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Dissipative, forced turbulence in two-dimensional magnetohydrodynamicsThe 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.
Document ID
19770020036
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Fyfe, D.
(National Center for Atmospheric Research Boulder, CO, United States)
Montgomery, D.
(National Center for Atmospheric Research Boulder, CO, United States)
Joyce, G.
(Iowa Univ. Iowa City, United States)
Date Acquired
September 3, 2013
Publication Date
January 1, 1976
Subject Category
Plasma Physics
Report/Patent Number
COO-2059-55
NASA-CR-152862
Report Number: COO-2059-55
Report Number: NASA-CR-152862
Accession Number
77N26980
Funding Number(s)
CONTRACT_GRANT: E(11-1)-2059
CONTRACT_GRANT: NGL-16-001-043
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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