Significance of shock and body slip conditions on Jovian entry heating

Details Significance of shock and body slip conditions on Jovian entry heating Significance of shock and body slip conditions on Jovian entry heating

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979odun.reptq....t&link_type=abstract

Progress Report, Aug. 1978 - Dec. 1978 Old Dominion Univ., Norfolk, VA. Dept. of Mechanical Engineering and Mechanics.

Physics

Atmospheric Heating, Jupiter Atmosphere, Shock Loads, Slip Flow, Axisymmetric Flow, Finite Difference Theory, Iterative Solution, Laminar Flow, Steady Flow, Viscous Flow

Scientific paper

The influence of the body and shock slip conditions on the heating of a Jovian entry body is investigated. The flow in the shock layer is considered to be axisymmetric, steady, laminar, viscous, and in chemical equilibrium. Realistic thermophysical and step-function spectral models are employed and results are obtained by implicit finite-difference and iteractive procedures. The freestream conditions correspond to a typical Jovian entry trajectory point. The results indicate that the effect of the slip conditions is significant when the altitudes are higher than 225 km and that the contribution of a radiative heat-flux term in the energy equation should not be neglected at any altitude.

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