The influence of precursor heating on viscous chemical nonequilibrium radiating flow around a Jovian entry body is investigated. Results obtained for a 45 deg hyperboloid blunt body entering the Jupiter's nominal antmosphere at zero angle of attack indicate that the nonequilibrium radiative heating rate is significantly higher than the corresponding equilibrium heating. The precursor heating, in general, increases the radiative and convective heating to the body and this increase is slightly higher for the nonequilibrium conditions. (DePo)
Effects of precursor heating on chemical and radiative nonequilibrium viscous flow around a Jovian entry body
Wirkung einer stossweisen Erwaermung auf das chemische und ausstrahlende Ungleichgewicht einer viskosen Stroemung in die Jupiter Atmosphaere
AIAA-Papers ; 1-9
1978
9 Seiten, 13 Bilder, 1 Tabelle, 18 Quellen
Aufsatz (Konferenz)
Englisch
Nonequilibrium radiative heating of a Jovian entry body
AIAA | 1979
|Influence of precurser heating on viscous flow around a Jovian entry body
Tema Archiv | 1978
|