Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13...77h&link_type=abstract
In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se
Astronomy and Astrophysics
Astronomy
Scientific paper
In the present paper we study the absolute and convective nature of instabilities in open shear flows by carrying out fully non-linear adiabatic 2-D hydrodynamic numerical simulations. We found the value of mean flow for which perturbations change from absolute to convective unstable. We fully recover the results of a previous analytic solution. We found that (i) an inviscid incompressible fluid is the most unstable configuration; (b) compressibility and viscosity decrease the value of mean flow necessary for the transition from absolute to convective instability; (c) even a viscosity has dominant influence over compressibility.
Erdelyi Robert
Homem M. T.
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