INCAS Bulletin (Sep 2015)

Computations of the Shock Waves at Hypersonic Velocities Taken into Account the Chemical Reactions that Appear in the Air at High Temperatures

  • Mihai Leonida NICULESCU,
  • Marius Gabriel COJOCARU,
  • Mihai Victor PRICOP,
  • Dumitru PEPELEA

DOI
https://doi.org/10.13111/2066-8201.2015.7.3.12
Journal volume & issue
Vol. 7, no. 3
pp. 129 – 133

Abstract

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The temperature in the nose region of a hypersonic vehicle can be extremely high, for example, reaching approximately 11 000 K at a Mach number of 36 (Apollo reentry). The bow shock wave is normal, or nearly normal, in the nose region of a blunt body, and the gas temperature behind this shock wave can be enormous at hypersonic speeds. In this case, the assumption of a calorically perfect nonreacting gas with the ratio of specific heats  of 1.4 gives an unrealistically high value of temperature. Therefore, the proper inclusion of chemically reacting effects is vital to the calculation of an accurate normal shock wave temperature.

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