Rate of change of vorticity covariance in dusty fluid turbulence in the presence of magnetic field

Details Rate of change of vorticity covariance in dusty fluid turbulence in the presence of magnetic field Rate of change of vorticity covariance in dusty fluid turbulence in the presence of magnetic field

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..169d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 1, March 1990, p. 169-172. Research supported by UGCI.

Statistics

Computation

Computational Fluid Dynamics, Covariance, Isotropic Turbulence, Magnetic Fields, Vorticity, Astrophysics, Beltrami Flow, Dust, Geophysics

Scientific paper

Expressions are derived for the rate of change of vorticity covariance
in dusty fluid turbulence in the presence of a magnetic field. The
influence of dust particles on the fluid motion is discussed,
considering the Beltrami field. It is shown that the rate of change of
vorticity covariance depends on the defining scalars.

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