A PURE HYDRODYNAMIC INSTABILITY IN SHEAR FLOWS AND ITS APPLICATION TO ASTROPHYSICAL ACCRETION DISKS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/830/i=2/a=86/pdf
Reference60 articles.
1. Bypass to Turbulence in Hydrodynamic Accretion: Lagrangian Analysis of Energy Growth
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4. A turbulent matter
5. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
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