Document Type
Article
Publication Date
1-2011
Abstract
The multispecies Boltzmann equation is numerically integrated to characterize the internal structure of a Mach 3 shock wave in a hard sphere gas. The collision integral is evaluated by the conservative discrete ordinate method [F. G. Tcheremissine, Comput. Math. Math. Phys. 46, 315 (2006)]. There was excellent agreement of macroscopic variables [Kosuge et al., Eur. J. Mech. B/Fluids 20, 87 (2001)]. The effect of species concentration and mass ratio on the behavior of macroscopic variables and distribution functions in the structure of the shock wave is considered for both two- and three-species gas mixtures. In a binary mixture of gases with different masses and varying concentrations, the temperature overshoot of the parallel component of temperature near the center of the shock wave is highest for the heavy component when the concentration of the heavy component is the smallest. The rise in the parallel component of temperature is revealed by the behavior of the distribution function.
Source Publication
Physics of Fluids
Recommended Citation
Eswar Josyula, Prakash Vedula, William F. Bailey, Casimir J. Suchyta; Kinetic solution of the structure of a shock wave in a nonreactive gas mixture. Physics of Fluids 1 January 2011; 23 (1): 017101. https://doi.org/10.1063/1.3541815
Comments
© 2011 Authors(s), published under an exclusive license with American Institute of Physics.
AFIT Scholar, as the repository of the Air Force Institute of Technology, furnishes the published Version of Record for this article in accordance with the sharing policy of the publisher, AIP Publishing. A 12-month embargo was observed.
This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in Physics of Fluids 23: 017101 as fully cited below and may be found at the DOI: 10.1063/1.3541815
Funding note: Support is provided by U.S. Air Force Office of Scientific Research contract monitored by F. Fahroo.