Characterization of kerosene distribution around the ignition cavity in a scramjet combustor

Kerosene distribution before its ignition in a scramjet combustor with dual cavity was measured using kerosene-PLIF under transverse injection upstream of the cavity and different injection pressures. The simulated flight condition is Ma 5.5, and the isolator entrance has a Mach number of 2.52, a to...

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Veröffentlicht in:Acta astronautica 2017-05, Vol.134, p.11-16
Hauptverfasser: Li, Xipeng, Liu, Weidong, Pan, Yu, Yang, Leichao, An, Bin, Zhu, Jiajian
Format: Artikel
Sprache:eng
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Zusammenfassung:Kerosene distribution before its ignition in a scramjet combustor with dual cavity was measured using kerosene-PLIF under transverse injection upstream of the cavity and different injection pressures. The simulated flight condition is Ma 5.5, and the isolator entrance has a Mach number of 2.52, a total pressure of 1.6MPa and a stagnation temperature of 1486K. Effects of injection pressure on fuel distribution characteristics were analyzed. The majority of kerosene is present in the cavity shear layer as well as its upper region. Kerosene extends gradually into the cavity, almost, at a constant angle. Large scale structures are evident on the windward side of kerosene. The cavity shear layer plays an important role in determining the kerosene distribution and its entrainment into the cavity. The middle part of cavity is the most suitable location for ignition as a result of a favorable local equivalent ratio. As the injection pressure increases, the penetration height gets higher with the rate of increase getting slower at higher injection pressure. Meanwhile, the portion of kerosene entrained into cavity through shear layer becomes smaller as injection pressure increases. However, the kerosene entrained into cavity still increase due to the increased mass flow rate of kerosene. •The cavity shear layer has great impact on kerosene entrainment into cavity.•Large scale structures are identified on the windward side of kerosene.•An unsteady and three-dimensional turbulent flow field is visualized around cavity.•The middle part of cavity is the most suitable location for ignition.
ISSN:0094-5765
1879-2030
DOI:10.1016/j.actaastro.2017.01.037