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NASA NTRS · 19790002205

Nonlinear axisymmetric liquid currents in spherical annuli

Abstract

A numerical analysis of non-linear axisymmetric viscous flows in spherical annuli of different gap sizes is presented. Only inner sphere was supposed to rotate at a constant angular velocity. The streamlines, lines of constant angular velocity, kinetic energy spectra, and spectra of velocity components are obtained. A total kinetic energy and torque needed to rotate the inner sphere are calculated as functions of Re for different gap sizes. In small-gap annulus nonuniqueness of steady solutions of Navier-Stokes equations is established and regions of different flow regime existences are found. Numerical solutions in a wide-gap annulus and experimental results are used in conclusions about flow stability in the considered range of Re. The comparison of experimental and numerical results shows close qualitative and quantitative agreement.

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BibTeXRIS

Astafyeva, N. M., Vvedenskaya, N. D., Yavorskaya, I. M.. 1978-10-01. Nonlinear axisymmetric liquid currents in spherical annuli. https://ntrs.nasa.gov/citations/19790002205

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