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Direct numerical simulations of transitional supersonic base flows

Direct numerical simulations of transitional supersonic base flows
Direct numerical simulations of transitional supersonic base flows
Transitional supersonic base flows at M=2.46 are investigated using Direct Numerical Simulations. Results are presented for Reynolds numbers based on the cylinder diameter ReD=30,000-100,000. As a consequence of flow instabilities, coherent structures develop that have a profound impact on the global flow behavior. Simulations with various circumferential domain sizes are conducted to investigate the effect of coherent structures associated with different azimuthal modes on the mean flow, in particular on the base pressure which determines the base drag.
Temporal spectra reveal that frequencies found in the axisymmetric mode can be related to dominant higher modes present in the flow. It is shown that azimuthal modes with low wavenumbers cause a flat base pressure distribution and that the mean base pressure value increases when the most dominant modes are deliberately eliminated. Visualizations of instantaneous flow quantities and turbulence statistics at ReD=100,000 show good agreement with experiments at a significantly higher Reynolds number. For these investigations, a high-order accurate compressible Navier-Stokes solver in cylindrical coordinates developed specifically for this research was used.
0001-1452
848-858
Sandberg, R.D.
41d03f60-5d12-4f2d-a40a-8ff89ef01cfa
Fasel, H.F.
45db4ae8-5501-4afd-9d6f-b35ac55e7629
Sandberg, R.D.
41d03f60-5d12-4f2d-a40a-8ff89ef01cfa
Fasel, H.F.
45db4ae8-5501-4afd-9d6f-b35ac55e7629

Sandberg, R.D. and Fasel, H.F. (2006) Direct numerical simulations of transitional supersonic base flows. AIAA Journal, 44 (4), 848-858.

Record type: Article

Abstract

Transitional supersonic base flows at M=2.46 are investigated using Direct Numerical Simulations. Results are presented for Reynolds numbers based on the cylinder diameter ReD=30,000-100,000. As a consequence of flow instabilities, coherent structures develop that have a profound impact on the global flow behavior. Simulations with various circumferential domain sizes are conducted to investigate the effect of coherent structures associated with different azimuthal modes on the mean flow, in particular on the base pressure which determines the base drag.
Temporal spectra reveal that frequencies found in the axisymmetric mode can be related to dominant higher modes present in the flow. It is shown that azimuthal modes with low wavenumbers cause a flat base pressure distribution and that the mean base pressure value increases when the most dominant modes are deliberately eliminated. Visualizations of instantaneous flow quantities and turbulence statistics at ReD=100,000 show good agreement with experiments at a significantly higher Reynolds number. For these investigations, a high-order accurate compressible Navier-Stokes solver in cylindrical coordinates developed specifically for this research was used.

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Submitted date: 13 June 2005
Published date: April 2006

Identifiers

Local EPrints ID: 35487
URI: http://eprints.soton.ac.uk/id/eprint/35487
ISSN: 0001-1452
PURE UUID: 40d7fffd-960d-4651-ab46-167909f3a115
ORCID for R.D. Sandberg: ORCID iD orcid.org/0000-0001-5199-3944

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Date deposited: 16 May 2006
Last modified: 15 Mar 2024 07:51

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Contributors

Author: R.D. Sandberg ORCID iD
Author: H.F. Fasel

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