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- W2317325519 abstract "A prediction procedure is described for efficiently obtaining off-stagnation solutions to the radiation-coupled, shocklayer equations that govern the heating events of hypervelocity entry into outer-planet atmospheres. Nonsimilar and turbulent transport terms have been developed and incorporated into an existing predictive procedure of the integral matrix type. The procedure is an inverse one which assumes a shock shape, then proceeds downstream, predicting a body shape. Reasonable comparison has been made with laboratory data, and with predictions of other investigators. Solutions presented are useful for the designers of the probe heatshield. Nomenclature = viscous density ratio, py/peu C = frozen specific heat, ZCpl-x^ D = binary diffusion coefficient f = stream function h = static enthalpy HT = total enthalpy j = diffusive mass flux k = von Karman's constant (0.44) £ = turbulent mixing length" @default.
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- W2317325519 date "1979-06-04" @default.
- W2317325519 modified "2023-09-28" @default.
- W2317325519 title "Methods for predicting off-stagnation point flowfields for planetary entry probes" @default.
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- W2317325519 doi "https://doi.org/10.2514/6.1979-1083" @default.
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