Mathematics
Scientific paper
Oct 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978odun.reptq....t&link_type=abstract
Final Report, 1 Jan. 1977 - 31 Mar. 1978 Old Dominion Univ., Norfolk, VA. Dept. of Mechanical Engineering and Mechanics.
Mathematics
Atmospheric Entry, Jupiter Atmosphere, Radiant Heating, Shock Heating, Flow Characteristics, Flow Equations, Helium, Hydrogen, Mathematical Models, Radiant Flux Density, Shock Layers
Scientific paper
Formulation is presented to demonstrate the significance of a simplified radiation model in investigating the flow phenomena in the viscous radiating shock layer of a Jovian entry body. The body configurations used are a 55 degree sphere cone and 50 degree hyperboloid. A nongray absorption model for hydrogen-helium gas is developed which consists of 30 steps over the spectral range of 0 to 20 eV. By employing this model, results were obtained for temperature, pressure, density, the shock layer and along the body surface. These are compared with results of two sophisticated radiative transport models available in the literature.
Subramanian S. V.
Tiwari S. N.
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