Numerical studies on supersonic spray combustion in high-temperature shear flows in a scramjet combustor

被引:18
作者
Ren, Zhaoxin [1 ]
Wang, Bing [2 ]
Zheng, Longxi [1 ]
Zhao, Dan [3 ]
机构
[1] Northwestern Polytech Univ, Sch Power & Energy, Xian 710072, Shaanxi, Peoples R China
[2] Tsinghua Univ, Sch Aerosp Engn, Beijing 100084, Peoples R China
[3] Univ Canterbury, Coll Engn, Dept Mech Engn, Private Bag 4800, Christchurch 8140, New Zealand
基金
中国国家自然科学基金;
关键词
Combustion; Flame kernel; Mixing layer; Numerical simulation; Shearing vortex; Spray flame; Supersonic flow; REACTING MIXING LAYER; LIQUID-FUEL SPRAY; AMBIENT-PRESSURE; FLAMELET MODEL; N-HEPTANE; IGNITION; GAS; SIMULATIONS; PARTICLE; EVAPORATION;
D O I
10.1016/j.cja.2018.06.020
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Numerical simulation is applied to detail the combustion characteristics of n-decane sprays in highly compressible vortices formed in a supersonic mixing layer. The multi-phase reacting flow is modeled, in which the shear flow is solved Eulerianly by means of direct numerical simulation, and the motions of individual sub-grid point-mass fuel droplets are tracked Lagrangianly. Spray combustion behaviors are studied under different ambient pressures. Results indicate that ignition kernels are formed at high-strain vortex braids, where the scalar dissipation rates are high. The flame kernels are then strongly strained, associated with the rotation of the shearing vortex, and propagate to envelop the local vortex. It is observed that the flammable mixtures entrained in the vortex are burned from the edge to the core of the vortex until the reactants are completely consumed. As the ambient pressure increases, the high-temperature region expands so that the behaviors of spray flames are strongly changed. An overall analysis of the combustion field indicates that the time-averaged temperature increases, and the fluctuating pressure decreases, resulting in a more stable spray combustion under higher pressures, primarily due to the acceleration of the chemical reaction. (C) 2018 Chinese Society of Aeronautics and Astronautics. Production and hosting by Elsevier Ltd.
引用
收藏
页码:1870 / 1879
页数:10
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