2012
DOI: 10.1017/s0001924000007302
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Numerical simulations of the flow through the inlet and isolator of a Mach 4 dual mode scramjet

Abstract: Results from numerical simulations of the three dimensional flow in the intake-isolator of a dual mode scramjet are presented. The FANS calculations have utilised the SST k-ω turbulence model. The effect of cowl length and cowl convergence angle on the inlet mass capture ratio, flow distortion, shock strength and pressure rise are studied in detail. Three cowl lengths and four or five cowl convergence angles for each cowl length are considered. The predicted values of the dimensionless wall static pressure and… Show more

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Cited by 13 publications
(2 citation statements)
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“…Additionally unstart due to back pressure created by the combustor has been noticed to be depending upon inlet geometry, contraction ratio and isolator length. Later Janarthanam and Babu (2012) have performed computational study employing Emami's intake geometry and experimental conditions. Three different cowl lengths and five cowl convergence angles were re-investigated computationally.…”
Section: Introductionmentioning
confidence: 99%
“…Additionally unstart due to back pressure created by the combustor has been noticed to be depending upon inlet geometry, contraction ratio and isolator length. Later Janarthanam and Babu (2012) have performed computational study employing Emami's intake geometry and experimental conditions. Three different cowl lengths and five cowl convergence angles were re-investigated computationally.…”
Section: Introductionmentioning
confidence: 99%
“…Azam Che Idris et al, Suggested Y+ values less than 1 to simulate shock wave boundary layer interactions in hypersonic intake [4]. Senthil kumar et al, have performed CFD simulations on SCRAMJET Inlet and noticed the direct effect of loss in total pressure recovery, inlet unsteadiness and flow distortion due to increase in cowl angle [5]. Janarthanam et al, CFD results of three-dimensional flow in the dual mode scramjet intake-isolator are agreed with experimental results at Mach 4 using SST k-ω turbulence model [6].…”
Section: Literature Reviewmentioning
confidence: 99%