transfer in magnetohydrodynamics. II. Kinematic dynamo

Pablo Mininni1, Alexandros Alexakis, Annick Pouquet

  • 1National Center for Atmospheric Research, P.O. Box 3000, Boulder, Colorado 80307, USA. mininni@ucar.edu

Summary

Turbulent velocity fluctuations amplify magnetic fields at small scales, while large-scale flows amplify the large-scale magnetic field. Energy transfer in magnetohydrodynamics involves both direct velocity-to-magnetic field coupling and magnetic energy cascades.

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