NASA NTRS ยท 19780032764
Magnetopause shapes - General solutions
Abstract
The problem of determining the shape of a magnetopause, namely, the tangential discontinuity separating (typically) the magnetic field of a source from external plasma, is reduced to solving an integral equation. No symmetry assumptions whatsoever are used in the derivation, consequently, realistic problems such as model shapes for the earth's magnetosphere (tilted dipole, flowing plasma, etc.) can in principle be treated. Moreover, the magnetic field source itself need not be a simple dipole. A variational method is suggested whereby the optimum parameters for any finite term trial shape are obtained.
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Michel, F. C.. 1977-11-01. Magnetopause shapes - General solutions. https://ntrs.nasa.gov/citations/19780032764
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