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Constant Density Approximations for the Flow Behind Axisymmetric Shock WavesThe incompressible rotational flow equations are used to obtain solutions for the flow behind axisymmetric shock waves with conic longitudinal sections. The nonlinear part of the term due to rotation is retained in the analysis. Numerical results for standoff distance and stagnation point velocity gradient are presented for the case in which the shock wave is a paraboloid, a sphere, or an oblate or prolate ellipsoid. A similarity parameter is proposed which correlates approximately the flow behind geometrically similar shock waves at different free-stream conditions.
Document ID
20040006387
Acquisition Source
Langley Research Center
Document Type
Other - NASA Technical Note (TN)
Authors
Munson, Albert G.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 21, 2013
Publication Date
May 1, 1961
Subject Category
Fluid Mechanics And Thermodynamics
Report/Patent Number
A-322
NASA-TN-D-857
Report Number: A-322
Report Number: NASA-TN-D-857
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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