The geometry of two-phase magnetofluid flows in a rotating system

Details The geometry of two-phase magnetofluid flows in a rotating system The geometry of two-phase magnetofluid flows in a rotating system

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149...83t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 1, Nov. 1988, p. 83-90.

Astronomy and Astrophysics

Astrophysics

2

Flow Geometry, Plasma Dynamics, Rotating Fluids, Two Phase Flow, Incompressible Flow, Magnetic Fields, Nonholonomic Equations, Steady Flow, Viscous Flow

Scientific paper

The Beltrami motion of steady, rotating, viscous, incompressible, perfectly-conducting two-phase fluid flows in the presence of a magnetic field is investigated. In the analysis, the governing equations have been decomposed along the vortex line triad. Conditions are determined for which the vortex lines are geodesics and the family of Maxwellian surfaces is a normal congruence of developables.

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