基于级联耦合的大功率测量技术研究

讨论了采用级联耦合测量技术的大功率测量系统,指出大功率测量条件下引起测量不确定度的因素,搭建了基于该技术的大功率校准系统,减小了系统测量不确定度,实现了功率放大器的高精度校准和测量。     

A tip clearance prediction model for multistage rotors and stators in aero-engines

Tip clearances of multistage rotors and stators greatly affect aero-engines’ aerodynamic efficiency, stability and safety. The inevitable machining and assembly errors, as well as the complicated error propagation mechanism, cause overproof or non-uniform tip clearances. However, it is generally accepted that tip clearances are difficult to predict, even under assembly state. In this paper, a tip clearance prediction model is proposed based on measured error data. Some 3D error propagation sub-models, regarding rotors, supports and casings, are built and combined. The complex error coupling relationship is uncovered using mathematical methods. Rotor and stator tip clearances are predicted and analyzed in different phase angles. The maximum, minimum and average tip clearances can be calculated. The proposed model is implemented by a computer program, and a case study illustrates its performance and verifies its feasibility. The results can be referred by engineers in assembly quality judgement and decision-making.     

一种星间设备系统偏差的标定方法

针对Ka波段测距体制中星间测距设备系统偏差标定困难从而影响自主导航精度的问题,提出用星地无线电双向时间比对的方法标定星间设备系统偏差。通过两条星地双向链路并在这两颗卫星间建立一条星间双向链路进行标定。结果表明：该方法能够标定星间设备系统偏差,其RMS优于1ns,从而起到提高星间时间同步精度的目的。     

主流压力梯度对气膜孔流量系数影响机理

测量了主流零压力梯度、正压力梯度及负压力梯度条件下气膜孔流量系数,分析了主流压力梯度对气膜孔流量系数的影响机理.结果显示:正、负压力梯度的存在对气膜孔流量系数的影响幅度最大值分别为22%及26%.主流压力梯度会对喷出气流施加弯转作用及挤压作用,同时也会改变喷出气流与近壁面主流的掺混作用,从而影响气膜孔流量系数.挤压作用使喷出气流管变细而增加喷出气流的流动损失;弯转作用主要影响喷出气流的流动轨迹,正压力梯度下弯转作用使喷出气流的轨迹靠近壁面而远离其自由喷射方向增加流动损失,负压力梯度的作用则相反;掺混作用会增加喷出气流的动量消耗,正压力梯度对掺混有抑制作用,从而减少喷出气流用于掺混的动量损失,负压力梯度则相反.      

一种改进的多点融合非均匀校正技术

针对空间宽幅相机在进行非均匀性校正过程中相机镜头与积分球输出口的相对位置发生变换后非均匀性校正精度下降的原因进行了分析,提出了一种改进的融合多点位置的非均匀校正新方法,即为了消除积分球的角均匀性和面均匀性的不足,采用获取多个位置的大量定标图像,融合求取平均值的方法得到校正系数来削弱这种影响,并进行试验验证分析。结果表明,多点融合的校正方法在积分球输出口光强不均匀、又无法固定相机与积分球相对位置的前提下,减少了积分球光强的不均匀性对系数可靠性的影响,相对辐射定标的非均匀校正精度得到大幅提高。     

铷频标物理系统的改进研究

物理系统是铷频标的核心部件,通过分析影响频率稳定度的因素,对物理系统内部结构进行了改进。改进后的物理系统采用分离滤光的三泡结构,增加了光学滤光技术,此外,物理系统还选用了磁控管微波腔。经测试,改进后的铷频标温度系数为9.7×10^-14/℃,频率稳定度约为1×10^-12/τ（1s≤τ≤10 000s）。     

中心进气转静系转盘风阻扭矩数值模拟

采用计算流体力学(CFD)商业软件CFX从流动参数及几何结构两个方面对中心进气转静系盘腔内转盘风阻扭矩特性进行了数值模拟研究,同时搭建一个转盘风阻扭矩实验台测量自由盘风阻扭矩.中心进气转静系转盘风阻扭矩与经典经验公式进行了对比,结果表明:利用数值模拟方法,得到的无量纲扭矩系数与经典经验关系式计算得到的数据总体相差小于10%,利用湍流参数来表征转盘转速以及叠加流流量,对于分析转盘风阻扭矩非常便利.利用湍流参数定量分析时需注意叠加流以及转速的量级同样影响着风阻扭矩的数值.几何结构对于风阻扭矩也有影响,但相比流动参数影响较小.      

星载SAR轨道及姿态误差模型分析

平台轨道及姿态误差模型是星载SAR数据模拟及相应的模拟系统的关键组成部分。简要分析了机载SAR和星载SAR的差异,重点对星载SAR的平台轨道及姿态模型进行了分析,最后对星载SAR回波信号仿真方法进行了分析。     

Periodic Variations of Drag Coefficient for the ANDE Spherical Satellites During its Lifetime

A drag coefficient (C_D) inversion method is introduced to study the variations of the drag coefficient for orbital satellites with spherical geometry. Drag coefficients of the four micro satellites in the Atmospheric Neutral Density Experiment (ANDE) are compiled out with this new method. The Lomb-Scargle Periodgram (LSP) analysis of the four ANDE satellites' C_D series has shown that there are obvious 5, 7, 9, and 27 days' period in those data. Interesting results are found through comparing the LSP analysis with series of the daily solar radio flux at 10.7 cm (F_10.7 index), the Ap index, and the daily averaged solar wind speed at 1AU. All series in the same time interval have an obvious period of about 27 days, which has already been explained as the association with the 27 days' solar rotation. The oscillating periods less than 27 days are found in series of C_D, Ap and solar wind speed at 1AU, e.g., the 5, 7, 9 days period. However, these short periods disappeared in the time series of F_10.7 index. The same periodicities of 5, 7, 9 days in Ap and solar wind are presented at the same time interval during the declining phase of solar cycle 23. While in the ascending phase of solar cycle 24, these short oscillations are not so obvious as that in the declining phase of solar cycle 23. These results provide definite evidence that the C_D variations with period of 5, 7 and 9 days are produced by a combination of space weather effects caused by the solar wind and geomagnetic activity.      

锥运动条件下新的速度误差补偿项研究

经典的捷联惯导积分算法往往需要在姿态更新过程中对圆锥误差项进行精确补偿。虽然考虑了载体姿态变化的影响,但速度更新算法通常忽略了圆锥效应的作用。就圆锥误差项引起的速度误差进行了研究。指出其与陀螺角增量对速度更新的影响方式相同。在假设的线性斜坡模型条件下,利用两个连续的角增量和比力增量,详细推导了新的速度误差项的二子样更新补偿算法。在一种特殊的机动条件下,即当载体绕横轴作圆锥角振动的同时又沿立轴作同频同相的线振动,推导的二子样优化算法能够使该误差补偿项的平均性能最优。仿真结果证明该优化算法能够对新的速度误差积分项进行有效的补偿。