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A computational study of separated flows over a NACA 0012 airfoil at transitional Reynolds numbers is performed. The transitional nature of the flowfield is incorporated into the computations through γ-Reθ transition model based on local variables. Fully turbulent and transitional computations are performed for steady airfoil flowfields and computed results are compared against experiments. The γ-Reθ transition model, in association with Menter’s SST turbulence model is used for the transitional solutions while, SST turbulence model alone is used for the fully turbulent solutions. Both steady and unsteady compressible flow analysis for transition onset prediction and flow separation characterization has been performed. Effects of free stream flow conditions on flow transition are examined.

In the design of solar powered cars aerodynamic efficiency is extremely important. Due to the limited power and energy sources available, the aerodynamic design of the car must provide a low coefficient of drag. In order to identify the major drag source areas in the design and to improve the aerodynamics performance of the current NDSU solar car an extensive computational fluid dynamics (CFD) study was performed using ANSYS CFX 10.0. The study was set into two paths. The first path focused on modifying the current NDSU solar car design in order to reduce the drag force. The second path was to design a completely new solar car with better aerodynamics performance. Through the CFD analysis of all the designs considered major drag source areas were identified as the underbody, the dome, and the nose section of the car.

Flow field computations and, in particular, that of pressure, skin friction, and heat transfer (for high speed flights) are the primary parameters in the design of aerospace vehicles. Most computational schemes based on either the inviscid Euler equations or various forms of the Navier-Stokes equations are remarkably accurate in the predictions of pressure distributions. However, computations of skin friction and heat transfer particularly at high speeds have been a source of considerable difficulty. Problems arise not only due to the grid resolution but also due to the particular numerical scheme employed. To address the difficulty associated with accurate computations of the velocity and temperature gradients, a comparative investigation of several Navier- Stokes codes is undertaken. Previous studies with regard to the effect of grid resolution are incorporated into the current investigation.