NASA NTRS · 19810036294
On the magnetoaerothermal instability
Abstract
A fundamental instability in MHD channel flow, hitherto unknown or unappreciated, is described. Lorentz force-driven secondary flow cells preferentially couple core temperature gradient modes into the near fields of the anode wall leading to a locally growing Lorentz force which eventually separates the anode boundary layer. The instability is described with both heuristic order-of-magnitude analyses and detailed three-dimensional, turbulent, MHD flow computations. This magnetoaerothermal instability will be manifested in commercial scale MHD generators of moderate MHD interaction parameter. Methods of control and prevention of the magnetoaerothermal instability exist.
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Demetriades, S. T., Oliver, D. A., Swean, T. F., Jr., Maxwell, C. D.. 1981-01-01. On the magnetoaerothermal instability. https://ntrs.nasa.gov/citations/19810036294
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