44th AIAA Thermophysics Conference 2013
DOI: 10.2514/6.2013-2634
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Coupled Flow Field Simulations of Charring Ablators with Nonequilibrium Surface Chemistry

Abstract: This paper describes the coupling of a Navier-Stokes solver to a material response code to simulate nonequilibrium gas-surface interactions. The Navier-Stokes solver used in this study is LeMANS, which is a three-dimensional computational fluid dynamics code that can simulate hypersonic reacting flows including thermo-chemical nonequilibrium effects. The material response code employed in this study is MOPAR, which uses the one-dimensional control volume finite-element method to model heat conduction and pyrol… Show more

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Cited by 12 publications
(11 citation statements)
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References 26 publications
(18 reference statements)
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“…In addition, since the gas is eventually blown into the chemical reacting boundary layer [6], correct modeling of the pyrolysis gas is also important to help determine the surface boundary conditions. The gas flow within the charring ablator is often modeled as a porous media flow, for which steady-state Darcy's law is usually assumed [7][8][9][10].…”
mentioning
confidence: 99%
“…In addition, since the gas is eventually blown into the chemical reacting boundary layer [6], correct modeling of the pyrolysis gas is also important to help determine the surface boundary conditions. The gas flow within the charring ablator is often modeled as a porous media flow, for which steady-state Darcy's law is usually assumed [7][8][9][10].…”
mentioning
confidence: 99%
“…Pyrolysis is the process in which the phenolic polymer gradually carbonizes at high temperature, losing mass and generating pyrolysis gases. These gases are then expelled through the porous structure of the material and blown into the chemical reacting boundary layer [2]. The other phenomenon, ablation, occurs in a thin layer near the surface, and it refers to the mass removal of the char (composed of nonpyrolyzed and residual carbonized material) through oxidation, sublimation, and spallation.…”
mentioning
confidence: 99%
“…NASA's Stardust project in 2006 reentered the Earth's atmosphere from a solar orbit at a record 12.9 km/s [24], placing it still behind the 15 km/s prediction for Martian return missions. Measurement of the flow temperature within the plasma sheath surrounding Stardust was not directly measurable, however simulations by Alkandry et al in 2013 using the LeMANS hypersonic flow solver predicted a peak temperature of approximately 50, 000K whilst showing good agreement with the heat shield surface temperature measurements of ground based spectroscopy [75,2].…”
Section: The 5 11 and Doubly-ionized Species Gas Models For Airmentioning
confidence: 97%
“…Here an appreciable fraction of doubly-ionized monatomic plasma was predicted above temperatures of 30, 000K for both species. At the predicted 50, 000K produced during solar orbit reentry speeds [2], the molar fraction of second order ions O 2+ and N 2+ and higher is expected to be in excess of 90% [73,1,9].…”
Section: The 5 11 and Doubly-ionized Species Gas Models For Airmentioning
confidence: 98%
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