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Numerical analysis of flow field over compound delta wing at subsonic and supersonic speeds

机译:亚音速和超音速复合三角翼上流场的数值分析

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A great number of supersonic aircrafts use delta wings. Since 1950, delta wings have been studied well and it has been observed that there appear two large counter-rotating leading edge vortices when delta wing structure flies at high angles of attack. These vortices are responsible for additional lift and they also provide a very high stall incidence to the wing. At high Mach numbers, compressibility advances leading edge separation and also expands the magnitude of the primary vortex. Shock waves appearing due to high-speed flow over the delta wing result in drastic changes in the flow characteristics. Although supersonic jets use delta wing configurations but most of the time they fly at subsonic speeds and hence the focus of present study is on both subsonic as well as supersonic regimes. The present study consist of numerical simulations of the flow-field over a compound delta wing at various Mach numbers ranging from 0.3 to 2.0 and angles of attack ranging from 0¿¿ to 15¿¿ using the computational model established in previous research [1]. Reynolds Averaged Navier-Stokes (RANS) based steady-state computations were carried out. Spalart Allmaras (SA) turbulence model is considered due to its less computational cost and good performance for simulating external flows. Since the study involves supersonic Mach numbers, compressibility was also incorporated in the computational model. The study with various freestream Mach numbers shows that there is a sudden change in flow fields with an increase in the Mach number for the range of 0.8 to 1.3. The flow near to the delta wing surface beneath the primary vortex becomes completely supersonic and shock waves appear when the flow reaches Mach number 0.85. Due to this shock wave formation, flow fields become more complex. At high Mach number because of the stronger magnitude of the primary vortex which prevents the evolution of the inner separation, the secondary vortex disappears. The results also confirm the hypothesis o- vortex breakdown which is also responsible for the nonlinear behavior of flow characteristics over the wing when there is an increase in Mach number.
机译:许多超音速飞机使用三角翼。自1950年以来,对三角翼的研究已得到很好的研究,并且观察到,当三角翼结构以高攻角飞行时,会出现两个较大的反向旋转的前缘涡旋。这些涡旋导致额外的升力,它们还为机翼提供了很高的失速发生率。在高马赫数下,可压缩性促进了前沿分离,并且还扩大了初级涡旋的幅度。由于三角翼上方的高速流动而产生的冲击波导致流动特性发生急剧变化。尽管超音速喷气机使用的是三角翼构型,但大多数时候它们以亚音速飞行,因此,本研究的重点是亚音速和超音速状态。本研究包括使用先前研究中建立的计算模型对复合三角翼在0.3至2.0的各种马赫数和0到15的迎角范围内的流场进行数值模拟[1]。 。进行了基于雷诺平均纳维-斯托克斯(RANS)的稳态计算。之所以考虑使用Spalart Allmaras(SA)湍流模型,是因为其计算成本较低,并且具有良好的模拟外部流的性能。由于研究涉及超音速马赫数,因此可压缩性也纳入了计算模型。对各种自由流马赫数的研究表明,在0.8至1.3的范围内,随着马赫数的增加,流场会发生突然变化。在主旋涡下方的三角翼表面附近的流动变得完全超音速,当流动达到马赫数0.85时会出现冲击波。由于这种冲击波的形成,流场变得更加复杂。在高马赫数下,由于初级涡旋强度更高,阻止了内部分离的发展,因此次级涡旋消失了。结果还证实了假设涡旋破坏,这也是当马赫数增加时机翼上流动特性的非线性行为的原因。

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