Effect of a finite ionization rate on the radiative heating of outer planet atmospheric entry probes

Details Effect of a finite ionization rate on the radiative heating of outer planet atmospheric entry probes Effect of a finite ionization rate on the radiative heating of outer planet atmospheric entry probes

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982umo..rept.....n&link_type=abstract

Final Report Missouri Univ., Rolla. Dept. of Mechanical and Aerospace Engineering.

Physics

Atmospheric Entry, Gas Flow, Heat Shielding, Inviscid Flow, Ionization, Radiative Heat Transfer, Helium, Hydrogen, Shock Waves, Stagnation Flow, Wall Flow

Scientific paper

The influence of finite rate ionization in the inviscid gas just behind the stagnation shock wave on the radiative heating of probes entering the hydrogen-helium atmosphere of the major plants was investigated. Two opposing conclusions were reached as to how the ionization rate assumption affects the radiative transfer. Hydrogen-helium shock waves with a cold nonblowing wall boundary condition at the probe heat shield are emphasized. The study is limited to the stagnation shock layer.

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