arXiv · 0810.2950
Amplification of magnetic fields by dynamo action in Gaussian-correlated helical turbulence
Abstract
We investigate the growth and structure of magnetic fields amplified by kinematic dynamo action in turbulence with non-zero kinetic helicity. We assume a simple Gaussian velocity correlation tensor, which allows us to consider very large magnetic Reynolds numbers, up to one trillion. We use the kinematic Kazantsev-Kraichnan model of dynamo and find a complete numerical solution for the correlation functions of growing magnetic fields.
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Leonid Malyshkin, Stanislav Boldyrev. 2008-10-16. Amplification of magnetic fields by dynamo action in Gaussian-correlated helical turbulence. https://doi.org/10.1088/0031-8949/2008/t132/014028
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