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超低轨与临近空间高速流中迎风微凹腔对尖前缘气动特性的影响

EFFECTS OF A WINDWARD MICRO-CAVITY ON THE AERODYNAMIC CHARACTERISTICS OF A SHARP LEADING EDGE IN HYPERSONIC FLOWS FROM NEAR SPACE TO ULTRA-LOW EARTH ORBIT

  • 摘要: 临近空间与超低轨道高超声速飞行中尖前缘构型应用广泛, 但受原子氧侵蚀与制造装配误差等因素影响, 前缘表面难以长期保持光滑, 易产生微凹腔与缝隙等缺陷, 从而改变近壁流动与壁面气动载荷分布. 本文采用直接模拟蒙特卡洛(DSMC)方法研究二维楔形尖前缘迎风微凹腔对气动特性的作用机理. 选取 70、110与150 km 三种高度工况, 在微凹腔深度0.05 ~ 2 mm范围内开展参数化计算, 获得腔内温度场、速度场与压力场响应, 提取微凹腔表面热流系数、压力系数与剪切力系数的周向分布, 并统计底面入射粒子速度分布以表征入射状态变化. 结果表明: 70 km工况下, 微凹腔对弓形激波形态及脱体位置影响有限, 但可诱导闭合回流与低温滞留, 显著削弱底面气动加热, 且底面热流系数随深度增大持续降低. 高度升至110与150 km后, 稀薄效应增强导致整体温度与压力水平下降, 微凹腔对周向热流的调制显著减弱; 同时, 腔内回流增强并出现侧壁低压带, 深凹腔使前缘近场速度扰动更为显著. 粒子统计显示, 高稀薄度条件下凹腔底面入射速度分布由单峰演化为自由来流高速峰与腔内低速峰并存的双峰结构, 且低速峰占比随微凹腔加深而提高. 上述结果可为稀薄效应下尖前缘微结构的气动特性评估与设计提供参考, 并为气固界面相互作用模型的入射条件表征提供依据.

     

    Abstract: Sharp leading edges are widely used in near-space and ultra-low-Earth-orbit hypersonic flight, but unavoidable surface imperfections can produce small windward cavities and gaps that locally distort the near-wall flow and alter the resulting aerodynamic loads. This work employs the Direct Simulation Monte Carlo (DSMC) method to examine how a windward micro-cavity on the sharp leading edge of a two-dimensional wedge alters aerodynamic heating and force loads. Simulations are performed at three altitudes (70, 110, and 150 km) with the cavity depth varied from 0.05 to 2 mm. The cavity-resolved temperature, velocity, and pressure fields are obtained. Distributions of the surface heat-flux, pressure, and shear-stress coefficients along the cavity-perimeter coordinate are evaluated, and incident velocity statistics of gas particles on the cavity bottom are used to characterize changes in the incidence state. At 70 km, the cavity has little effect on the bow-shock shape and stand-off distance, but it promotes a closed recirculation region with low-temperature gas retention, markedly reducing bottom heating; accordingly, the bottom heat-flux coefficient decreases monotonically with increasing cavity depth. At 110 and 150 km, stronger rarefaction lowers the overall temperature and pressure levels and weakens the sensitivity of circumferential heating to cavity depth. Meanwhile, the internal recirculation becomes more distinct and a low-pressure band develops along the sidewall, and deeper cavities induce more pronounced disturbances in the near-field velocity around the leading edge. Particle statistics further show that, in the highly rarefied regime, the streamwise incident-velocity distribution on the cavity bottom changes from a single-peak form to a bimodal form consisting of a freestream high-speed peak and a low-speed peak, with the low-speed contribution increasing as the cavity deepens. These results support aerodynamic assessment and design of sharp-leading-edge micro-features under rarefaction effects and provide incident conditions derived from particle statistics for gas–surface interaction modeling.

     

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