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An Empirical Method for Prediction of Hypersonic Rarefied Flow-Field Structure

An Empirical Method for Prediction of Hypersonic Rarefied Flow-Field Structure
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摘要 Numerical simulations are presented about the effects of gas rarefaction on hypersonic flow field.Due to the extremely difficult experiment,limited wind-tunnel conditions and high cost,most problems in rarefied flow regime are investigated through numerical methods,in which the direct simulation Monte-Carlo(DSMC)method is widely adopted.And the unstructured DSMC method is employed here.Flows around a vertical plate at a given velocity 7 500 m/s are simulated.For gas rarefaction is judged by the free-stream Knudsen number(Kn),two vital factors are considered:molecular number density and the plate′s length.Cases in which Kn varies from 0.035 to13.36 are simulated.Flow characters in the whole rarefied regime are described,and flow-field structure affected by Knis analyzed.Then,the dimensionless position D*of a certain velocity in the stagnation line is chosen as the marker of flow field to measure its variation.Through flow-field tracing and least-square numerical method analyzing,it is proved that hypersonic rarefied flow field expands outward linearly with the increase of 1/2Kn.An empirical method is proposed,which can be used for the prediction of the hypersonic flow-field structure at a given inflow velocity,especially the shock wave position. Numerical simulations are presented about the effects of gas rarefaction on hypersonic flow field. Due to the extremely difficult experiment, limited wind-tunnel conditions and high cost, most problems in rarefied flow regime are investigated through numerical methods, in which the direct simulation Monte-Carlo (DSMC) method is widely adopted. And the unstructured DSMC method is employed here. Flows around a vertical plate at a given velocity 7 500 m/s are simulated. For gas rarefaction is judged by the free stream Knudsen number (Kn), two vi- tal factors are considered: molecular number density and the plate's length. Cases in which Kn varies from 0. 035 to 13.36 are simulated. Flow characters in the whole rarefied regime are described, and flow field structure affect- ed by Kn is analyzed. Then, the dimensionless position D~ of a certain velocity in the stagnation line is chosen as the marker of flow field to measure its variation. Through flow-field tracing and least-square numerical method an- alyzing, it is proved that hypersonic rarefied flow field expands outward linearly with the increase of √Kn. An empirical method is proposed, which can be used for the prediction of the hypersonic flow field structure at a given inflow velocity, especially the shock wave position.
出处 《Transactions of Nanjing University of Aeronautics and Astronautics》 EI CSCD 2017年第5期543-552,共10页 南京航空航天大学学报(英文版)
关键词 hypersonic rarefied flow KN direct simulation Monte-Carlo(DSMC)mothod linear expansion flowfield prediction hypersonic rarefied flow Kn direct simulation Monte Carlo (DSMC) mothod linear expansion flow field prediction
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