Introduction
Lunar Prospector Impact
Hypersonic Forward-Facing Cavity Flow
Direct Numerical Simulation of Rarefied Flows
Simulations of Gas Dynamics, Radiation and Particulates in Volcanic Plumes on Io
Rarefied / Continuum Flow Solver
Turbulent Flow Over Riblets
Unsteady Flow Between Segments of Hypersonic Projectile
Reduction of Hypersonic Nose Tip Ablation
Drag Reduction Techniques Using MEMS
Temporal Evolution of the Lunar Exosphere

Computational Fluid

Physics Laboratory

Coordinator: Dr. David Goldstein

The Computational Fluid Physics Laboratory (CFPL) utilizes computational fluid dynamics (CFD) and direct numerical simulation (DNS) techniques to probe the physics of unsteady complex fluid problems.

Current projects involve:

  • Using direct numerical simulation (DNS) to study turbulent boundary layer flow and various drag reduction techniques including surface textures and MEMS microjets.
  • Using a particle based technique (DSMC) to model volcanic sulphur dioxide volcanos on Jupiter's moon Io and the escape of the atmosphere of Pluto.
  • Using DSMC to examine Taylor-Couette flow characteristics on a small gap between a rotor and stator in a compressor.

More information on current and past projects can be found by clicking on the left menu.

The Computational Fluid Physics Lab is affiliated with the Department of Aerospace Engineering of the University of Texas at Austin

Our work has been sponsored in whole or in part by various sources including:

For further inquiries, email us or contact:

      Dr. David Goldstein
      Center for Aeromechanics Research
      Department of Aerospace Engineering and Engineering Mechanics - C0600
      University of Texas at Austin
      Austin, TX  78712

      Phone: (512) 471-4187
      

This page is maintained by: Conrad Lee. Last Revised: April 12, 2002