Galactic structures in the viscous gas flow in the channel with solid walls

 
PIIS023408790000571-2-1
DOI10.31857/S023408790000571-2
Publication type Article
Status Published
Authors
Affiliation: Keldysh Institute of Applied Mathematics RAS
Address: Russian Federation, Moscow
Affiliation: Keldysh Institute of Applied Mathematics RAS
Address: Russian Federation, Moscow
Journal nameMatematicheskoe modelirovanie
EditionVolume 30 Number 7
Pages16-28
Abstract

Hydromechanical processes occurring in the viscous flow of gas (air), moving in a narrow channel are considered. It was established that under this case the gas flow by about two-thirds of the length of the channel turbulent, and then becomes laminar and vortex with decreasing rotation vortices speed along longitudinal coordinate. Under the influence of viscous forces around some centers expanding to the periphery the "garland" are formed, it is like having a place in the cosmos. Along the perimeter of a rotating structure are somewhat similar "strings".

Keywordsnumerical simulation, turbulent flow, Reynolds number, galactic structure
Received25.09.2018
Publication date27.09.2018
Number of characters631
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