A state-to-state model of H-2/He plasmas coupling the master equations for internal distributions of heavy species with the transport equation for the free electrons has been used as a basis for implementing a multi-temperature kinetic model. in the multi-temperature model internal distributions of heavy particles are Boltzmann, the electron energy distribution function is Maxwell, and the rate coefficients of the elementary processes become a function of local temperatures associated to the relevant equilibrium distributions. The slatedo-state and multi-temperature models have been compared in the case of a homogenous recombining plasma, reproducing the conditions met during supersonic expansion though converging-diverging nozzles.

Multi-temperature Model Derived from State-to-State Kinetics for Hypersonic Entry in Jupiter Atmosphere

Colonna G;D'Ammando G;Pietanza L D;Capitelli M
2014

Abstract

A state-to-state model of H-2/He plasmas coupling the master equations for internal distributions of heavy species with the transport equation for the free electrons has been used as a basis for implementing a multi-temperature kinetic model. in the multi-temperature model internal distributions of heavy particles are Boltzmann, the electron energy distribution function is Maxwell, and the rate coefficients of the elementary processes become a function of local temperatures associated to the relevant equilibrium distributions. The slatedo-state and multi-temperature models have been compared in the case of a homogenous recombining plasma, reproducing the conditions met during supersonic expansion though converging-diverging nozzles.
2014
Istituto di Nanotecnologia - NANOTEC
Inglese
AIP Conference Proceedings, AIP 29th RGD
1628
1162
1167
6
Sì, ma tipo non specificato
13-18 July 2014
Xi'an, China
elementary pmcesses in H-2/He plasma
state-to-state kinetics
multi-temperature model
recombining plasma
5
none
Colonna, G; D'Ambrosio, D; D'Ammando, G; Pietanza, L D; Capitelli, M
273
info:eu-repo/semantics/conferenceObject
04 Contributo in convegno::04.01 Contributo in Atti di convegno
   Planetary Entry Integrated Models
   PHYS4ENTRY
   FP7
   242311
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/268704
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