The effect of Coriolis force on acceleration covariance in MHD turbulent dusty flow with rotational symmetry

Details The effect of Coriolis force on acceleration covariance in MHD turbulent dusty flow with rotational symmetry The effect of Coriolis force on acceleration covariance in MHD turbulent dusty flow with rotational symmetry

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..257d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 257-268. Research supported by UGCI.

Physics

1

Coriolis Effect, Magnetohydrodynamic Flow, Magnetohydrodynamic Turbulence, Two Phase Flow, Viscous Flow, Acceleration (Physics), Covariance, Incompressible Flow, Scalars, Symmetry

Scientific paper

This paper considers MHD turbulent dusty flow of an incompressible,
viscous fluid which is nearly isotropic with rotational and spatially
homogeneous turbulence. The expression for acceleration covariance in
the presence of Coriolis force has been derived, and solution has been
obtained in terms of defining scalars.

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