Published April 15, 2025 | Version Published
Journal Article

Ionization induced by fluid–solid interaction during hypervelocity impact

  • 1. ROR icon Virginia Tech
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon United States Naval Research Laboratory

Abstract

This paper presents a computational model to represent and investigate hypervelocity impacts that occur in an atmospheric environment, focusing on energy partitions and impact-induced ionization. The computational domain includes the projectile, the target, and the ambient gas. The physical model combines the compressible Navier–Stokes equations, a complete thermodynamic equation of state (EOS) for each material, and a non-ideal, multi-species Saha equation for ionization prediction. Material interfaces are tracked using an extended two-equation level set method, and the interfacial mass, momentum, and energy fluxes are computed by the FIVER (FInite Volume method with Exact multi-material Riemann problems) method. Using this model, the impact of tantalum on soda-lime glass (SLG) within argon gas is analyzed. Shock compression experiments are conducted to capture the thermodynamics of SLG under high pressure and temperature, yielding shock Hugoniot data up to 112 GPa and 5300 K. This data is used to calibrate a Noble-Abel stiffened gas EOS. Impact simulations are performed with initial velocity ranging from 3 km / s to 7 km / s . Time histories of the pressure, temperature, and plasma density fields are compared across the three materials. Less than 1% of the total impact energy is transferred to the ambient gas, yet its specific internal energy is of the same order of magnitude as that of the projectile and target. Argon gas exhibits higher temperature and plasma density than SLG and tantalum. The ionization of SLG is found to be highly selective, with the metallic elements contributing over 99.9% of the plasma's charged particles despite comprising less than 15% of the molar composition. In general, the results suggest that the plasma's density and energy depend on both impact velocity and the material combination, including the ambient gas. The plasma's composition further reflects the properties (e.g., ionization energies) of the chemical elements in each material.

Copyright and License

© 2025 Elsevier Ltd. All rights are reserved, including those for text and data mining, AI training, and similar technologies.

Acknowledgement

S.T.I, A.N., and K.W. gratefully acknowledge the support of the U.S. Office of Naval Research (ONR) under awards N00014-19-1-2102 and N00014-24-1-2509, the support of the U.S. Air Force Office of Scientific Research under contract No. FA9550-22-C-001, and the support of the National Science Foundation (NSF), United States under award CBET-1751487. J.G.M. gratefully acknowledges the support of ONR through U.S. Naval Research Laboratory’s core funding. PDA gratefully acknowledges support from ONR, United States under awards N00014-16-1-2751, N00014-17-1-2772, N00014-18-1-2712, and N00014-20-1-2603.

Conflict of Interest

The authors declare the following financial interests/personal relationships which may be considered as potential competing interests: The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Additional details

Funding

Office of Naval Research
N00014-19-1-2102
Office of Naval Research
N00014-24-1-2509
United States Air Force Office of Scientific Research
FA9550-22-C-001
National Science Foundation
CBET-1751487
United States Air Force Research Laboratory
Office of Naval Research
N00014-16-1-2751
Office of Naval Research
N00014-17-1-2772
Office of Naval Research
N00014-18-1-2712
Office of Naval Research
N00014-20-1-2603

Dates

Accepted
2025-02-04
Available
2025-02-12
Available online
Available
2025-02-16
Version of record

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)
Publication Status
Published