NASA NTRS · 19780057145
Axisymmetric ideal MHD stellar wind flow
Abstract
The ideal MHD equations are reduced to a single equation under the assumption of axisymmetric flow. A variational principle from which the equation is derivable is given. The characteristics of the equation are briefly discussed. The equation is used to rederive the theorem of Gussenhoven and Carovillano.
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Heinemann, M., Olbert, S.. 1978-06-01. Axisymmetric ideal MHD stellar wind flow. https://ntrs.nasa.gov/citations/19780057145
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