Stagnation Point Flow of a Radiating Gas of a Large Optical Thickness
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概要
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This paper deals theoretically with the stagnation point flow of a radiating gas when the global optical thickness is large. The radiative heat transfer is assumed to be of the same order of magnitude as the convective one and the Mach number is assumed to be small A method of solution is used in which the isentropic outer flow, the diffusive (Rosseland type) layer flow and the radiation layer flow are considered successively. Actual analysis has been carried out to the second approximation correct to the order of the inverse square root of the Bouguer number. Effects due to the radiation slip are studied in detail. Numerical results are also obtained for the distributions of the flow velocity and the temperature in the diffusive layer and the radiation layer. They are compared with those of a radiative boundary layer flow on a flat plate.
- 社団法人日本物理学会の論文
- 1974-01-15
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