Abstract
Results of computational work demonstrating magnetogasdynamic flow control within the internal inlet of a full-scale, Mach 10 scramjet engine simulation are presented. As part of the analysis, a control volume approach with an electron beam ionization model is presented for the first time in the context of the established computational method used. We conclude that applying magnetogasdynamic interaction entirely upstream of a expansion-induced flow separation zone was not effective at improving the inlet efficiency. For most parameters tested, any pressure gains incurred in the region of electromagnetic interaction were all but negated by an additional sidewall expansion at the inlet throat. Magnetogasdynamic acceleration can efficiently reduce the net inlet drag in some cases while minimizing the increase in heat transfer and decrease in overall efficiency measures. Finally, placement of the electromagnetic interaction region near the wall was the most important factor in determining the wall heat transfer and proved to be a relatively efficient method for limiting drag increases. However, further work is recommended to determine the optimum distance from the wall to target the electron beam ionization. '
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