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Hypersonic Viscous Flow Over Large Roughness ElementsViscous flow over discrete or distributed surface roughness has great implications for hypersonic flight due to aerothermodynamic considerations related to laminar-turbulent transition. Current prediction capability is greatly hampered by the limited knowledge base for such flows. To help fill that gap, numerical computations are used to investigate the intricate flow physics involved. An unstructured mesh, compressible Navier-Stokes code based on the space-time conservation element, solution element (CESE) method is used to perform time-accurate Navier-Stokes calculations for two roughness shapes investigated in wind tunnel experiments at NASA Langley Research Center. It was found through 2D parametric study that at subcritical Reynolds numbers, spontaneous absolute instability accompanying by sustained vortex shedding downstream of the roughness is likely to take place at subsonic free-stream conditions. On the other hand, convective instability may be the dominant mechanism for supersonic boundary layers. Three-dimensional calculations for both a rectangular and a cylindrical roughness element at post-shock Mach numbers of 4.1 and 6.5 also confirm that no self-sustained vortex generation from the top face of the roughness is observed, despite the presence of flow unsteadiness for the smaller post-shock Mach number case.
Document ID
20110012469
Acquisition Source
Langley Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Chang, Chau-Lyan
(NASA Langley Research Center Hampton, VA, United States)
Choudhari, Meelan M.
(NASA Langley Research Center Hampton, VA, United States)
Date Acquired
September 8, 2013
Publication Date
January 1, 2009
Subject Category
Fluid Mechanics And Thermodynamics
Report/Patent Number
LF99-8641
Funding Number(s)
WBS: WBS 599489
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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