An 11-species model with state-specific atomic H kinetics reproduces experimental radiance profiles from H2/He shocks and improves ionization and radiation predictions compared to alternate models.
Aeroheating U ncertainties in Uranus and Saturn Entries by the Monte Carlo Method
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State-Specific Kinetic Modeling of Atomic H for H$_2$/ He Entry Flows
An 11-species model with state-specific atomic H kinetics reproduces experimental radiance profiles from H2/He shocks and improves ionization and radiation predictions compared to alternate models.