计算气动光学研究进展

计算气动光学是采用数值计算的方法研究高速空气动力流场对光波传输和光学成像影响的一门交叉学科,在红外成像制导设计等工程应用中发挥着重要的作用。总结了计算气动光学研究的三种基本计算方法,包括基于CFD简化方法的光学统计估算、基于RANS流场的计算和基于LES/DNS瞬态流场的计算,对这三种计算方法的基本理论、计算过程进行了介绍,综述了新近的一些计算气动光学研究进展,最后指出了未来的研究重点和方向。     

Geomagnetic activity driven by solar wind turbulence

Within the framework of the solar wind—magnetosphere coupled system, intense perturbations in the solar wind, causing geomagnetic storms and substorms, have been widely studied by means of the so-called coupling parameters. However, remarkable variations in the geomagnetic field occur even in absence of such perturbations. In those conditions, solar wind MHD turbulence might have a role. Recent results have shown that solar wind turbulence can be described not only as a mixture of inward and outward stochastic Alfvénic fluctuations, but includes also advected structures, dominated by an excess of magnetic energy.     

几种常用格式和湍流模型在高速流动中的适用性研究

针对高超声速飞行器中存在的强激波、激波/边界层干扰、分离、湍流等复杂流动现象,对比分析了当前计算流体力学中的主要空间离散格式及湍流模型,发现不同格式对强激波的分辨率基本相同,Roe和LDE(low diffusion E-CUSP(convective upwind split pressure))格式对摩擦因数和传热系数的模拟优于其他格式;S-A(Spalart-Allmaras)一方程湍流模型计算的摩擦因数比k-ωSST(shear stress transport)两方程湍流模型高10%左右,而后者预测的分离区约为前者的2倍,且分离点靠前.     

Solar wind turbulence during the solar cycle deduced from Galileo coronal radio-sounding experiments

Seven coronal radio-sounding campaigns were carried out during the active lifetime of the Galileo spacecraft in the years 1994–2002. The observational data analyzed in the present work are S-band frequency fluctuation measurements recorded during the solar conjunctions at different phases of solar activity cycle #23, specifically: periods near solar maximum (three conjunctions), near solar minimum (three conjunctions) and during the ascending phase (one conjunction). These data are all applicable to low heliographic latitudes, i.e. to the slow solar wind. The rms frequency fluctuation and power-law index of the frequency fluctuation temporal spectra are determined as a function of heliocentric distance. The turbulence power spectrum tends to be flatter inside ca. 20 solar radii during all phases of the solar cycle. This coincides with a transition in the flow from the inner acceleration region to the outer region of constant velocity. The radial falloff rate and absolute level of the rms frequency fluctuation are essentially invariant over the solar cycle.     

导弹撞地概率对参数选择的影响

研究了巡航导弹的撞地概率和系统参数选择的关系问题。首先在考虑了地形随机输入和低空风随机干扰共同作用的情况下，推导了撞地概率的计算方法。其次以导弹主要参数（ａ２４和Ｋｈ）的选择为例，在给定条件下求出了它们和撞地概率的关系曲线，并分析了它们对撞地概率的影响。研究结果表明，协调选择ａ２４和Ｋｈ等参数，能有效降低撞地概率，提高巡航导弹的作战效能。     

关于热量与质量传递的湍流模式问题

本文发展了一个新的热量与质量传递的标量—压力相关模式。讨论了局部平衡湍流的标量脉动与速度脉动相关。同时将所得理论结果和自由射流中关于温度脉动的测量数据进行了比较。     

THE PREDICTIONS OF CONVECTIVE HEAT TRANSFER ON TURBINE BLADE AIRFOIL BY USING LOW－REYNOLDS NUMBER TURBULENCE MODEL

ＴＨＥＰＲＥＤＩＣＴＩＯＮＳＯＦＣＯＮＶＥＣＴＩＶＥＨＥＡＴＴＲＡＮＳＦＥＲＯＮＴＵＲＢＩＮＥＢＬＡＤＥＡＩＲＦＯＩＬＢＹＵＳＩＮＧＬＯＷ－ＲＥＹＮＯＬＤＳＮＵＭＢＥＲＴＵＲＢＵＬＥＮＣＥＭＯＤＥＬＴＨＥＰＲＥＤＩＣＴＩＯＮＳＯＦＣＯＮＶＥＣＴＩＶＥ...     

JJ—7飞机对大气紊流的横航向响应及乘座品质计算

本文对JJ-7飞机的横航向晴空大气紊流响应及乘座品质进行了计算.计算结果表明,JJ-7飞机的横航向大气紊流响应值不大,乘座品质基本上满足要求,可以为飞行员接受.     

基于LADRC的无人机高精度定高控制

针对复杂气流扰动对无人机（UAV）航迹高度控制的影响,对存在复杂气流扰动下的定高控制策略、控制结构和控制器参数优化展开研究,实现高精度高度控制。基于线性自抗扰控制（LADRC）确定总体控制架构,设计扩张状态观测器（ESO）观测估计纵向高度通道和速度通道中存在的总扰动,在控制中引入扰动补偿,减小扰动对系统输出造成的影响。对UAV在飞行过程中存在的大气紊流扰动或离散突风等风干扰分析其功率谱密度,构造考虑风扰动对高度影响、时域响应特性和稳定裕度的综合目标函数,通过粒子群优化算法得到具有高精度、高抗干扰性能的控制器参数,优化中考虑风干扰的功率谱密度分布,减小了控制器参数设计的保守性。通过与常规比例-积分-微分（PID）控制器控制效果进行对比,说明基于线性自抗扰控制器的纵向高度控制的优异性能。