Nonmonotonic dependence of a convective heat flux on the blowing rate of opaque admixtures blown into a radiative H-He shock layer

Physics

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Atmospheric Entry, Blunt Bodies, Convective Heat Transfer, Gas Injection, Jupiter Atmosphere, Radiative Heat Transfer, Shock Layers, Ablative Materials, Blowing, Gas Flow, Graphite, Heat Flux, Helium, Hydrogen, Navier-Stokes Equation, Opacity, Viscous Flow

Scientific paper

Results are presented for an analysis of radiative transfer and convective transport in a radiative H-He shock layer near the critical point of a blunt body when graphite ablation products are blowing off the body's surface. It is found that, for shock-layer conditions that would be typical for the motion of an entry probe in the atmosphere of Jupiter, the dependence of the convective heat flux on the rate at which the ablation products are blowing off the surface is substantially monotonic in nature. The maximum convective flux produced at a certain blowing rate is shown to be commensurate with the radiative flux to the surface.

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