By Kozo Fujii, Kazuhiro Nakahashi, Shigeru Obayashi, Satoko Komurasaki
ISBN-10: 3540274073
ISBN-13: 9783540274070
ISBN-10: 3540312617
ISBN-13: 9783540312611
This quantity includes 20 papers offered on the 6th foreign Nobeyama Workshop at the New Century of Computational Fluid Dynamics, Nobeyama, Japan, April 21-24, 2003. The Nobeyama Workshop makes a speciality of predicting the following 100 years of improvement of Fluid Dynamics, accounting for the present prestige and destiny tendencies of excessive functionality computation and conversation. The papers hide computational electromagnetics, astrophysical subject matters, CFD learn and functions as a rule, large-eddy simulation, vortical flows, mesh iteration issues, visualization, DNA computing, multidisciplinary simulation and optimisation, in addition to algorithmic advancements. The Workshops are recognized for the casual and focused surroundings of in-depth dialogue due to all of the efforts of Prof. Kunio Kuwahara at ISAS, Japan. In occasion of his sixtieth birthday, this workshop was once devoted to him.
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Extra resources for New Developments in Computational Fluid Dynamics: Proceedings of the Sixth International Nobeyama Workshop on the New Century of Computational Fluid Dynamics, Nobeyama, Japan, April 21 to 24, 2003 (Notes on Numerical Fluid Mechanics and Multidisciplinary
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The counter-flow jet interaction with the bow shock replaces the single wave to a triple shock structure [14]. The shock bifurcation was also discovered by the side-by-side computational and experimental study of the jet spike. At the bifurcation point between the steady and unsteady states, the drag reduction also attains the Hypersonic Magneto-Aerodynamic Interaction Figure 1 25 Streamline trace of the jet spike flow field maximum value. The bifurcation is the consequence of breakdown of the subsonic upstream feedback loop between the Mach disk and the unsteady free shear layer [14].
9. Note that the Case 2 geometry has 5-times larger corner radius than the Apollo. When the results of the Case 2 is compared with that of the Apollo, it is obvious that the shoulder radius has significant effect on the aerodynamic characteristics for 38 K. 9 the base entry (180 degrees). The CLmax of the Case 2 is approximately half of that of the Apollo. The computed pressure contours and the near-surface streamlines are plotted in Figs. 7(a) and 7(b), respectively for each geometry. The reason for the CL difference is that the separation occurs always at the shoulder for the Apollo but the location of separation changes depending on the angle of attack for the Case 2.
The computational grid used in this study is 143 × 107 × 169 with the O-O topology. 4. Figure 9 shows an instantaneous view of the computed vorticity magnitude contours by the LES/RANS hybrid method. There exists strong flow unsteadiness and the flow field changes in time although only one shot is shown 42 K. Fujii Figure 9 Instantaneous view of the vorticity magnitude contours: LES/RANS hybrid computation Figure 10 Instantaneous view of the vorticity magnitude contours: RANS hybrid computation here.
New Developments in Computational Fluid Dynamics: Proceedings of the Sixth International Nobeyama Workshop on the New Century of Computational Fluid Dynamics, Nobeyama, Japan, April 21 to 24, 2003 (Notes on Numerical Fluid Mechanics and Multidisciplinary by Kozo Fujii, Kazuhiro Nakahashi, Shigeru Obayashi, Satoko Komurasaki
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