1994
DOI: 10.2514/3.496
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Review of chemical-kinetic problems of future NASA missions. II - Mars entries

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Cited by 705 publications
(327 citation statements)
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“…15) and varies up to 1.5 times for different models; its minima and maxima are shifted towards the shock front for the models. 69,70 Concluding these results we can recommend the use of the Scanlon model 70 for reaction #1 at high temperatures, providing a more reliable behavior of the fluid dynamic variables and energy fluxes.…”
Section: B Transport Properties and Heat Fluxesmentioning
confidence: 99%
See 1 more Smart Citation
“…15) and varies up to 1.5 times for different models; its minima and maxima are shifted towards the shock front for the models. 69,70 Concluding these results we can recommend the use of the Scanlon model 70 for reaction #1 at high temperatures, providing a more reliable behavior of the fluid dynamic variables and energy fluxes.…”
Section: B Transport Properties and Heat Fluxesmentioning
confidence: 99%
“…Indeed, the model 64 may be not applicable under such high-temperature conditions. For this reason, we assess three different data sets for reaction #1: the McKenzie model 64 and the models of Park 69 and Scanlon. 70 A comparison of the rate coefficients k 1 ðTÞ for nitrogen (see Fig.…”
Section: B Transport Properties and Heat Fluxesmentioning
confidence: 99%
“…The §ow has been modeled as a reacting gas mixture of 9 species (Ar, CO 2 , N 2 , O 2 , CO, NO, N, O, and C). Reaction mechanism and chemical kinetics taken into account in the present work are from [6,13].…”
Section: Reentrymentioning
confidence: 99%
“…For the di¨usion coe©cient of the ith species in the mixture, the multicomponent di¨usion coe©cient is applied, where species mass di¨usivity is evaluated by Kinetic Theory [5]. Flow¦eld chemical reactions proceed with forward rates that are expressed in the Arrhenius form and reaction rate parameters are due to Park et al [13].…”
Section: Design Analysis Based On Computational Fluid Dynamicsmentioning
confidence: 99%
“…Simulation of thermochemical interaction between high-enthalpy §ows of air and other gases and heat-protective materials (HPM) in high-enthalpy WTs for §ight conditions of bodies with hypersonic speeds in atmosphere of the Earth, Mars, and other planets is among key problems of air thermodynamics [1].…”
Section: Introductionmentioning
confidence: 99%