1993
DOI: 10.2514/3.25468
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Navier-Stokes solutions with surface catalysis for Martian atmospheric entry

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Cited by 56 publications
(14 citation statements)
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“…The values of γ w are however consistent with those found in the literature, which also show a large variation. For example, East, Stalker & Baird (1980) use γ w ≈ 3 × 10 −3 which they regard as typical for oxygen and nitrogen recombination on oxidized metallic surfaces with a wall temperature of 300 K. In contrast, Anderson (1973) determined values of γ w using experimental measurements of stagnation-point heat transfer rates in supersonic flow and gave a value for metallic surfaces, including platinum, of 0.09 for 400 ± 100 K. The standard assumption is that γ w increases with temperature, but Chen & Chandler (1993) state, unusually, that it may also be a function of pressure. The free-stream pressures for cases 1 to 4 are included in table 9, and clearly there is no direct relationship between p and γ w in these flows.…”
Section: Comparison With Experimental Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…The values of γ w are however consistent with those found in the literature, which also show a large variation. For example, East, Stalker & Baird (1980) use γ w ≈ 3 × 10 −3 which they regard as typical for oxygen and nitrogen recombination on oxidized metallic surfaces with a wall temperature of 300 K. In contrast, Anderson (1973) determined values of γ w using experimental measurements of stagnation-point heat transfer rates in supersonic flow and gave a value for metallic surfaces, including platinum, of 0.09 for 400 ± 100 K. The standard assumption is that γ w increases with temperature, but Chen & Chandler (1993) state, unusually, that it may also be a function of pressure. The free-stream pressures for cases 1 to 4 are included in table 9, and clearly there is no direct relationship between p and γ w in these flows.…”
Section: Comparison With Experimental Resultsmentioning
confidence: 99%
“…Stewart, Rakich &Lanfranco 1983 andScott 1985 and references contained therein). Some more recent studies considered the effects of catalytic walls on a shock/boundary layer interaction (Grumet et al 1991), catalytic effects on a model of Martian atmospheric entry (Chen & Chandler 1993), and hypersonic flow past a sharp cone with finite catalytic walls (Miller et al 1995).…”
Section: Introductionmentioning
confidence: 99%
“…Relative to dissociation energy, vibrational energy is an order of magnitude more important in carbon dioxide than in nitrogen, see for example Rock et al 6 For Martian planetary entry, predicting the aerothermodynamic loading on a vehicle is critical and the role of thermochemical effects has been pointed out in numerous studies. [7][8][9] For example, the increase in transition Reynolds number with increasing stagnation enthalpy was found to be significantly more pronounced in carbon dioxide than in nitrogen. 10,11 In addition to its importance in flight, carbon dioxide thermochemistry can also be significant in flow acceleration to hypersonic velocities in ground testing facilities.…”
Section: A Thermochemistry Of Carbon Dioxide In Ground Test Facilitiesmentioning
confidence: 99%
“…In studying the Martian atmosphere entry, mainly the limit cases of an ideal catalytic surface (with a maximum rate of heterogeneous recombination of the dissociated carbon dioxide components) and a noncatalytic surface were considered in the literature [16][17][18]. Phenomenological models of the catalytic properties of heat-shield coatings of spacecraft entering the Martian atmosphere based on a detailed analysis of the heterogeneous catalytic reaction mechanism were suggested in [19,20].…”
Section: Introductionmentioning
confidence: 99%