A 23-species State-to-State (StS) thermochemical model for H₂/He mixtures is developed and used to simulate 1-D shocks at conditions relevant for ice and gas giant entry flows. To implement this StS model, a literature review of the state-specific excitation and ionization rates of atomic H is first performed. While electron impact rates from various sources are found to be in relatively good agreement, large discrepancies are found in the limited data available on heavy particle impact rates. To investigate the impact of these discrepancies on the predicted shock and radiance profiles, simulations are performed for three different versions of the kinetic model, each with a different set of heavy particle impact rates from the literature. Of these three models, two are found to over-predict and one is found to under-predict the radiance values seen in corresponding experimental data from the NASA Ames Electric Arc Shock Tube (EAST) facility. A sensitivity analysis to the electron and heavy particle impact rates is then performed, from which an improved kinetic model with modified rates is proposed. This modified kinetic model is found to reproduce the total integrated radiance from one of the EAST shot conditions reasonably accurately. However, some discrepancies are still found in the relative contributions to the total radiance from different spectral features, suggesting that additional improvements to the kinetic model still need to be made.
Published January 2024
| Published
Conference Paper
State-Specific Kinetic Modeling for Predictions of Radiative Heating in H₂/He Entry Flows
Abstract
Copyright and License
© 2024 by the American Institute of Aeronautics and Astronautics, Inc.
Acknowledgement
This work is supported by the NASA entry systems modeling project under grant number 80NSSC21K1751.
Additional details
- National Aeronautics and Space Administration
- 80NSSC21K1751
- Other Numbering System Name
- AIAA Paper
- Other Numbering System Identifier
- 2024-1482