Vincenzo Carbone Dipartimento di Fisica, Università della Calabria Rende (CS) – Italy [email protected] Models for turbulence.
3D Vortices in Stratified, Rotating, Shearing Protoplanetary Disks April 8, 2005 - I PAM Workshop I: Astrophysical Fluid Dynamics Philip Marcus – UC Berkeley.
STABILITY AND TRANSPORT IN TAYLOR- COUETTE FLOW: APPLICATION TO PROTOPLANETARY DISKS B. DUBRULLE CNRS, Groupe instabilité et Turbulence SPEC/DRECAM/DSM,
SOLAR WIND TURBULENCE; WAVE DISSIPATION AT ELECTRON SCALE WAVELENGTHS S. Peter Gary Space Science Institute Boulder, CO Meeting on Solar Wind Turbulence.
Jungyeon Cho, Alex Lazarian and Ethan T. Vishniac- Simulations of MHD Turbulence in a Strongly Magnetized Medium
Introduction to (weak) wave turbulence
Method and System for Monitoring and Analyzing Energy Consumption in Operated Chemical Plants US8554381
Reynolds Transport
Fluent 13.0 Lecture06-Turbulence
1 Lecture 9 - Kolmogorov’s Theory Applied Computational Fluid Dynamics Instructor: André Bakker © André Bakker (2002-2005) © Fluent Inc. (2002)
Symmetries of turbulent state Gregory Falkovich Weizmann Institute of Science Rutgers, May 10, 2009 D. Bernard, A. Celani, G. Boffetta, S. Musacchio.
Shocks! David Burgess Astronomy Unit Queen Mary, University of London.
