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Some recent applications of XTRAN3SA time marching finite difference code, XTRAN3S that solves the three dimensional transonic small perturbation equation for flow over isolated wings was developed. During initial applications of the program, problems were encountered in the prediction of unsteady forces. The use of a revised grid and force calculation scheme improved those predictions. Comparisons are made between predicted and experimental pressure data for a rectangular supercritical wing. Comparisons of steady and unsteady data at M sub infinity = 0.700 show good agreement between calculated and experimental values. A comparison of steady data at M sub infinity 0.825 shows poor agreement between calculations and experiment. Program difficulties were encountered with swept and tapered configurations.
Document ID
19830018544
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Seidel, D. A.
(NASA Langley Research Center Hampton, VA, United States)
Bennett, R. M.
(NASA Langley Research Center Hampton, VA, United States)
Ricketts, R. H.
(NASA Langley Research Center Hampton, VA, United States)
Date Acquired
September 4, 2013
Publication Date
May 1, 1983
Subject Category
Aerodynamics
Report/Patent Number
NAS 1.15:85641
NASA-TM-85641
Report Number: NAS 1.15:85641
Report Number: NASA-TM-85641
Meeting Information
Meeting: AIAA Appl. Aerodyn. Conf.
Location: Danvers, MA
Country: United States
Start Date: July 13, 1983
End Date: July 15, 1983
Accession Number
83N26815
Funding Number(s)
PROJECT: RTOP 505-33-43-09
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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