Measurement of cosmic ray elemental composition from the CAKE balloon experiment

CAKE (Cosmic Abundances below Knee Energies) was a prototype balloon experiment for the determination of the charge spectra and abundances of the primary cosmic rays (CR) with Z > 10. It was a passive instrument made of layers of CR39® and Lexan®/Makrofol® nuclear track detectors; it had a geometric acceptance of ∼0.7 m² sr for Fe nuclei. Here, the scanning and analysis strategies, the algorithms used for the off-line filtering and for the tracking in automated mode of the primary cosmic rays are presented, together with the resulting CR charge distribution and their abundances.     

目标捕获后航天器组合体的角动量转移与抑振规划

针对失稳目标捕获后航天器组合体的位姿调整与稳定问题，提出一种组合体角动量转移与振动抑制复合规划方法。首先建立了同时考虑了空间机械臂、目标卫星太阳翼、服务卫星太阳翼等柔性构件的航天器组合体动力学模型。然后提出角动量转移优化方法，规划机械臂最终构型，保证组合体相对稳定后的角速度最小；基于粒子群算法设计了机械臂最优抑振轨迹规划方法，抑制角动量转移过程中的机械臂和太阳翼的柔性振动。最后通过数值仿真验证了规划方法的有效性。仿真结果表明，该方法能够有效实现组合体的角动量转移，并显著降低组合体的柔性振动，具有工程实用性。     

基于光切法测量的曲面重构技术

从实际应用出发,论述了光切法应用于曲面数据采样的原理及方法;对采样数据的预处理技术进行了简要总结,详细讨论了点云数据的精简,提出采用简化多边形来精简点云数据的方法;并说明在Geomagic环境下进行数据精简以及曲面重构技术的应用,证明了该方法的有效性.     

Investigations of an integrated angular velocity measurement and attitude control system for spacecraft using magnetically suspended double-gimbal CMGs

This paper presents an integrated angular velocity measurement and attitude control system of spacecraft using magnetically suspended double-gimbal control moment gyros (MSDGCMGs). The high speed rotor of MSDGCMG is alleviated by a five-degree-of-freedom permanent magnet biased AMB control system. With this special rotor supported manner, the MSDGCMG has the function of attitude rate sensing as well as attitude control. This characteristic provides a new approach to a compact light-weight spacecraft design, which can combine these two functions into a single device. This paper discusses the principles and implementations of AMB-based angular velocity measurement. Spacecraft dynamics with DGMSCMG actuators, including the dynamics of magnetically suspended high-speed rotor, the dynamics of inner gimbal and outer gimbal, as well as the determination method of spacecraft angular velocity are modeled, respectively. The effectiveness of the proposed integrated system is also validated numerically and experimentally.     

宽带信号角跟踪和四通道单脉冲方案

分析了宽带信号角跟踪的特殊问题及其实现方案。基于互相关函数的角误差检测方法,推导出了在非相关噪声及相关噪声背景下差路信号的输出信噪比及其角度随机误差的数学表达式,进而给出了带宽增益和最佳带宽的概念,以及提高输出信噪比的方法。为了在低载噪比（C/N）时获得角捕获所需要的和路信号以及差路的归一化信号,提出了四通道单脉冲方案。最后归纳出了低C/N时宽带信号角捕获和角跟踪的几种方法并提出了建议。     

利用GPS进行角速度确定的研究

提出了一种利用GPS进行载体角速度测量的方法 ,建立了测量数学模型 ,并进行了计算机仿真 ,仿真结果表明 ,该方案可以得到较为满意的结果     

微机-机械扫描阀测压系统精确度改善与提高

本文对采用计算机-机械扫描阀测压系统在压力测量过程中影响测量精确度的诸因素进行了分析,介绍了改善和提高其测量精确度的几种方法。结果表明:效果显著,方法正确。     

曲面零件五坐标扫描检测路径产生方法研究

针对曲面零件对五坐标扫描检测的需求,在对REVO五坐标旋转扫描测头的技术特征进行分析的基础上,提出了适用于五坐标扫描检测路径规划的球面法,通过测尖运动球形包络面与被测工件曲面的相交线来确定检测路径,测量主要由测尖扫描完成,减少测量机的三轴移动,实现高速坐标扫描测量。     

微小卫星多约束姿态机动规划方法

针对微小卫星姿态控制中存在的多重指向约束和角速率约束问题，提出一种基于对数型势函数的多约束姿态机动规划方法。首先针对微小卫星携带的光学传感器需躲避强光天体而天线需指向地面保证对地通信这一约束特性，采用对数型势函数方法保证约束姿态指向满足任务要求;其次，针对姿态角速率限制的问题，引入障碍Lyapunov函数确保姿态角速率始终处于约束范围内。与在线优化方法相比，该方法具有计算量小的显著优势，非常适合星上处理能力有限的微小卫星。此外，考虑外界干扰力矩的影响，引入自适应干扰估计律，增强了控制系统的鲁棒性。最后，通过数学仿真对本文方法进行了校验，仿真结果表明，该方法能够快速实现卫星姿态机动到期望指向，与此同时，在整个姿态机动过程中，均满足多重指向约束和姿态角速率约束 要求 。     

Multiple Coulomb scattering method to reconstruct low-energy gamma–ray direction in the GAMMA-400 space-based gamma–ray telescope

The GAMMA-400 currently developing space-based gamma-ray telescope is designed to measure the gamma-ray fluxes in the energy range from ～20?MeV to several TeV in the highly elliptic orbit (without shadowing the telescope by the Earth) continuously for a long time. The physical characteristics of the GAMMA-400 gamma-ray telescope, especially the angular and energy resolutions (at 100-GeV gamma rays they are ～0.01° and ～1%, respectively), allow us to consider this space-based experiment as the next step in the development of extraterrestrial high-energy gamma-ray astronomy. In this paper, a method to improve the reconstruction accuracy of incident angle for low-energy gamma rays in the GAMMA-400 space-based gamma-ray telescope is presented. The special analysis of topology of pair-conversion events in thin layers of converter was performed. Applying the energy dependence of multiple Coulomb scattering for pair components, it is possible to estimate the energies for each particle, and to use these energies as weight in the angle reconstruction procedure. To identify the unique track in each projection the imaginary curvature method is applied. It allows us to obtain significantly better angular resolution in comparison with other methods applied in current space-based experiments. When using this method for 50-MeV gamma rays the GAMMA-400 gamma-ray telescope angular resolution is about 4°.