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Nonlinear axisymmetric liquid currents in spherical annuliA 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.
Document ID
19790002205
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Astafyeva, N. M.
(NASA Headquarters Washington, DC United States)
Vvedenskaya, N. D.
(NASA Headquarters Washington, DC United States)
Yavorskaya, I. M.
(NASA Headquarters Washington, DC United States)
Date Acquired
September 3, 2013
Publication Date
October 1, 1978
Subject Category
Fluid Mechanics And Heat Transfer
Report/Patent Number
NASA-TM-75559
REPT-385
Accession Number
79N10376
Funding Number(s)
CONTRACT_GRANT: NASW-3198
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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