The Physics of Asymptotic High-Speed Flow Regimes I: Thermodynamics and Kinetics

21 Sept 2026, 11:00
30m
The Angevin Castle (Mola Di Bari)

The Angevin Castle

Mola Di Bari

Lungomare Dalmazia, 70042 Mola di Bari (BA) Italy
Ablative-Radiative TPS and Meteors Radiation modeling and simulation

Speaker

Mario Lino da Silva (Instituto de Plasmas e Fusão Nuclear - Instituto Superior Tecnico)

Description

What are the asymptotic limits of high-speed flows? Many years ago, it was postulated that post-shock temperatures would eventually reach a cap postulated to be around 20,000K, as increasing shock speeds would lead to endothermic processes offsetting the additional energy processed through the shock. These include, the excitation of a plethora of higher energy levels known to exist near dissociation and ionization thresholds for the flow species, dissociation and ionization reactions, and finally radiation which would lead to additional energy bleeding away from the shock layer.

The first part of this work discusses different updates to kinetic and thermodynamic models for air, capable of modeling the physical-chemical properties of plasmas at such high temperatures and ionization levels. We will point out additional theoretical hurdles in defining thermodynamic properties at extremely high temeratures, and the implications on the principle of detailed balance.

Radiative effects, modeled in a loose coupling, are discussed in a separate part II presentation.

Summary

First part of a work describing the development of a detailed aerothermal model valid at assymptotic velocities in excess of 20km/s.

Authors

Mario Lino da Silva (Instituto de Plasmas e Fusão Nuclear - Instituto Superior Tecnico) Tiago Garrão

Presentation materials

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