NASA NTRS · 19770020036
Dissipative, forced turbulence in two-dimensional magnetohydrodynamics
Abstract
The equations of motion for turbulent two-dimensional magnetohydrodynamic flows are solved in the presence of finite viscosity and resistivity, for the case in which external forces (mechanical and/or magnetic) act on the fluid. The goal is to verify the existence of a magnetohydrodynamic dynamo effect which is represented mathematically by a substantial back-transfer of mean square vector potential to the longest allowed Fourier wavelengths. External forces consisting of a random part plus a fraction of the value at the previous time step are employed, after the manner of Lilly for the Navier-Stokes case. The regime explored is that for which the mechanical and magnetic Reynolds numbers are in the region of 100 to 1000. The conclusions are that mechanical forcing terms alone cannot lead to dynamo action, but that dynamo action can result from either magnetic forcing terms or from both mechanical and magnetic forcing terms simultaneously.
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Fyfe, D., Montgomery, D., Joyce, G.. 1976-01-01. Dissipative, forced turbulence in two-dimensional magnetohydrodynamics. https://ntrs.nasa.gov/citations/19770020036
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