系统级EMC实验中常见虚假信号的分析与验证

对系统级电磁兼容性试验中常见的虚假信号的产生原因和特点进行了理论分析,并通过软件仿真和试验予以验证,证明虚假信号是低噪声放大器（LNA）等设备在大功率信号的作用下,由于其非线性特性引起的,而实际上并不存在。文章最后给出了虚假信号的判别方法,即通过加减衰减器观察信号幅值的变化,可判断检测信号的真伪。同时,对系统级EMC试验的测试系统给出了改进建议。     

空间飞行器的对接分离与地面模拟试验的仿真分析研究

对两对接飞行器的分离过程和地面模拟试验过程进行了理论分析,论述了两飞行器在分离瞬 间空间分离过程与地面模拟试验过程之间的对应比拟关系;依据地面试验中给出的多种工况 ,利用多体动力学软件ADAMS仿真分析并比对了地面和空间零重力两种环境条件下两飞行器 分离时的运动特性,讨论了地面五自由度对接分离气浮平台模拟两飞行器在空间实际分离时 带来的原理误差影响。     

微小卫星星地数据链路层通讯协议的研究和开发

卫星和地面之间的交流通过它们之间的数据通讯来实现。为了实现星地通讯,必须选定双方都要遵守的协议。考虑到星地通信的可靠性和效率,在选择通讯协议时需遵循实用且最简单的原则。参考CCSDS的相关建议和Ax．25协议,开发了一种星地链路层通信协议。纳星一号飞行试验的运行结果表明,该协议具有较高的数据传榆效率和良好的可靠性,可以满足微小卫星的实际通信要求。     

卫星钟差预报的Kalman算法及其性能分析

钟差预报是卫星导航系统应用中的一项关键技术。Kalman算法作为一种最优预测算法,在原子钟时间尺度、GPS钟差预报中得到了广泛的使用。但是,GPS钟差预报的Kalman模型中通常只考虑了钟差的确定性部分,将随机性部分简单作为白噪声处理。对随机性部分采用幂律谱模型,分析了Kalman算法用于卫星导航系统钟差预报的性能和适用条件。论文首次详细讨论了钟差变化中的确定性部分和随机性部分对钟差预报误差的影响;文中还完善了前人文献中利用阿伦方差计算Kalman预报噪声方差阵的推导;最后利用IGS数据,比较和分析了四种情况下Kalman预报、递推最小二乘和灰色系统GM(1,1)预报精度。结果表明在数据充足的情况下,对于一天内的短期预报,Kalman算法精度最高,预报结果与IGS事后精密钟差的标准差小于10ps。
     

KrF激光对高速飞片的驱动特性研究

利用诱导空间非相干技术平滑的KrF准分子（248nm）激光驱动带有烧蚀层的平面靶，研究激光空间均匀性对产生完整飞片的影响，结果表明激光不均匀性在2％以下，能够产生完整的高速飞片，且完整飞片能够维持20ns以上不破裂；当激光不均匀性达到5％，激光引入流体力学不稳定性种子应很强，冲击波在靶内输运过程中不稳定性不断发展增强，到靶背时强到足以使飞片解体甚至气化，不能产生完整的飞片。为了获得尽可能高的飞片速度，采用激光与烧蚀层参数不匹配方法，使冲击波对飞片作多次加速。利用功率密度为1012 W/cm2的KrF激光与含50μm Kapton烧蚀层的5μm铝飞片作用，得到速度约10km/s的高速飞片，与模拟结果吻合得很好。     

利用和开发Windows自带的VPN技术研究

通过实例,介绍了利用现有的Windows系统的功能,实现VPN的方法,对使用纯软件实现VPN、降低企业联网成本有一定的参考价值。     

Improving regional ionospheric TEC mapping based on RBF interpolation

Radial basis function (RBF) interpolation with multi-quadric is developed to perform ionospheric total electron content (TEC) mapping for the Chinese region between 15°N ~ 40°N and 100°E ~ 125°E. TEC measurements from the Centre for Orbit Determination in Europe (CODE) covering the solar maximum year 2011 are used to investigate the performance of the proposed RBF interpolation method. The differences between the RBF interpolated TEC and the CODE TEC are within 0.5 TECU and the root mean square error (RMSE) is very small when 49 data points are used. The maximum difference is ~5 TECU and the error is less than 1 TECU with 25 samples. Our study suggests that a random distribution of measurement points gives smaller RMSEs than a homogenous distribution when the number of sample points is low. The study indicates that RBF interpolation offers a powerful and reliable tool for ionospheric TEC mapping.     

In-orbit operation and performance of the CubeSat Soft X-ray polarimeter PolarLight

PolarLight is a compact soft X-ray polarimeter onboard a CubeSat, which was launched into a low-Earth orbit on October 29, 2018. In March 2019, PolarLight started full operation, and since then, regular observations with the Crab nebula, Sco X-1, and background regions have been conducted. Here we report the operation, calibration, and performance of PolarLight in the orbit. Based on these, we discuss how one can run a low-cost, shared CubeSat for space astronomy, and how CubeSats can play a role in modern space astronomy for technical demonstration, science observations, and student training.     

Numerical Simulation of Characteristics of CEX Ions in Ion Thruster Optical System

Charge exchange(CEX) ions could inflict severe damages on the ion thruster optical system. This article is aimed at investigating the characteristics of the CEX ions and their influences upon the optical system by means of particle-in- cell(PIC) ion simulation and Monte Carlo collision(MCC) methods. The results from numerical simulation indicate that despite the fact that CEX ions appear in the entire beamlet region near the ion optical system, the ones that present themselves downstream of the accelerator grid have good reason for attracting more attention. As their trajectories are significantly affected by the local electric field, a great number of CEX ions are accelerated toward grids resulting in sputtering erosion. When the influences of the CEX ions are considered in the numerical simulation, there could hardly be observed augments in the screen grid current, but the accelerator grid current increases from zero to 1. 4% of the beamlet current. It can be understood from the numerical simulation that the CEX ions formed in the region far downstream of the accelerator grid should be blamed for the erosion on the downstream surface of the accelerator grid.