Abstract
The standard two-scale theory of the dynamo coefficient α in incompressible isotropic helical MHD turbulence is extended to include nonlinear effects of B̄, the large-scale magnetic field. We express α in terms of statistical quantities that can be calculated from numerical simulations of the case B̄ = 0. For large magnetic Reynolds numbers, our formula agrees approximately with that of Kraichnan but disagrees with that of Cattaneo & Hughes.
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CITATION STYLE
APA
Field, G. B., Blackman, E. G., & Chou, H. (1999). Nonlinear α‐Effect in Dynamo Theory. The Astrophysical Journal, 513(2), 638–651. https://doi.org/10.1086/306877
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