纤维增韧陶瓷基复合材料的比例极限应力与残余热应力关系

从细观力学角度分析并建立了纤维增韧陶瓷基复合材料从制备温度冷却到室温过程中产生的残余热应力与复合材料的比例极限应力的关系模型。该模型表明,减少复合材料的残余热应力或提高复合材料的纤维与基体的模量比,均可提高复合材料的比例极限应力。通过单调拉伸实验测试了先驱体浸渍裂解法(PIP)制备的2D SiC/SiC复合材料的比例极限应力,并采用文中建立的比例极限应力与残余热应力关系模型,计算出复合材料SiC基体的残余热应力为-19.5 MPa。分析表明,该结果是合理的。此外,引用了公开文献报道的5种复合材料体系数据,用于验证文中所建立的比例极限应力与残余热应力关系模型的适应性和可靠性,计算结果与实验结果最大误差为18.6%,表明该模型具有较好的适应性和可靠性,可为纤维增韧陶瓷基复合材料的研究提供新思路。     

机载电源模块通用测试平台设计

针对机载电源模块种类繁多，功能各异，传统手工测试方法繁琐、复杂的缺点，设计了一种通用电源模块测试平台，它具有自动化程度高、可靠性强、使用及维护方便等特点，通过不同的适配器可以测试不同的电源模块，可扩展性强。给出了该平台的硬件组态、功能实现及相应软件设计流程，实际使用表明该测试平台具有极高可靠性和实用性，可以大幅度缩短电源模块的研制和生产周期。     

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.     

Spectroscopy peculiarities of thermal plasma of electric arc discharge between electrodes with Zn admixtures

Plasma of the free burning electric arc between Ag–SnO₂–ZnO composite electrodes as well as brass electrodes were investigated. The plasma temperature distributions were obtained by Boltzmann plot method involving Cu I, Ag I or Zn I spectral line emissions. The electron density distributions were obtained from the width and from absolute intensity of spectral lines. The laser absorption spectroscopy was used for measurement of copper atom concentration in plasma. Plasma equilibrium composition was calculated using two independent groups of experimental values (temperature and copper atom concentration, temperature and electron density). It was found that plasma of the free burning electric arc between brass electrodes is in local thermodynamical equilibrium. The experimental verification of the spectroscopic data of Zn I spectral lines was carried out.     

三角网格面自动铺丝定角度路径规划算法

研究三角网格曲面上的路径规划问题,以局部测地线为补充,提出了改进的定角度初始路径规划算法。该算法避免了传统参数化求解过程的无解和多解情况,尤其适用于曲率变化较大的复杂曲面和拼接曲面。采用等距覆盖算法来获得均匀的满铺路径,并分别提出基于路径样条线末端延伸和芯模曲面整体延拓的两种边界处理思路,以解决偏移路径无法到达曲面边界的问题。以某机翼模型为算例对上述算法进行验证,利用计算机辅助三维交互应用(Computer aided three-dimensional interactive application,CATIA)的逆向工程模块实现了完整的算法可视化,建立了三维建模软件与路径规划算法的系统关系。验证表明本文提出的算法可靠、系统、适应性强,具有工程应用价值。     

A concept mission for the Stellar Population and Evolution with Cubesats (SPEC)

Binary or multiple stellar systems, constituting almost a third of the content of the Milky Way, represent a high priority astronomical target due to their repercussions on the stellar dynamical and evolutionary parameters. Moreover the spectral study of such class of stars allows to better constrain the evolutionary theories of the Galactic stellar populations. By resolving the members of stellar systems through photometric observations we are able to perform more detailed measurements to infer their mass. In this paper we investigate the feasibility of a cubesat based mission including an optical payload to directly optically discriminate the members of a selected sample of binary systems. The scientific targets, consisting 11?M class dwarf stars binary systems, have been extracted from the already studied Riaz catalogue. These subset has been selected considering the star distance, the members angular separation, and the distance from the Galactic plane (due to limit the background and foreground contamination). The satellite concept is based on a 6 unit Cubesat embedding some commercial off the shelf components and an ad hoc designed optical payload occupying almost 4 units. The optical configuration has been chosen in order to fit the angular resolution requirements, as derived from the target characteristics. Moreover, according to the optical analysis and the computed field of view some requirements on the attitude control system have been inferred and fulfilled by the component selection. The paper is organized as in the following: a brief scientific introduction is made; consequently the project is described with particular attention to the optical design and the standard sub-systems; finally the conclusions are drawn and the future perspectives are investigated.     

光纤陀螺仪中尖峰脉冲引起漂移 的误差分析及其抑制

首次分析了光纤陀螺仪探测器输出信号中频率固定的尖峰脉冲对光纤陀螺 仪零偏漂移的影响机理,给出了尖峰脉冲影响光纤陀螺仪零偏漂移的误差模型;根据干 涉式数字闭环光纤陀螺仪探测器输出信号的特点,提出了一种基于高速集成模拟开关的 时域选通尖峰脉冲抑制具体实现方法,实验验证了尖峰脉冲引起的零偏漂移大小和理论 分析接近,表明了误差模型的正确性,同时表明该方法能够有效降低尖峰脉冲引起的光 纤陀螺仪零偏漂移。     

光纤环内部应力试验研究

光纤环是光纤陀螺的核心敏感部件,其内部应力值的大小和分布对光纤陀螺的整体性能有很大影响.光纤环的内部应力主要包含拉伸应力、弯曲应力和固化应力等,光纤环的绕制工艺和固化工艺等都会对光纤环的应力产生影响.通过测量不同绕制工艺下光纤环的应力分布和偏振串扰分布,得出光纤环绕制张力越小、光纤环直径越大、固化胶的收缩率越小,光纤环的应力也越小,相应的偏振串扰值也越小,为光纤环绕制技术的提高提供依据.     

基于自回归与最小均方理论的振动环境下 光纤陀螺仪滤波方法

针对振动应力下光纤陀螺产生测量误差增大的问题,从振动对光纤环的影响机理出发,分析了振动应力下光纤陀螺干涉信号的表现形式,提出了基于自回归最小均方滤波理论的光纤陀螺滤波方法,将AR模型的平稳性和最小均方根滤波的自适应性相结合,提取平稳数据的特性参数,对高频信号进行滤波,降低非互易相移产生陀螺角速度误差值的干扰.试验表明,该方法简单可行,有效地降低了振动应力下光纤陀螺输出信息的噪声,抑制了由振动引起的陀螺漂移.     

高强太阳光无线能量传输能量供给平台设计

为了满足微小卫星群落编队飞行技术快速发展的需要,设计了一种能量供给平台.该平台中菲涅尔透镜（太阳能聚集装置）收集空间太阳光,并将聚焦光能耦合进光纤束（柔性转向装置）以进行传输和换向.由3个薄透镜组成的透镜组（二次发射装置）将出射光线整合成高强平行光束进行光能传输,将光能以高强太阳光形式无线传输至航天器群落,实现能量供给.该能量供给平台能量收集传输效率可达到70%以上,在提高效率、降低成本方面具有一定的优越性.