Assessment of CFD capability for prediction of hypersonic shock interactions

Knight, Doyle; Longo, J.M.A.; Drikakis, Dimitris; Gaitonde, Datta V.; Lani, Andrea; Nompelis, Ioannis; Reimann, Bodo; Walpot, L.

doi:10.1016/j.paerosci.2011.10.001

Cited by 121 publications

(59 citation statements)

References 29 publications

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“…Another comprehensive effort, again with teams working under the umbrella of AFOSR and RTO/AVT programs, culminated in a series of simulations, with high-temperature effects, which are summarized in a review article by Knight et al [118]. Fig.…”

Section: Heat Transfer and Skin Friction Coefficientmentioning

confidence: 99%

Progress in shock wave/boundary layer interactions

Gaitonde

2015

Progress in Aerospace Sciences

521

126

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Section: Heat Transfer and Skin Friction Coefficientmentioning

confidence: 99%

Progress in shock wave/boundary layer interactions

Gaitonde

2015

Progress in Aerospace Sciences

521

126

View full text Add to dashboard Cite

“…In our numerical model, both the electromagnetic and flow field equations are discretized by means of a second-order accurate finite volume method implemented within COOLFluiD, [43][44][45][46][47] an open computational platform for multi-physics and plasma 30, 48-50 in particular. The COOLFluiD ICP solver relies upon the AUSM+up scheme 51 for discretizing convective fluxes and upon a central treatment of diffusive fluxes.…”

Section: Methodsmentioning

confidence: 99%

Modeling of Non-equilibrium Plasmas in an Inductively Coupled Plasma Facility

Zhang

Lani

Chew³

et al. 2014

45th AIAA Plasmadynamics and Lasers Conference

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This paper presents the results of the numerical simulation of plasma flows inside the torch of the VKI inductively coupled plasma facility. The main purpose of this work is the parametric investigation of thermo-chemical non-equilibrium effects on the plasma jet at different operating pressures ranging from 3 to 15 kPa. The test gas is an ionized air mixture including eleven species. While the induced electric field inside the torch is computed by solving Helmholtz induction equation, a standard two-temperature formulation is used to account for non-equilibrium effects. In particular, the present analysis assesses the impact of different models for chemical kinetics and for vibration-chemistry-vibration coupling on the resulting plasma field. Solutions previously computed assuming LTE conditions are used as a reference for our benchmarks. Considerable differences on both the induced electric and temperature field are highlighted for the lower pressure cases.

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“…The latter is an open-source platform for high-performance scientific computing 3 featuring advanced computational models/ solvers for tackling re-entry aerothermodynamics (Degrez et al 2009;Lani et al 2013a;Munafo et al 2013;Garicano Mena et al 2015), simulation of experiments in highenthalpy facilities (Knight et al 2012;Zhang et al 2016), ideal magnetohydrodynamics for space weather prediction (Yalim et al 2011;Lani et al 2014), radiation transport by means of ray tracingand Monte Carlo (Santos & Lani 2016) algorithms, etc.…”

Section: Numerical Schemes and Boundary Conditionsmentioning

confidence: 99%

Multi-fluid Modeling of Magnetosonic Wave Propagation in the Solar Chromosphere: Effects of Impact Ionization and Radiative Recombination

Maneva

Laguna

Lani

et al. 2017

ApJ

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In order to study chromospheric magnetosonic wave propagation including, for the first time, the effects of ionneutral interactions in the partially ionized solar chromosphere, we have developed a new multi-fluid computational modelaccounting for ionization and recombination reactions in gravitationally stratified magnetized collisional media. The two-fluid model used in our 2D numerical simulations treats neutrals as a separate fluid and considers charged species (electrons and ions) within the resistive MHD approach with Coulomb collisions and anisotropic heat flux determined by Braginskiis transport coefficients. The electromagnetic fields are evolved according to the full Maxwell equations and the solenoidality of the magnetic field is enforced with a hyperbolic divergence-cleaning scheme. The initial density and temperature profiles are similar to VAL III chromospheric model in which dynamical, thermal, and chemical equilibrium are considered to ensure comparison to existing MHD models and avoid artificial numerical heating. In this initial setup we include simple homogeneous flux tube magnetic field configuration and an external photospheric velocity driver to simulate the propagation of MHD waves in the partially ionized reactive chromosphere. In particular, we investigate the loss of chemical equilibrium and the plasma heating related to the steepening of fast magnetosonic wave fronts in the gravitationally stratified medium.

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Assessment of CFD capability for prediction of hypersonic shock interactions

Cited by 121 publications

References 29 publications

Progress in shock wave/boundary layer interactions

Progress in shock wave/boundary layer interactions

Modeling of Non-equilibrium Plasmas in an Inductively Coupled Plasma Facility

Multi-fluid Modeling of Magnetosonic Wave Propagation in the Solar Chromosphere: Effects of Impact Ionization and Radiative Recombination

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