47th AIAA Aerospace Sciences Meeting Including the New Horizons Forum and Aerospace Exposition 2009
DOI: 10.2514/6.2009-1317
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Modeling of Viscous Shock Tube Using ES-BGK Model Kinetic Equations

Abstract: The viscous effects on unsteady shock wave propagation are investigated by numerical solution of the Boltzmann model kinetic equations. The kinetic equations are solved for two unsteady non-equilibrium flow problems, namely, the one-dimensional Riemann problem and a two-dimensional viscous shock-tube. The numerical method comprises the discrete velocity method in the velocity space and the finite volume discretization in physical space using various flux schemes. The discrete version of H-theorem is applied fo… Show more

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Cited by 6 publications
(5 citation statements)
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“…Thus, entropy generation rate can be a useful quantity in calculating the location and velocity of both the shock wave and contact discontinuity. This can be extended further to study the rarefaction effects and shock speed attenuation by boundary layer interaction in 2D shock tube [25] as discussed below.…”
Section: D Shock Tubementioning
confidence: 97%
“…Thus, entropy generation rate can be a useful quantity in calculating the location and velocity of both the shock wave and contact discontinuity. This can be extended further to study the rarefaction effects and shock speed attenuation by boundary layer interaction in 2D shock tube [25] as discussed below.…”
Section: D Shock Tubementioning
confidence: 97%
“…The ESBGK equilibrium distribution function is of the form [34]: Eqs. (26) and (27), the ESBGK model has ten unknowns α 1 -α 10 . In addition to solving for the conservation of mass and momentum, we solve for the conservation of six additional higher moments of equilibrium distribution function to obtain these coefficients [34]:…”
Section: Esbgk Modelmentioning
confidence: 99%
“…(13), (14) and Eqs. (26), (27). The central idea behind COMET is to couple the velocity ordinates strongly through a point-implicit direct solution of the distribution function values in each cell, and to traverse the spatial cells in a Gauss-Seidel procedure.…”
Section: Comet Solvermentioning
confidence: 99%
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“…The discrepancy at higher pressures ͑p Ͼ 2700 Pa͒ occurs because the current model neglects the unsteady gas inertia term. An unsteady Boltzmann equation model 8,16 or a continuum regime slip-flow model 5 is expected to work better for such high pressures.…”
mentioning
confidence: 99%