Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/75502
Title: Wave number selection under the action of accelerated rotation
Authors: Krivonosova, O.
Zhilenko, D.
Gritsevich, M.
Issue Date: 2019
Publisher: Institute of Physics Publishing
Citation: Krivonosova O. Wave number selection under the action of accelerated rotation / O. Krivonosova, D. Zhilenko, M. Gritsevich // Journal of Physics: Conference Series. — 2019. — Vol. 1163. — Iss. 1. — 12035.
Abstract: Unsteady viscous incompressible flows in a spherical layer due to an increase in the rotation velocity of the inner sphere with constant acceleration are investigated. The acceleration starts at the Reynolds numbers Re corresponding to a stationary flow and ends at Re higher than the stability limit of the stationary flow, whereupon the rotation velocity of the inner sphere remains constant. The outer sphere is fixed and the spherical layer thickness is equal to the inner sphere radius. The inner sphere acceleration effect is studied on both the formation of one of two possible secondary-flow structures after the acceleration has been stopped, namely, traveling azimuthal waves with wavenumbers of 3 or 4, and on the change in the flow structure during the action of the acceleration. It is shown that not only an increase in the acceleration but also a decrease in Re corresponding to the acceleration onset can lead to an increase in the deviation of the instantaneous velocity profiles from their stationary values and can be accompanied by a variation in the secondary flow wavenumber. © Published under licence by IOP Publishing Ltd.
Keywords: ACCELERATION
BERYLLIUM COMPOUNDS
FLOW STRUCTURE
REYNOLDS NUMBER
SECONDARY FLOW
ACCELERATED ROTATION
ACCELERATION EFFECTS
CONSTANT ACCELERATION
ROTATION VELOCITY
STATION-ARY VALUES
VELOCITY PROFILES
VISCOUS INCOMPRESSIBLE FLOWS
WAVE-NUMBER SELECTION
SPHERES
URI: http://elar.urfu.ru/handle/10995/75502
Access: info:eu-repo/semantics/openAccess
Conference name: 3rd International Conference on Computer Simulations in Physics and Beyond, CSP 2018
Conference date: 24 September 2018 through 27 September 2018
SCOPUS ID: 85064380197
WOS ID: 000471139000035
PURE ID: 9311469
ISSN: 1742-6588
DOI: 10.1088/1742-6596/1163/1/012035
Sponsorship: This work was supported by the Russian Foundation for Basic Research Project No. 16-05-00004 and 18-08-00074. MG acknowledges,in part, support from the ERC Advanced Grant No. 320773. Research at the Ural Federal University is supported by the Act 211 of the Government of the Russian Federation, agreement No 02.A03.21.0006.
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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