Dissociative recombination in reactive flows related to planetary atmospheric entries - Archive ouverte HAL
Communication Dans Un Congrès Année : 2015

Dissociative recombination in reactive flows related to planetary atmospheric entries

Résumé

The Dissociative Recombination (DR) processes play a significant role in plasma chemistry. This article illustrates this role from the modeling point of view in the case of reactive flows related to atmospheric entry plasmas. Two situations are investigated, for which the studied plasma is nitrogen. The first configuration corresponds to the relaxation process behind a strong shock wave moving at high Mach number in a shock tube, the second one to the recombination taking place in an expanding plasma flowing in a diverging nozzle. In both cases, the collisional-radiative model CoRaM-N-2, involving N-2, N, N-2(+), N+ and electrons, is implemented in an Eulerian 1D code able to compute the aerodynamic fields; calculations are performed in standard conditions. We show that, according to the rate coefficients used for the DR processes, the population density of the charged species especially N-2(+) is strongly modified only for the post-shock flow.

Dates et versions

hal-01459293 , version 1 (07-02-2017)

Identifiants

Citer

Arnaud Bultel, Julien Annaloro, Marie-Claude Druguet. Dissociative recombination in reactive flows related to planetary atmospheric entries. DR2013: NINTH INTERNATIONAL CONFERENCE ON DISSOCIATIVE RECOMBINATION: THEORY, EXPERIMENT, AND APPLICATIONS, 2015, Unknown, Unknown Region. ⟨10.1051/epjconf/20158406005⟩. ⟨hal-01459293⟩
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