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NASA NTRS · 20080034485

Efficient Unstructured Grid Adaptation Methods for Sonic Boom Prediction

Abstract

This paper examines the use of two grid adaptation methods to improve the accuracy of the near-to-mid field pressure signature prediction of supersonic aircraft computed using the USM3D unstructured grid flow solver. The first method (ADV) is an interactive adaptation process that uses grid movement rather than enrichment to more accurately resolve the expansion and compression waves. The second method (SSGRID) uses an a priori adaptation approach to stretch and shear the original unstructured grid to align the grid with the pressure waves and reduce the cell count required to achieve an accurate signature prediction at a given distance from the vehicle. Both methods initially create negative volume cells that are repaired in a module in the ADV code. While both approaches provide significant improvements in the near field signature (< 3 body lengths) relative to a baseline grid without increasing the number of grid points, only the SSGRID approach allows the details of the signature to be accurately computed at mid-field distances (3-10 body lengths) for direct use with mid-field-to-ground boom propagation codes.

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BibTeXRIS

Campbell, Richard L., Carter, Melissa B., Deere, Karen A., Waithe, Kenrick A.. 2008-08-18. Efficient Unstructured Grid Adaptation Methods for Sonic Boom Prediction. https://ntrs.nasa.gov/citations/20080034485

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