
Research Group: Stratified, Rotating Fluid Flow
Mark Petersen, Neil Martinsen-Burrell
Jeff Weiss, Keith Julien, Michael Sprague
Collaborators
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Joe Werne
Colorado Research Associates
Research Interests: High Rayleigh-number convection, penetrative convection, rotating convection; transport processes and coherent structures in fluid turbulence; instability processes in geophysical and astrophysical flows; stratified shear turbulence, gravity-wave breaking; stratified shear magnetohydrodynamic instability and turbulence; accurate spectral numerical methods, large-scale and high-performance computing, massively parallel computing (Cray T3E, XT3, XT4; IBM SP; SGI Origin 2000, ALTIX).
Michael A. Sprague
University of California at Merced, School of Natural Sciences, Program in Applied Mathematics.
Research Interests: Numerical simulation of geophysical flows. Michael is using a parallel Chebyshev- Petrov-Galerkin program to solve a reduced set of non-hydrostatic quasi-geostrophic equations for rapidly rotating convection, which is applicable to ocean deep convection. As a Ph.D. student in Mechanical Engineering, Michael developed a coupled spectral-element/finite-element program for near-free-surface ship-shock simulation that incorporates nonlinear cavitation effects and field separation.
Edgar Knobloch
University of California at Berkeley
Department of Physics
Research Interests: nonlinear dynamics of dissipative systems;
bifurcation theory, particularly in systems with symmetry;
transition to chaos;
low-dimensional behavior of continuous systems;
turbulent transport and theory of turbulence;
nonlinear waves.
Jeff Weiss
University of Colorado, Boulder
Program in Atmospheric and Oceanic Sciences
Research Interests:
Dr. Weiss' research is focused on theoretical problems in geophysical fluid dynamics, with particular emphasis on nonlinear phenomena and the role of coherent structures
Glen Stewart
University of Colorado, Boulder,
Laboratory for Atmospheric and Space Physics
Research Interests:
Origin and evolution of the solar system, with an emphasis on modeling the solid-body accretion of the terrestrial planets and the solid cores of the giant planets. Accretion of the Moon after a giant impact on the Earth. Modeling of satellite wakes and spiral density waves in planetary rings. Nonlinear dynamics of the three-body problem as applied to problems in solar system dynamics.
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