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NASA NTRS ยท 19970014679

Drag reduction in turbulent MHD pipe flows

Abstract

This is a preliminary study devoted to verifying whether or not direct simulations of turbulent Magneto-Hydro-Dynamic (MHD) flows in liquid metals reproduce experimental observations of drag reduction. Two different cases have been simulated by a finite difference scheme which is second order accurate in space and time. In the first case, an external azimuthal magnetic field is imposed. In this case, the magnetic field acts on the mean axial velocity and complete laminarization of the flow at N(sub a) = 30 has been achieved. In the second case, an axial magnetic field is imposed which affects only fluctuating velocities, and thus the action is less efficient. This second case is more practical, but comparison between numerical and experimental results is only qualitative.

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BibTeXRIS

Orlandi, P.. 1996-12-01. Drag reduction in turbulent MHD pipe flows. https://ntrs.nasa.gov/citations/19970014679

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