Developing a new general circulation model for planetary atmospheres - how (and why!) Claire Newman Kliegel Planetary Science Seminar March 1st 2005.
Modeling Titans Atmosphere with Observational Constraints Claire E. Newman Kliegel Planetary Science Seminar February 24th 2009.
Galactic Dynamos and ISM Turbulence. Steve Cowley,UCLA/ Imperial College Alex Schekochihin, Imperial Jim McWilliams, UCLA Greg Hammett, Princeton Greg.
The Modeling of Surface TNR’s on Compact Stars Nova – review X-Ray bursts on NS – first steps.
CIMMSE TC Wind Group Conference Call
TUBULENT FLUXES OF HEAT, MOISTURE AND MOMENTUM: BASICS OF TURBULENCE What is turbulence? Alfred Blackadar: “No definition of turbulence can be given at.
High Performance Computing in Magnetic Fusion Energy Research
Balloon-Borne Sounding System (BBSS)
TUBULENT FLUXES OF HEAT, MOISTURE AND MOMENTUM: BASICS OF TURBULENCE
Balloon-Borne Sounding System (BBSS) Used for atmospheric profiling Measures P, T, RH, wind speed and direction Uncertainties arise from incorrect surface.
