NASA Technical Paper

NASA Technical Paper
Author:
Publisher:
Total Pages: 84
Release: 1979
Genre: Science
ISBN:

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Numerical Results for the Diffraction of a Normal Shock Wave by a Sphere and for the Subsequent Transient Flow

Numerical Results for the Diffraction of a Normal Shock Wave by a Sphere and for the Subsequent Transient Flow
Author: Richard W. Barnwell
Publisher:
Total Pages: 44
Release: 1967
Genre: Aerodynamics
ISBN:

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The finite-difference method which Peter D. Lax developed for treating unsteady inviscid flow fields is used to study the transient flow in the shock layer of a sphere that has been struck by a normal shock wave. Transient flow of this sort is encountered when a shock tube is used as a supersonic wind tunnel. Time histories of the shock detachment distance and the stagnation-point pressure and tangential velocity gradient are presented for ranges of the incident-shock Mach number and the perfect-gas specific-heat ratio. These results show that the stagnation-point pressure approaches the steady value much more rapidly than the shock detachment distance. In general, the stagnation-point pressure but more rapidly than the shock detachment distance. As the specific-heat ratio is decreased and the incident-shock Mach number is increased, the variation of the velocity gradient with respect to the shock detachment distance becomes more nearly linear.

NASA Technical Note

NASA Technical Note
Author:
Publisher:
Total Pages: 418
Release: 1975
Genre:
ISBN:

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Inviscid Radiating Shock Layers about Spheres Traveling at Hyperbolic Speeds in Air

Inviscid Radiating Shock Layers about Spheres Traveling at Hyperbolic Speeds in Air
Author: Richard W. Barnwell
Publisher:
Total Pages: 88
Release: 1969
Genre: Aerodynamics, Hypersonic
ISBN:

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Time-dependent finite-difference techniques are used to obtain numerical solutions for the problem of the inviscid flow of radiating equilibrium air past sphere traveling at hyperbolic speeds. The effects of absorption are included, and results are presented for both gray and nongray absorption coefficient models for spheres with different radii. It is shown that the nondimensional heat-flux distributions for the gray and nongray models are similar and that these distributions are weak functions of the radius of the sphere and the altitude and strong functions of the flight velocity.