Axisymmetric ideal MHD stellar wind flow

Details Axisymmetric ideal MHD stellar wind flow Axisymmetric ideal MHD stellar wind flow

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978jgr....83.2457h&link_type=abstract

Journal of Geophysical Research, vol. 83, June 1, 1978, p. 2457-2460.

Astronomy and Astrophysics

Astrophysics

60

Axisymmetric Flow, Magnetohydrodynamic Flow, Stellar Winds, Astrophysics, Enthalpy, Equations Of State, Gravitational Fields, Ideal Gas, Magnetohydrodynamic Waves, Perturbation Theory, Solar Wind, Variational Principles

Scientific paper

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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