Theory of heat transfer to a shock-tube end-wall from an ionized monatomic gas

Author:

Fay James A.,Kemp Nelson H.

Abstract

This paper deals with the calculation of the convective heat transfer rate to the end-wall of a shock tube from a monatomic gas heated by a reflected shock. We consider a range of shock strengths for which the equilibrium thermodynamic state is one of appreciable ionization. The resulting boundary-layer problem involves the thermal conductivity and ambipolar diffusion coefficient for a partially ionized monatomic gas. The formulation here is restricted to the case of a catalytic wall and equal temperatures for all species. We ignore the effect of the plasma sheath at the wall. Consideration is given to three limiting cases for which similarity-type solutions of the boundary-layer equations may be found: (1) complete thermodynamic equilibrium behind the reflected shock and within the boundary layer; (2) equilibrium behind the reflected shock, but no gas-phase recombination in the boundary layer; (3) no ionization in either region. Numerical calculations are carried out for argon using estimated values of thermal conductivity and ambipolar diffusion, and compared with shock-tube experiments of Camac & Feinberg (1965). For no ionization, calculations were made with thermal conductivity varying as the ¾ power of the temperature, which fits the estimates of Amdur & Mason (1958) up to 15,000°K. Excellent agreement with experiment is obtained confirming an extrapolation of this power law up to 75,000°K. For ionized cases, based on estimates of Fay (1964), the theory predicts heating rates 20–40% lower than measured values. Some possible reasons for this discrepancy are discussed.

Publisher

Cambridge University Press (CUP)

Subject

Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics

Reference18 articles.

1. Camac, M. & Teare, J. D. 1964 Avco-Everett Res. Lab. Res. Rep. no. 183.

2. Kemp, N. H. 1964 Dept. Mech. Eng. Fluid Mech. Lab., M.I.T., Cambridge, Pub. no. 64–6.

3. Lauver, M. R. 1964 Phys. Fluids,7,611.

4. Hornbeck, J. 1951 Phys. Rev. 84,615.

5. Camac, M. & Kemp, N. H. 1963 Amer. Inst. Aero. Astro. Paper no. 63–460.

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