激光陀螺在中、远程防空导弹上的应用

分析了激光陀螺的工作原理，介绍了激光陀螺的性能特点，提出激光陀螺具有传统的机电陀螺和其他类型陀螺所无法比拟的优点，其性能特征完全满足捷联惯导对惯性测量元件的要求，军事应用前景十分广阔，同时，对激光陀螺在新一代防空导弹上的应用作了展望。     

闭环光纤陀螺的温度补偿

为使全数字闭环光纤陀螺在全温度(-40～+65℃)范围内的性能保持一致,采用了控制光源以稳定光功率和波长,以及对集成光器件进行温度补偿两种技术措施。试验结果表明,研制的光纤陀螺在全温度范围内,标度因数和零偏的温度灵敏度分别小于2×10-5℃-1、0.008(°)/(h·℃),达到了中等精度光纤陀螺的要求。     

单Y型集成光学芯片的性能和集成光学陀螺关键技术研究

详细阐述了工程化多功能集成光学单Ｙ芯片的物理特性及对集成光学陀螺性能的影响。在陀螺相位检测过程中着重分析单Ｙ器件的背反射量对陀螺输出信号畸变的影响，由此建立的数学模型能很好地说明实验结果。     

Unbiased acceleration measurements with an electrostatic accelerometer on a rotating platform

The Gravity Advanced Package is an instrument composed of an electrostatic accelerometer called MicroSTAR and a rotating platform called Bias Rejection System. It aims at measuring with no bias the non-gravitational acceleration of a spacecraft. It is envisioned to be embarked on an interplanetary spacecraft as a tool to test the laws of gravitation.     

光纤陀螺中分形噪声的参数估计和去除

光纤陀螺零漂信号中主要存在分形噪声和高斯白噪声,采用传统的时间序列分析法很难去除这类混合噪声.基于小波分析,提出一种分步估计加性白噪声强度和分形随机过程参数的新方法.先通过拟合自相关函数,估计出白噪声的强度;再在小波变换域估计分形噪声参数,并选取适当软阈值对测量值滤波.实验结果表明该估计和降噪方法有效地去除了光纤陀螺中的混合噪声,且不需要噪声的先验知识,具有很好的适应性.      

圆锥运动及其影响的3种描述方法

从旋转矢量方法、欧拉角方法及刚体有限转动方法出发对圆锥运动及其影响进行了阐述,得到了各方法下的等效陀螺漂移公式以及三者之间的关系;并对圆锥补偿算法在每种方法下的补偿效果进行了研究.结果表明: 刚体有限转动方法与旋转矢量方法是完全等价的,欧拉角方法仅在小角度振动情况下与它们等价;圆锥补偿算法在旋转矢量方法和欧拉角方法下均有效,并在振动角较小时补偿效果一致.旋转矢量方法和刚体有限转动方法重点在于圆锥补偿算法的开发,而欧拉角方法重点则在于指导圆锥运动转台实验设计以验证圆锥补偿算法.      

飞控系统性能与可靠性一体化设计技术

通过分析性能与可靠性一体化设计国内外相关研究工作的研究成果与不足,提出了性能与可靠性一体化设计(IDPaR,Integrating Design for Performance and Reliability)的研究思路.从产品发生故障的内、外因角度建立了性能与可靠性一体化设计综合模型,提出了性能可靠度的定义和计算方法.并针对典型飞控系统,给出了各类内外影响因素的具体建模方法,总结提出了性能与可靠性一体化设计算法流程和分析方法.最后以某型导弹为案例,进行性能与可靠性一体化设计技术的应用验证.      

全光纤陀螺信号处理技术研究

采用数字、模拟混合信号处理方法，模拟信号处理主要针对光源驱动、相位调制器(PZT)的控制、相位跟踪、探测器信号的滤波和解调进行，数字信号处理器(DsP)根据模拟解调信号进行Sagnac相移计算、相敏参考信号自动选择，以及大小量程分档控制。此方法可有效发挥模拟、数字信号处理的优点，提高光纤陀螺的总体性能。     

Free fall tests of the accelerometers of the MICROSCOPE mission

The MICROSCOPE mission is fully dedicated to the in-orbit test of the Universality of free fall, the so-called Weak Equivalence Principle (WEP), with an expected accuracy better than 10⁻¹⁵. The test principle consists in comparing the accelerations of two proof masses of different composition in the Earth gravitational field. The payload embarks two pairs of test-masses made of Platinum Rhodium and Titanium alloys at the core of two dedicated coaxial electrostatic accelerometers. These instruments are under qualification for a launch in 2016.     

Impact of a novel hybrid accelerometer on satellite gravimetry performance

The state-of-the-art electrostatic accelerometers (EA) used for the retrieval of non-gravitational forces acting on a satellite constitute a core component of every dedicated gravity field mission. However, due to their difficult-to-control thermal drift in the low observation frequencies, they are also one of the most limiting factors of the achievable performance of gravity recovery. Recently, a hybrid accelerometer consisting of a regular EA and a novel cold atom interferometer (CAI) that features a time-invariant observation stability and constantly recalibrates the EA has been developed in order to remedy this major drawback. In this paper we aim to assess the value of the hybrid accelerometer for gravity field retrieval in the context of GRACE-type and Bender-type missions by means of numerical closed-loop simulations where possible noise specifications of the novel instrument are considered and different components of the Earth’s gravity field signal are added subsequently. It is shown that the quality of the gravity field solutions is mainly dependent on the CAI’s measurement accuracy. While a low CAI performance (10^?8 to 10^?9?m/s²/Hz^1/2) does not lead to any gains compared to a stand-alone EA, a sufficiently high one (10^?11?m/s²/Hz^1/2) may improve the retrieval performance by over one order of magnitude. We also show that improvements which are limited to low-frequency observations may even propagate into high spherical harmonic degrees. Further, the accelerometer performance seems to play a less prominent role if the overall observation geometry is improved as it is the case for a Bender-type mission. The impact of the accelerometer measurements diminishes further when temporal variations of the gravity field are introduced, pointing out the need for proper de-aliasing techniques. An additional study reveals that the hybrid accelerometer is – contrary to a stand-alone EA – widely unaffected by scale factor instabilities.