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In-Lab Shallow-Water Simulations of Gaseous Discs for Astrophysical Fluid Dynamics

Published online by Cambridge University Press:  13 February 2013

G.P. Chernikov ,
A.M. Fridman ,
E.N. Snezhkin ,
J. Sommeria  and
Yu.M. Torgashin
G.P. Chernikov
Affiliation:
National Research Centre “Kurchatov Institute”, 1 Acad. Kurchatova Sq., 123182 Moscow, Russia
A.M. Fridman
Affiliation:
Institute of Astronomy RAS, 48 Pyatnitskaya St., 119017 Moscow, Russia
E.N. Snezhkin
Affiliation:
National Research Centre “Kurchatov Institute”, 1 Acad. Kurchatova Sq., 123182 Moscow, Russia
J. Sommeria
Affiliation:
Coriolis/LEGI, 21 avenue des Martyrs, 38000 Grenoble, France
Yu.M. Torgashin
Affiliation:
Institute of Astronomy RAS, 48 Pyatnitskaya St., 119017 Moscow, Russia

Abstract

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Presented is a brief review of firsthand laboratory experiments with the use of fast rotating shallow water for simulation of important 2D objects and phenomena of astrophysical fluid dynamics, which alternatively can only be studied theoretically, computationally and very rarely through astronomical observations. Among them are sheared supersonic rotation, instabilities of flows at such rotation, vortical solitary waves, turbulence, and wave over-reflection

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 58: ECLA - European Conference on Laboratory Astrophysics , 2012 , pp. 161 - 165
Copyright
© The Author(s) 2013

References

Références

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