On hydrodynamic shear turbulence in Keplerian disks: Via transient growth to bypass transition
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20030269/pdf
Reference63 articles.
1. A mostly linear model of transition to turbulence
2. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
3. A Powerful Local Shear Instability in Weakly Magnetized Disks. IV. Nonaxisymmetric Perturbations
4. Nonlinear Stability, Hydrodynamical Turbulence, and Transport in Disks
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