液压能源管路系统振动主动控制的理论研究

对飞机液压能源管路系统的振动问题进行了探讨.提出一种基于振动主动控制(VAC)技术对飞机液压能源管路系统进行消振的方法,在手段上采用压电/压电致伸技术,以压电陶瓷(PZT)作为作动器,具有驱动力大、响应频率高和体积小等优点;控制方法上采用参数寻优的控制策略,它能始终能根据外界干扰因素的变化来调整控制参数.经过理论分析和仿真验证,证明其具有良好的自适应性和鲁棒性,在变转速和变负载情况下始终能保持最佳的消振效果.     

用电离层特性参量提取等效风场信息

导出了利用中低纬电离层特性参量获取电离层F层峰区高度上等效风场（包含电场和风场信息在内）的基本方程，并尝试用该方法从电离层特性参量（峰高和临频）提取等效风场信息，利用武汉站DGS-256电离层数字测高仪数据及由美国Massachusetts Lowell大学最新版的剖面反演程序换算得到F层峰高，获得了武汉地区夏季至日点附近，冬季至日点附近，冬季地磁特别宁静的九天和冬季平均等效风场的初步特征，并利用Fejer经验电场模式计算冬季电场引起的垂直漂移，估计电场和风场对武汉地区的垂直等效风场的贡献大小，结果表明：等效风场呈现出白天与夜晚幅度和方向的差异。至日点附近冬季与夏季白天的幅度差异以及明显的凌晨凹陷现象；平均情况下，垂直等效风场幅度和方向的变化主要是由中性风引起，受电场的影响不大。     

雷暴云准静电场和夜间低电离层的电离

用点电荷模型计算雷暴云突然放电后形成的准静电后形成的准静电场随高度的分布，以E/N（E的电场大小，N为大气密度）为输入参量，在一定条件下，对Boltzmann方程数值求解，计算电离层电子数密度的扰动。计算结果表明，在约70-90km之间，在约放电后的10ms内，准静电场大于中性大气的击穿电场，将引起大气的雪崩电离，从而引起夜间低电离层电子密度的显著增加，但这种电子密度的增加是暂的，在很短的时期内就恢复到平静时的水平，恢复时间随高度的变化而不同。     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.     

一般硬化材料弹塑性旋转盘的变分解法

首先在小弹塑性范围内用应变的奇次四项式相当精确地拟合一般硬化材料的拉伸曲线;再在体积不变条件下用弹性位移场的已知模态和一待定幅值构成弹塑性位移场;最后用势能原理确定该幅值而得到封闭解。     

半浮区液桥自由面振荡特征

使用一套双路同步显微放大录像及图像处理系统,研究了夹角为90°的两个竖直剖面沿轴向不同高度液桥自由表面的位移振荡,得到轴向不同高度上的环向相位差,观测到在振荡周期内液桥表面轮廓线在不同时刻均不相交的特点。实验结果表明,液桥自由面振荡除具有径向扰动及轴向振荡变化外,还存在环向波动变化。根据实验结果,讨论了环向波动基本变化规律以及本实验在测量精度和测量误差方面存在的问题。     

研究用现场数据估计系统可靠性参数置信区间

研究用元部件现场信息估计系统可靠性参数,如系统可靠度、可靠寿命等区间估计问题。文中提出了一种新的估计方法——替换百分点法,并运用Monte Carlo数字仿真对估计的置信度和精度进行了分析,研究结果表明此方法具有工程应用价值。     

多机并联火箭羽流流场及其底部热环境分析

For the problem that the plume flow field structure of a multi engine parallel rocket is complicated and the bottom thermal environment is extremely harsh, which may cause the failure of the engine structural components, the plume flow field and thermal environment at different altitudes are studied through numerical simulation. The result is compared with the measured results in flight which shows that when the rocket is flying at a low altitude, the plume of the engines do not interfere with each other. As the flight altitude increases, the plumes gradually expand and begin to interfere with each other, and finally there is an obvious backflow at the bottom of the rocket. The maximum heat flux at the moment of take off is basically the same as the measured value in flight. Before the backflow occurs, the heat flux mainly consists of radiant heat, the convective heat flow increases as the flight altitude grows, but it is also much smaller than the peak heat flow at takeoff. The result has certain guiding significance for the optimal design of engine structure thermal protection.     

基于微型涡喷发动机热喷流的无源流体推力矢量喷管的控制规律

流体推力矢量喷管型面固定、活动部件少、结构重量轻，能够为高机动飞行器提供有效的飞行控制手段，但无源流体推力矢量喷管热喷流的偏转控制规律尚未完全掌握。为了推进无源流体推力矢量技术的实用化，本文设计研制了适用于微型涡喷发动机的耐高温喷管模型，对该喷管在微型涡喷发动机热喷流状态下的控制规律进行研究。利用非接触光学显示和测量手段——红外热成像拍摄和粒子图像测速（PIV）技术对主射流流动特性进行研究，获得流动矢量角随二次流控制阀门闭合度变化的控制规律；利用六分量盒式天平测力实验研究无源流体推力矢量喷管的力学特性，获得推力矢量角随二次流控制阀门闭合度变化的控制规律。研究结果表明：该构型喷管在微型涡喷发动机热喷流下主射流连续可控偏转，最大流动矢量角为-12.3°/12.3°，最大推力矢量角为-12.9°/12.8°，控制规律接近线性，不存在主射流偏转突跳问题。     

Geometric calibration of Colour and Stereo Surface Imaging System of ESA’s Trace Gas Orbiter

There are many geometric calibration methods for “standard” cameras. These methods, however, cannot be used for the calibration of telescopes with large focal lengths and complex off-axis optics. Moreover, specialized calibration methods for the telescopes are scarce in literature. We describe the calibration method that we developed for the Colour and Stereo Surface Imaging System (CaSSIS) telescope, on board of the ExoMars Trace Gas Orbiter (TGO). Although our method is described in the context of CaSSIS, with camera-specific experiments, it is general and can be applied to other telescopes. We further encourage re-use of the proposed method by making our calibration code and data available on-line.