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Braz. J. Phys. vol.35 número1

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Academic year: 2018

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Figure 1. Shape of satellite SARA
Figure 2. Numerical grid.
Figure 5. Comparison with the DSMC of the coefficient C p ; Mach 10. θ10203040 50 60 70 80 9000.050.10.150.20.250.30.35Re = 2161,8Re = 4000Re = 4000 ( DSMC )Ch
Figure 9. Temperatures distribution along the stagnation line, Mach 20, R e = 4323.6. X (m)Massfraction-0.03-0.02 -0.0100.10.20.30.40.50.60.70.8YYYYY with V-V without V-VONNOO2N2
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