On the geometry of streamlines of a dusty fluid in MHD flows

Details On the geometry of streamlines of a dusty fluid in MHD flows On the geometry of streamlines of a dusty fluid in MHD flows

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.106...35s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 106, no. 1, Nov. 1984, p. 35-40.

Astronomy and Astrophysics

Astrophysics

Dust, Flow Geometry, Laminar Flow, Magnetohydrodynamic Flow, Maxwell Fluids, Two Phase Flow, Conducting Fluids, Incompressible Flow, Particle Density (Concentration)

Scientific paper

The steady nondissipative flow of an infinitely conducting incompressible dusty fluid in a magnetic field is investigated analytically, considering the streamline geometry of a fluid for which the distribution function of the dust particles is variable and the particle velocities are assumed to be parallel to the motion of the fluid. The nonholonomic geometric approach of Marris and Passman (1969) is applied, and it is found that Maxwellian surfaces corresponding to the surfaces of constant pressure can be obtained under certain defined conditions.

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