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Computational aerodynamics: Advances and challenges

Published online by Cambridge University Press:  04 February 2016

Dimitris Drikakis
Affiliation:
University of Strathclyde, Glasgow, UK
Dochan Kwak
Affiliation:
NASA Ames Research Center, Moffett Field, USA
Cetin C. Kiris
Affiliation:
NASA Ames Research Center, Moffett Field, USA
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Abstract

Computational aerodynamics, which complement more expensive empirical approaches, are critical for developing aerospace vehicles. During the past three decades, computational aerodynamics capability has improved remarkably, following advances in computer hardware and algorithm development. However, most of the fundamental computational capability realised in recent applications is derived from earlier advances, where specific gaps in solution procedures have been addressed only incrementally. The present article presents our view of the state of the art in computational aerodynamics and assessment of the issues that drive future aerodynamics and aerospace vehicle development. Requisite capabilities for perceived future needs are discussed, and associated grand challenge problems are presented.

Information

Type
Research Article
Copyright
Copyright © Royal Aeronautical Society 2016 
Figure 0

Figure 1. Multi-scale modelling of materials and multi-material interfaces across length scales.

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Figure 2. Computational grid for the DLR-F6 geometry; a) surface mesh of the DLR-F6 quadrature points; b) corresponding quadrature points.

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Figure 3. Predicted drag coefficient (CD) error for DLR-F6 obtained from second- and third-order methods and comparison with the mean values of the solutions of the 2nd Drag Prediction Workshop. The blue line (labelled as present) has been obtained using a high-order RANS code (Azure)(123) in conjunction with the second-order MUSCL and third-order WENO schemes on the coarsest grid.

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Figure 4. Rotorcraft flow simulations in top view in forward flight and hover.

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Figure 5. Examples of three different grid topologies for launch environment simulation.

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Figure 6. Geometry and point probe locations for jet impingement test case for space-time convergence study. Flow conditions are from the experiment by Nakanishi et al(129): Nozzle exit temperature = 300K, jet Mach number, M = 1.8.

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Figure 7. Spatial convergence study for 2D case(129).

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Figure 8. Mach number distribution for four points in the Apollo 6 trajectory using SST turbulence model(133) with hybrid grid(134).