2014
DOI: 10.1103/physreve.90.013009
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Nonequilibrium shock-heated nitrogen flows using a rovibrational state-to-state method

Abstract: A rovibrational collisional model is developed to study the internal energy excitation and dissociation processes behind a strong shock wave in a nitrogen flow. The reaction rate coefficients are obtained from the ab initio database of the NASA Ames Research Center. The master equation is coupled with a one-dimensional flow solver to study the nonequilibrium phenomena encountered in the gas during a hyperbolic reentry into Earth's atmosphere. The analysis of the populations of the rovibrational levels demonstr… Show more

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Cited by 149 publications
(77 citation statements)
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“…The degeneracy (or statistical weight) and the energy of a given state i ∈ I are denoted by the symbols g i and E i , respectively. Alternatively, the rovibrational states of N 2 ( 1 Σ + g ) can be sorted according to their rotational (J) and vibrational (v) quantum numbers via the mapping functions [19,20]:…”
Section: Introductionmentioning
confidence: 99%
“…The degeneracy (or statistical weight) and the energy of a given state i ∈ I are denoted by the symbols g i and E i , respectively. Alternatively, the rovibrational states of N 2 ( 1 Σ + g ) can be sorted according to their rotational (J) and vibrational (v) quantum numbers via the mapping functions [19,20]:…”
Section: Introductionmentioning
confidence: 99%
“…The distance between the shock front and the position at which H 2 is half consumed is defined as the half-reaction thickness, δ. At 0.1 atm, when the collision frequency is low, the two-temperature model seems to overestimate the vibrational relaxation, as mentioned by Bender et al (2015) and Panesi et al (2014). These halfreaction thickness features are further demonstrated in Figure 3.…”
Section: D Testsmentioning
confidence: 65%
“…In addition, a collisional model has been elaborated by Panesi et al 15,16 and the assessment of the time required to reach a Boltzmanian distribution for the rotational distribution has been derived. The conditions n 0 ¼ 7.2 Â 10 22 m À3 , T 0 A ¼ 10 000 K have been studied for the total density and the kinetic temperature, respectively.…”
Section: Typesmentioning
confidence: 99%
“…(16). Finally, the rate coefficient of each backward elementary process is derived from the one of the forward elementary process using the detailed balance principle involving the Boltzmann, Guldberg and Waage and Saha equilibrium constants.…”
Section: Radiative Processesmentioning
confidence: 99%