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Sustained turbulence and magnetic energy in nonrotating shear flows
Farrukh Nauman1,2, Eric G Blackman1
1Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA.
Abstract:
From numerical simulations, we show that nonrotating magnetohydrodynamic shear flows are unstable to finite amplitude velocity perturbations and become turbulent, leading to the growth and sustenance of magnetic energy, including large scale fields. This supports the concept that sustained magnetic energy from turbulence is independent of the driving mechanism for large enough magnetic Reynolds numbers.
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