基于时间误差补偿的HJ-1C卫星几何定位改进

利用距离多普勒算法对 HJ-1C（“环境一号”C）卫星图像进行定位,其初始定位精度为1100~1400m,不能很好地满足实际应用的需要。进一步分析后发现,HJ-1C卫星图像几何定位误差主要分布在方位向,通过对影响HJ-1C卫星几何定位精度的因素进行分析,得出合成孔径雷达（Synthetic Aperture Radar, SAR）时间误差是影响几何定位的关键因素,因此文章提出通过时间误差补偿提高HJ-1C卫星几何定位精度。该方法首先计算SAR时间误差,然后对SAR载荷时间进行补偿,最后利用距离多普勒算法进行定位,并对HJ-1C卫星图像进行了验证。结果表明,HJ-1C卫星定位精度提高到300m左右,得到了有效的改进。     

F1方程式赛车后升力翼的气动特性

以比例为1∶3的F1方程式赛车后升力翼为研究对象,研究了后升力翼攻角变化对F1方程式赛车气动阻力和气动升力的影响规律.在攻角为12°时,气动升力与气动阻力的比值的绝对值达到最大,此攻角就是F1方程式赛车后升力翼的最佳攻角,模型风洞试验验证了这一结论.      

基于傅里叶变换的HY-1B卫星影像条带噪声去除

HY-1B卫星是中国第二颗海洋遥感卫星,水色水温扫描仪（COCTS）是其主要载荷。文章针对COCTS图像条带噪声的特点,采用傅里叶变换方法,设计了一种新的滤波器,对图像进行条带噪声去除．并同传统的低通滤波方法处理结果进行比较。实验结果表明,新的傅里叶变换方法能够有效地去除图像的条带噪声,其去除效果要优于传统的低通滤波方法。     

基于小波变换的卫星阻力系数分析

以不同弧长解算天宫一号空间实验室连续55天（d） GPS轨道数据得到卫星阻力系数Cd 序列,并对同期的太阳辐射通量 f 10.7 和地磁活动指数 ap,Ap序列高、低频多层小波分解。空间环境参量和Cd 序列各层信号滑动相关性的统计分析结果表明小波分解的阻力系数序列与对应的 f 10.7 ,Ap 序列整体具有很好的滞后相关性,验证了通过 f 10.7 ,Ap 预报 Cd 的可行性。对不同回归模型和回归分析样本序列长度n分析Cd预报值残差表明：采用f 10.7 一元回归模型,并取n20 d时, Cd 预报结果最优。另外,NRLMSIS-00模型在350km高度的中低纬度区域,地磁活动上升相响应过度,而下降相则响应不足;太阳辐射通量上升相响应适度,下降相响应过度。最后对应用前景进行总结,该方法对提高航天器轨道预报精度具有重要参考价值。     

偏置动量小卫星抗干扰能力分析与验证

环境减灾-1A、1B（HJ-1A、1B）卫星和海洋-1B（HY-1B）卫星是三颗偏置动量小卫星,均采用偏置动量轮控制和磁力矩器控制,其姿态控制系统具有较强的抗干扰能力。文章对该卫星的抗干扰能力进行了分析和仿真,并根据在轨运行数据给出了验证结果,表明控制系统具有一定的控制精度和稳定性。     

自动化测试系统在环境减灾-1A、1B卫星中的应用

在环境减灾-1A、1B（HJ-1A、1B）卫星的研制中,双星并行电性能综合测试是一个非常复杂和细致的过程,为此应用了卫星自动化测试系统,实现了测试信息的集中管理、测试数据的综合利用和测试流程的自动化,提高了测试工作的效率和质量。文章介绍HJ-1A、1B双星并行自动化综合测试系统,主要阐述测试实时数据库、自动化测试控制台、参数自动化监视软件等。     

Operation and Application of A, B Satellites for Environment and Disaster Monitoring and Forecasting

Environment and disaster monitoring and forecasting small satellite constellation A and B satellites (HJ-1-A, B) are called "environment and disaster reduction satellites A and B' for short. The constellation adopts a 10:30 LT sun-synchronous circular orbit, with orbit altitude of 649 km. HJ-1-A and HJ-1-B are distributed with a phase difference of 180o in the same orbital plane, so as to enhance the time resolution of earth observation. The satellites have orbit maintenance capability, the lifetime is 3 years. Both satellites adopt CAST968 platforms. Two wide-coverage multispectral CCD cameras with resolution 30 m and width 700 km, a super-spectral imager with resolution 100 m and width 50 km as well as a data transmission subsystem of 120 Mbit/s are deployed on HJ-1-A, which also carries Ka communication testing equipment of Thailand. HJ-1-B has two wide-coverage multispectral CCD cameras (the same as satellite A), one infrared camera with resolution 150 m and width 720 km and a data transmission subsystem of 60 Mbit/s. The coverage period of the wide-coverage multispectral CCD camera is 48 hours. The revisit period of super-spectral imager is 96 hours and the coverage period of infrared camera is 96 hours.      

高声强声场模拟装置设计与声试验1/3倍频程控制技术研究

为了提高混响室声场模拟能力,北京卫星环境工程研究所自研一套高声强声场模拟试验设备。文章介绍了该设备的行波管发声系统设计和消声降噪处理过程——行波终端设计以及声试验控制仪器的原理。经过调试试验验证,测量结果满足声压级165 d B行波声场的要求,行波管试验段性能良好,达到167.9 d B,消声道出口噪声能够满足环境模拟需求。     

固体火箭发动机动力相似准则研究

本文以小发动机模拟大发动机为目标，探讨固体火箭发动机的动力相似准则，首先把动力相惟问题归结为燃烧室，喷管一体化流动的相似问题，通过对全三维Ｎ－Ｓ方程所进行的无量纲化分析，在几何相似的前提下，得到固体火箭发动机动力的流上似准则，再通过对控制方程的单值性条件所进行了无量纲化分析，得到了在初始状相似条件下的燃速相似准则；另外还得到了飞行条件相似、燃烧温度相似以及普朗特数相等。并进一步对这些准则进行了分析     

Fast solar radiation pressure modelling with ray tracing and multiple reflections

Physics based SRP (Solar Radiation Pressure) models using ray tracing methods are powerful tools when modelling the forces on complex real world space vehicles. Currently high resolution (1?mm) ray tracing with secondary intersections is done on high performance computers at UCL (University College London). This study introduces the BVH (Bounding Volume Hierarchy) into the ray tracing approach for physics based SRP modelling and makes it possible to run high resolution analysis on personal computers. The ray tracer is both general and efficient enough to cope with the complex shape of satellites and multiple reflections (three or more, with no upper limit). In this study, the traditional ray tracing technique is introduced in the first place and then the BVH is integrated into the ray tracing. Four aspects of the ray tracer were tested for investigating the performance including runtime, accuracy, the effects of multiple reflections and the effects of pixel array resolution.Test results in runtime on GPS IIR and Galileo IOV (In Orbit Validation) satellites show that the BVH can make the force model computation 30–50 times faster. The ray tracer has an absolute accuracy of several nanonewtons by comparing the test results for spheres and planes with the analytical computations. The multiple reflection effects are investigated both in the intersection number and acceleration on GPS IIR, Galileo IOV and Sentinel-1 spacecraft. Considering the number of intersections, the 3rd reflection can capture $99.12\%\text{,}99.14\%$, and $91.34\%$ of the total reflections for GPS IIR, Galileo IOV satellite bus and the Sentinel-1 spacecraft respectively. In terms of the multiple reflection effects on the acceleration, the secondary reflection effect for Galileo IOV satellite and Sentinel-1 can reach 0.2?$\text{nm}/{\text{s}}^2$ and 0.4?$\text{nm}/{\text{s}}^2$ respectively. The error percentage in the accelerations magnitude results show that the 3rd reflection should be considered in order to make it less than $0.035\%$. The pixel array resolution tests show that the dimensions of the components have to be considered when choosing the spacing of the pixel in order not to miss some components of the satellite in ray tracing. This paper presents the first systematic and quantitative study of the secondary and higher order intersection effects. It shows conclusively the effect is non-negligible for certain classes of misson.