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dc.contributor.authorKiang, David Tien Siken_US
dc.contributor.authorTam, Christopher Kwong Wahen_US
dc.contributor.authorKerrebrock, Jack L.en_US
dc.contributor.otherMassachusetts Institute of Technology. Gas Turbine Laboratoryen_US
dc.date.accessioned2016-10-06T21:22:00Z
dc.date.available2016-10-06T21:22:00Z
dc.date.issued1970en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/104691
dc.descriptionOctober 1970en_US
dc.descriptionIncludes bibliographical references (leaf 10)en_US
dc.description.abstractThe noise produced by convection of turbulence through an oblique shock wave has been measured and compared to theoretical predictions by Ribner and Kerrebrock. There is excellent agreement with the theoretical prediction that, for a fixed turbulent input, the downstream noise pressure (divided by the mean pressure), should first increase very rapidly, and then decrease as the normal Mach number of the shock is increased from unity to values of the order of 1.5. This behavior implies that a part of the noise from supersonic jets should behave similarly, with a sharp increase, then a decrease as the nozzle pressure ratio is raised from unity.en_US
dc.description.sponsorshipThis Research Carried Out in the Gas Turbine Laboratory, M.I.T., in Cooperation with Lewis Research Center, NASA, under Grant NGL 22-009-383en_US
dc.format.extent10 leavesen_US
dc.publisherCambridge, Mass. : Gas Turbine Laboratory , Massachusetts Institute of Technology, [1970]en_US
dc.relation.ispartofseriesGTL report #102en_US
dc.subject.lcshJet planes -- Noiseen_US
dc.subject.lcshShock wavesen_US
dc.subject.lcshTurbulenceen_US
dc.titleNoise generation by shock-turbulence interactionen_US
dc.typeTechnical Reporten_US
dc.identifier.oclc09673913en_US


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