直升机机动飞行仿真的气动建模及试验研究

 建立了适用于直升机机动飞行仿真的动力学模型。为了提高模型的真实度,着重通过瞬态操纵实验研究建立了旋翼非定常气动模型;又通过旋翼/ 机身气动干扰试验研究,并运用神经网络技术建立了一种新的机身气动力模型。使用该仿真模型做出的UH260A 直升机仿真计算结果与飞行试验数据符合良好。     

考虑冷气喷射的涡轮叶栅尾缘损失理论分析

 基于Denton 的尾缘流动理论, 发展了一种考虑冷气喷射的二维、可压涡轮叶栅尾缘混合损失模型,研究了涡轮叶栅尾缘损失的特征, 定量评估了影响尾缘损失的各种参数。研究表明, 冷气流量是影响尾缘损失的一个重要参数, 对于主流马赫数为11 1 的典型情况, 冷气流量从0 增大到10%, 损失增大315 倍。叶片尾缘基压变化对损失也具有明显的影响, 其它影响损失的参数包括叶栅出口位置边界层动量厚度、冷气总压、叶栅尾缘厚度等。     

新一代歼击机超机动飞行的动态逆控制

 根据反馈线性化理论, 讨论了神经网络自适应非线性动态逆控制设计。首先根据时标分离原则, 采用动态逆方法设计快回路和慢回路控制器; 其次提出基于模型逆的神经网络非线性直接自适应控制方案, 设计一种在线神经网络用于补偿模型逆误差。仿真表明, 该控制方案具有较好的自适应能力和鲁棒性。     

Modelling of the electromagnetic field in the interplanetary space and in the Earth's magnetosphere

A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented. In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the observational data for September 24–26, 1998 magnetic storm (Dst _min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997. This revised version was published online in August 2006 with corrections to the Cover Date.     

Phase coherence of foreshock MHD waves: wavelet analysis

The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies lower than the ion gyrofrequency are responsible for generating the phase coherence. This revised version was published online in August 2006 with corrections to the Cover Date.     

AR模型在时间序列误差分析中的应用

为检测某火控系统的性能,采用统计量分析和AR模型预测相结合来对火控系统实时解算的数据进行分析的一种方法。根据分析结果可以看出,距离误差和航向误差是两种不同类型的误差,距离误差主要是由随机的量测误差构成的,而航向误差主要是系统误差。     

三维四向编织复合材料基本性能的有限元模拟

依据三维四向编织复合材料的结构特点,建立了能真实反映其空间构型的"双纽线"单元体胞模型,并以此为基础,采用有限元方法对C／SiC三维四向编织复合材料的基本性能参数进行了数值模拟,获得了该材料在制备冷却阶段的热变形行为以及残余应力和残余应变的分布状况,同时获得了制备后室温条件下该材料的等效弹性模量与等效热膨胀系数值。     

带矢量喷管的涡扇发动机动态过程研究

建立带矢量喷管的涡扇发动机动态数学模型。研究了矢量喷管偏转角和偏转角速度对涡扇发动机工作的影响。研究结果表明 ,不同的矢量喷管偏转角速度对发动机涡轮前燃气温度会产生不同温度峰值 ,而且温度峰值随矢量偏转角速度增大而增大。而在一定的不同矢量角作用下 ,发动机的阶跃响应过程调节参数无明显变化      

液体火箭发动机试验台贮箱增压系统模块化仿真

采用一维理想气体流动的有限元状态变量模型,运用模块化建模与仿真方法和Fortran90语言进行了某液体火箭发动机试验台贮箱增压系统工作过程的仿真,获得了细致的管网状态参数分布曲线,为分析贮箱增压系统的工作过程及各组件的作用提供了数值依据。数学模型和模块化建模与仿真方法显示出较好的有效性和通用性。      

应用于强化传热的相变材料微胶囊的制备及特性

相变材料微胶囊(MEPCM)悬浮液是一种高热容冷却介质,其应用可大幅提高高功率设备液体冷却性能。本文对相变材料微胶囊的制备及其热特性进行了研究,研制了以蜜胺树脂为壁材、22烷为芯材、粒径10微米、不同芯材含量且适合于电子设备液体冷却的双层壁MEPCM。通过光学显微镜以及扫描电镜(SEM)观察到包覆完好的圆球状MEPCM。研究了制备过程中影响粒径以及包覆特性的因素。最后的DSC热分析表明了MEPCM具有很高的蓄热能力。