高超声速化学非平衡粘性激波层方程的数值解

本文讨论了高超声速粘性激波层方程数值计算时差分格式引起的物理失真问题。具体分析了全隐格式格式粘性的影响,并作了数值试验。为了验证隐式结果的可靠性。在超声速激波风洞中测量了钝锥的表面压力分布,并与计算结果作了比较,两者基本一致。 本文采用隐式有限差分法数值计算了高超声速化学非平衡粘性激波层绕细长球锥的流动。计算时采用连续方程和法向动量方程耦合求解的方法以解决细长体远后身区计算中的问题。应用网格技术和加强系数矩阵主对角元素优势的方法提高了化学非平衡流计算的雷诺数范围。文中给出了高超声速化学非平衡流的计算结果,并与其它文献的结果作了比较。     

球心非对称的钝圆头体近区绕流场气动特性分析研究

本文采用数值模拟对球心非对称的钝圆头体附近流场气动特性进行分析研究。数值求解三维可压缩NS方程，采用NND格式，以修正的Baldwin-Lomax代数模型对不同飞行状态进行数值模拟，分析了球心非对称钝圆头体对流场的影响，与部分试验比较结果满意。     

Multiple-constraint cooperative guidance based on two-stage sequential convex programming

An improved approach is presented in this paper to implement highly constrained cooperative guidance to attack a stationary target. The problem with time-varying Proportional Navigation (PN) gain is first formulated as a nonlinear optimal control problem, which is difficult to solve due to the existence of nonlinear kinematics and nonconvex constraints. After convexification treatments and discretization, the solution to the original problem can be approximately obtained by solving a sequence of Second-Order Cone Programming (SOCP) problems, which can be readily solved by state-of-the-art Interior-Point Methods (IPMs). To mitigate the sensibility of the algorithm on the user-provided initial profile, a Two-Stage Sequential Convex Programming (TSSCP) method is presented in detail. Furthermore, numerical simulations under different mission scenarios are conducted to show the superiority of the proposed method in solving the cooperative guidance problem. The research indicated that the TSSCP method is more tractable and reliable than the traditional methods and has great potential for real-time processing and on-board implementation.     

木材在锥形量热仪上的点燃实验研究

利用锥形量热仪研究了外加辐射热流和电火花点火高度对木材着火时的点燃时间、表面温度、质量损失速率等点燃特征参数的影响,提出了室内火灾中木材点燃的临界质量通量判据。研究结果表明,增大外加辐射热流,木材点燃时间缩短,点燃的临界表面温度减小,但临界质量通量不变;增大电火花的点火高度,木材点燃时间延长,点燃的临界表面温度升高,临界质量通量增大;对于特定场所,可以用临界质量通量作为木材点燃的判据。     

共轴式双旋翼直升机锥体测量技术研究

根据目前国内共轴式双旋翼直升机的维护需求,简要介绍了该类直升机旋翼锥体的测量方法.针对现有测量方法存在的缺点和不足,提出了一种采用新型的采用光学传感器测量该类直升机旋翼锥体的技术和方法,通过外场的实际应用,收到了良好效果,验证了其有效性.     

月壤剖面锥型螺旋刃成孔钻头设计

针对月壤剖面钻进成孔探测需求,提出一种锥型螺旋刃成孔钻头,建立其钻进排屑性能的理论模型,并以此开展钻头结构参数的优化设计。在此基础上,分析螺旋刃切削姿态及其切削参数,基于直线刃平面切削理论建立锥型螺旋刃成孔钻头钻进切削负载预估模型,开展锥型螺旋刃成孔钻头模拟月壤剖面钻进负载特性试验验证。研究结果表明,相比于直线刃钻头,锥型螺旋刃成孔钻头的钻进排屑性能更优,而且钻进切削负载模型与试验结果具有较好的吻合度。研究成果对我国拟实施的月面钻取采样工程具有重要的借鉴价值。     

某燃气轮机空气雾化喷嘴的试验研究

进行了某型燃机空气雾化喷嘴燃油喷雾特性的试验研究。得到以下结论：在油压不变的情况下,雾化锥角总是随着空气压力的增加有所减小,索特尔平均直径SMD随之迅速减小,整体减小幅度大约在10-30μm;气压不变时,雾化锥角和索特尔平均直径随着油压的增加而稍有增大;当气压为0.3MPa时,索特尔平均直径基本都保持在30μm以内。     

扩张半角对无喷管助推器性能的影响分析(英文)

用数值分析的方法研究了扩张半角对固冲发动机无喷管助推器性能的影响规律.研究结果表明,随着扩张半角的增大,比冲先增加后减小,扩张半角取22°可使比冲达到近优:这一结论与有关文献的实验结果基本一致;从流动损失方面考虑,在无喷管助推器设计中,药柱出口端面与冲压喷管之间不应出现台阶,应使扩张段连续地过渡到冲压喷管上.本文结论可为无喷管助推器的设计改进提供参考.     

高超声速钝球柱外形表面热流分布研究

文章采用数值求解雷诺平均Navier-Stokes方程方法对高超声速钝球柱地面试验模型进行了计算,比较了不同头部半径和肩部半径条件下表面热流的分布特征。研究表明：钝球柱头部区域表面热流分布与头部半径和肩部半径紧密相关。其中,头部半径对热流分布特征和热流大小均存在显著影响。当头部半径较小时,头部区域热流呈现双峰值分布,热流由驻点峰值逐渐下降,接近肩部时开始上升,至肩部峰值点后又继续下降。随着头部半径的增大,驻点热流减小,肩部热流增加,双峰值分布逐渐演变为单峰值分布,热流由驻点单调上升至肩部峰值点;相对于头部半径,肩部半径主要影响热流大小,驻点热流和肩部热流均随肩部半径的增大而增加,不同肩部半径计算模型的头部热流分布规律基本一致。     

Study of VLF wave with relativistic effect in Saturn magnetosphere in the presence of parallel A.C. electric field

Cassini radio and plasma wave surveys aim to study radio emissions, plasma waves, thermal plasma and dust near Saturn. Using the characteristic solution and dynamics method, the influence of electron beam on the loss cone and bi-Maxwellian distribution of whistler mode waves in the parallel alternating electric field and magnetic field is studied. The dispersion relation and the growth rate of Saturn's magnetic layer were deduced and calculated in detail. Parameter analysis is performed by changing the parameters of the plasma like number density, AC frequency, temperature anisotropy, etc. The influence of AC frequency on Doppler shift and the comparative study of growth rate of oblique and parallel propagating waves are analyzed using generalized distribution function. We found temperature anisotropy ${\text{A}}_{\text{T}}=1.25$ can explain the linear spatiotemporal growth rate of whistler mode waves. It provides the majority of the observed frequency integral power. It can be seen that the effective parameters for the generation of Whistler mode waves are not only temperature anisotropy, but also the relativistic factors discussed in the results and discussion section, and the AC field frequency and width of the loss cone distribution function.