星载ScanSAR天线指向稳定度对辐射校正的影响

基于均匀加权天线模型,推导星载ScanSAR天线指向不稳定引起的多普勒中心频率估计误差,建立多普勒中心频率估计误差与图像辐射校正精度之间的数学模型,进而提出星载ScanSAR辐射校正对天线指向稳定度的要求。最后,通过计算机仿真,验证了理论分析的正确性。     

Integral inversion of GRAIL inter-satellite gravitational accelerations for regional recovery of the lunar gravitational field

We present an integral-based approach for high-resolution regional recovery of the gravitational field in this article. We derive rigorous remove-compute-restore integral estimators relating the line-of-sight gravitational acceleration to an arbitrary order radial derivative of the gravitational potential. The integral estimators are composed of three terms, i.e., the truncated integration, the low-frequency line-of-sight gravitational acceleration, and the high-frequency truncation error (effect of the distant zones). We test the accuracy of the integral transformations and of the integral estimators in a closed-loop simulation over the Montes Jura region on the nearside of the Moon. In this way, we determine optimal sizes of integration radii and grid discretisation. In addition, we investigate the performance of the regional integral inversion with synthetic and realistic GRAIL observations. We demonstrate that the regional inversion results of the disturbing gravitational potential and its first order radial derivative in the Montes Jura mountain range are less contaminated by high-frequency noise than the global spherical harmonic models.     

大气总温传感器误差修正方法研究

大气总温的准确测量对民用飞机的飞行安全至关重要。以古德里奇公司的102CP2AG总温传感器为例．详细论述了总温测量过程中对恢复系数、时间常数、自加热、防冰加热等误差的修正原理与使用方法。     

粒子拖尾长度对高频DPIV测量误差的影响

基于连续激光源的高采样频率DPIV系统在进行曝光时可能会产生粒子拖尾现象。明渠湍流试验和数值模拟试验结果显示，粒子拖尾长度的增加会导致平均流速减小和湍流强度增大。分析表明，导致平均流速误差的原因之一是诊断窗口边缘局部粒子图像的缺失，且图像缺失程度会随着粒子拖尾长度增加而增大，从而使平均速度随粒子拖尾长度增加而减小；粒子拖尾的另一个直接后果是增大了粒子图像的有效粒径，从而导致湍流强度增大。通过增大第二个诊断窗口的尺寸，进行相关函数标准化和相关系数补偿等方法，可以消除粒子拖尾长度引起的误差。     

基于最小二乘支持向量机的工具误差分离与折合

制导工具误差分离与折合是导弹精度评定中的重要问题,提出了利用支持向量机方法获得工具误差系数估计和进行弹道误差折合的新方法,由于支持向量机综合考虑了结构风险和经验风险,使得模型的泛化能力增强。仿真计算表明,与最小二乘和主成分方法相比,最小二乘支持向量机获得的误差系数估计与真值更加接近,折合得到的全程弹道遥外差更加准确。     

Central difference predictive filter for attitude determination with low precision sensors and model errors

Attitude determination is one of the key technologies for Attitude Determination and Control System (ADCS) of a satellite. However, serious model errors may exist which will affect the estimation accuracy of ACDS, especially for a small satellite with low precision sensors. In this paper, a central difference predictive filter (CDPF) is proposed for attitude determination of small satellites with model errors and low precision sensors. The new filter is proposed by introducing the Stirling’s polynomial interpolation formula to extend the traditional predictive filter (PF). It is shown that the proposed filter has higher accuracy for the estimation of system states than the traditional PF. It is known that the unscented Kalman filter (UKF) has also been used in the ADCS of small satellites with low precision sensors. In order to evaluate the performance of the proposed filter, the UKF is also employed to compare it with the CDPF. Numerical simulations show that the proposed CDPF is more effective and robust in dealing with model errors and low precision sensors compared with the UKF or traditional PF.     

Lightweight structure of a phase-change thermal controller based on lattice cells manufactured by SLM

Thermal controllers equipped with phase-change materials are widely used for maintaining the moderate temperatures of various electric devices used in spacecraft. Yet, the structures of amounts of thermal controllers add up to such a large value that restricts the employment of scientific devices due to the limit of rocket capacity. A lightweight structure of phase-change thermal controllers has been one of the main focuses of spacecraft design engineering. In this work, we design a lightweight phase-change thermal controller structure based on lattice cells. The structure is manufactured entirely with AlSi10 Mg by direct metal laser melting. The dimensions of the structure are 230 mm × 170 mm × 15 mm, and the mass is 190 g, which is 60% lighter than most traditional structures(500–600 g) with the same dimensions. The 3 D-printed structure can reduce the risk of leakage at soldering manufacture by a welding process. Whether the strength of the designed structure is sufficient is determined through mechanical analysis and experiments. Thermal test results show that the thermal capacity of the lattice-based thermal controller is increased by50% compared to that of traditional controllers with the same volume.     

大规模无参考译文质量自动评测技术的研究

传统的译文质量自动评测方法主要针对机器自动翻译结果并通过与参考译文的对比实现译文质量的评估。提出一种大规模无参考译文质量自动评测方法,该方法可以在无参考译文的情况下,从正确性、流畅性和忠实度等方面对人工译文进行质量检查并标注可能的错误点,即利用语言规则实现正确性的判断,利用语言模型实现流畅性的判断,利用词对齐结果和词典信息实现忠实度的判断。基于该方法实现的译文质量辅助检查系统在国家知识产权局百万专利翻译项目中的应用效果表明,使用该系统的测试组较未使用该系统的测试组的平均译文质量和终稿完成效率均有明显提升。     

静基座捷联惯性组合加速度计高阶误差项显著性分析

在标定捷联惯组加速度计时,一般采用多位置试验,但是目前并未对多位置试验所能标定出的误差系数数量和标定结果的有效性进行分析,本文针对这一问题展开了研究.首先,阐述了带有高次误差项的捷联惯组加速度计误差模型.然后,针对一般6位置标定方法无法完成这一模型标定的缺陷,提出了一种18位置标定方法.进行标定后,运用显著性分析方法,对误差模型本身和其中的参数的有效性进行了分析.最后,通过重复进行去除最不显著项、再标定、显著性检验等步骤,获得了试验室条件下所能标定的捷联惯组加速度计组合误差模型.     

基于广义相对论的轨道摄动下星间激光相位比对

针对纳米到皮米量级星间激光测距,在地心非旋转坐标系(GCRS)下,考虑卫星轨道摄动引起的广义相对论效应,建立了星间单向以及双向星间激光相位比对模型.通过仿真研究了地球主引力场范围内轨道摄动引起的广义相对论效应对星间激光相位比对误差的影响,并通过星间激光相位比对误差计算星间激光测距误差.不同轨道高度的卫星仿真结果表明,对...