Rate of change of vorticity covariance of MHD turbulence in a rotating system

Details Rate of change of vorticity covariance of MHD turbulence in a rotating system Rate of change of vorticity covariance of MHD turbulence in a rotating system

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.172..279k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 172, no. 2, Oct. 1990, p. 279-284.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Turbulence, Rotating Fluids, Vorticity, Coriolis Effect, Equations Of Motion, Mathematical Models, Turbulent Flow

Scientific paper

In this paper we are concerned with incompressible MHD turbulence in a rotating system and have derived an equation for the rate of change of vorticity covariance of MHD turbulent flow. The result derived shows that the defining scalars x(r, t), ~(r, t), and y(r, t) for the rate of change of vorticity covariance solely depend on the defining scalars of the tensors Wi,, P~3, FkJ, T~1, and RkJ,f already defined in the text

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