2016
DOI: 10.2514/1.t4549
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Air Collisional-Radiative Modeling with Heavy-Particle Impact Excitation Processes

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Cited by 15 publications
(9 citation statements)
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“…Figure shows the results of heavy-particle impact excitation rate measurements as well as theoretical predictions on an Arrhenius plot. Although a few estimates exist for electronic excitation rates due to N–N, N–O, and O–O collisions (relevant to high-temperature air CR models , ), to the authors’ knowledge, these are the first direct shock tube measurements of O* formation rates by O–Ar collisions. Best fits of the current experiments were obtained using the format k M (1, i ) = A T b exp­(− C / T ), where the temperature dependence term b was fixed at 1/2 to match the dependence from the theoretical formulation, the activation energy term C was set to E i (in K), and the best fit was determined by varying the parameter A .…”
Section: Shock Tube Experimentsmentioning
confidence: 99%
See 1 more Smart Citation
“…Figure shows the results of heavy-particle impact excitation rate measurements as well as theoretical predictions on an Arrhenius plot. Although a few estimates exist for electronic excitation rates due to N–N, N–O, and O–O collisions (relevant to high-temperature air CR models , ), to the authors’ knowledge, these are the first direct shock tube measurements of O* formation rates by O–Ar collisions. Best fits of the current experiments were obtained using the format k M (1, i ) = A T b exp­(− C / T ), where the temperature dependence term b was fixed at 1/2 to match the dependence from the theoretical formulation, the activation energy term C was set to E i (in K), and the best fit was determined by varying the parameter A .…”
Section: Shock Tube Experimentsmentioning
confidence: 99%
“…Lemal et al , recently used a CR model for high-temperature air to analyze shock tube radiation measurements. Data were acquired behind fast incident shocks (∼10–11 km/s) traveling in low-pressure (∼13 Pa) air; kinetic temperatures initially behind shock waves were ∼6 × 10 4 K, quickly falling to ∼1 × 10 4 K after less than 2 μs.…”
Section: Introductionmentioning
confidence: 99%
“…The nonequilibrium chemical kinetics of atmospheric re-entry flows have been studied extensively since the 1960s. A typical earth atmospheric re-entry flow, such as in the Fire II flight experiment launched within the framework of the Apollo program, can reach Mach >30 and a stagnation gas temperature above 11,000 K. ,, At such high temperatures, the constituents of air become partially ionized, and radiative heating can contribute to over 30% of the total heat flux. , In such high-speed re-entry systems, the excited atomic species, O* and N*, play important roles in radiative heating/cooling. For proper design of the thermal protection system for space vehicles, it is thus crucial to understand the fundamental kinetics of the excited atomic species at extreme temperatures.…”
Section: Introductionmentioning
confidence: 99%
“…A variety of detailed chemistry models are available in the literature [2,[48][49][50][51]. Most of them are hybrid models combining a state-to-state approach, for part of the internal energy levels populations, together with a multitemperature approach, assuming that the rest of the energy level populations follow Boltzmann distributions at their relevant temperature.…”
Section: Mixture Description and Chemical Mechanismmentioning
confidence: 99%