基于全零点FIR前向滤波网络的超分辨成像方法研究

距离多普勒成像的距离分辨率和横向分辨率,分别取决于发射信号的有效带宽和目标相对于雷达在相干积累时间内的转角。采用的方法可以突破上述的限制,其方法是采用全零点FIR 前向滤波网络,在成像处理前进行线性预测滤波,仿真结果表明,这是一种改善距离多普勒成像雷达分辨率的有效方法。     

反射器夹层面板精密成形原理

对高精度、大面积不可展双曲反射面的制造问题,提出了基于"离散钉模、真空负压、蜂窝夹层、应力释放、回弹补偿"的高精度反射面板成形原理;建立了四边自由面内多点约束的薄板大挠度弯曲解法及夹层板成形过程仿真模型,用于确定成形工艺参数;利用动力显式和静力隐式算法相结合的方法实现成形过程仿真;通过开缝和开槽方法释放面内压应力,确定了面板开缝和开槽方案;通过逆向修正离散模包络面,使其与成形模拟得到的夹层板型面误差最小,得到模具修正因子,补偿回弹误差.在此基础上开发了夹层板精密成形CAE系统.该方法制造的面板型面精度RMS达到25 μm以下,已成功地应用于多项大型紧缩场和毫米波天线的制造.      

高超声速钝锥模型及其尾迹红外辐射实验研究

介绍了利用InSb红外辐射计在弹道靶上测量底部直径为10mm、半锥角和头部半径分别为9°、2.2mm(模型A),8°、0.6mm(模型B)的两种非烧蚀钝锥模型及其尾迹的红外辐射.模型速度大于6km/s,飞行环境压力约4.8kPa,红外辐射测量波段为1~3μm、3~5μm.结果表明:非烧蚀钝锥模型头身部红外辐射远大于尾迹红外辐射,在相同飞行速度和环境压力条件下,模型A产生的红外辐射比模型B产生的红外辐射强.     

利用RDSS系统测量数据提取电离层TEC参数的研究

提出了一种基于无线测定卫星业务(RDSS)系统观测数据提取电离层TEC参数的方法,利用此方法计算分析了2006年5月地面中心地区电离层垂向TEC的日变化趋势.研究结果表明,利用RDSS系统观测数据提取的电离层垂向TEC,在北京时间每日凌晨0400时左右达到最小值,在午后1400时左右达到最大值,符合电离层TEC参数受太阳活动影响较大的物理规律.结果说明研究方法是可行且有效的,文章还对可能存在的误差进行了探讨.      

复调制ZFFT的TMS320C25实现

介绍了用ＴＭＳ３２０Ｃ２５数字信号处理器实现复调制ＺｏｏｍＦＦＴ（ＺＦＦＴ）频率细化技术，在所举的例子中，用１０２４复数点选带ＦＦＴ获得通常８１９２复数点基带ＦＦＴ的频率分辨力。实验结果表明，此种频率细化方法特别适用于不能同时处理Ｎ点，而又要求Ｎ点ＦＦＴ频率分辨力的频谱分析场合，文中给出了几种提高Ｃ２５ＦＦＴ运算速度的方法，使１０２４复数点ＦＦＴ的运算时间减少到１２．６ｍｓ，可供工程应用参考。     

弹载遥测传输设备回顾与展望

分三个阶段对北京遥测技术研究所弹箭遥测传输设备五十年来的发展历程作了简要回顾,阐述了遥测传输设备在不同时期的技术应用与发展,总结现阶段遥测传输设备的技术状况,并提出未来几年弹载遥测的发展方向及需要解决的问题。     

基于ICCD的空间微光成像系统成像性能研究

研究基于像增强型CCD（ICCD）的空间高分辨率微光成像系统的成像性能。通过理论推导及数学仿真的方法，对系统在微光条件下的能量传递、极限分辨力、信噪比以及调制传递函数进行分析计算。研究表明，系统在黎明照度条件下具有较好探测能力，通过对ICCD器件制冷可以有效提高系统信噪比，实现满月照度的探测成像。     

Whipple防护屏弹道极限参数试验

在中国空气动力研究与发展中心FD-18A超高速碰撞靶上进行了Whipple防护屏的超高速撞击试验。弹丸为LY12铝球,撞击速度为4.5km/s,撞击角为0°。通过固定弹丸速度、变弹丸直径、寻找弹丸临界直径的办法获得了该Whipple防护屏在试验条件下的弹道极限参数。试验结果表明速度为4.5km/s时的弹丸临界直径为0.35cm,大于用Christiansen方程预测的0.27cm。     

紧缩平面场扫描架系统研制

紧缩平面场(CATR)是在较小的微波暗室里模拟远场的电磁环境,以行进各种天线的测量和研究.其最终性能指标要由紧缩平面场扫描架评定.根据紧缩平面场扫描测量原理,及其对扫描架平面度、直线度、定位精度及自动化程度的要求,研制了极坐标型紧缩场扫描架系统,通过采用高精度直线导轨、平面度微调方式和基于工业控制计算机的数字控制技术,达到了所要求的检测精度,满足了紧缩平面场扫描测量的要求.     

Mitigation of receiver biases in ionospheric observables from PPP with ambiguity resolution

PPP (Precise Point Positioning) is a GNSS (Global Navigation Satellite Systems) positioning method that requires SSR (State Space Representation) corrections in order to provide solutions with an accuracy of centimetric level. The so-called RT-PPP (Real-time PPP) is possible thanks to real-time precise SSR products, for orbits and clocks, provided by IGS (International GNSS Service) and its associate analysis centers such as CNES (Centre National d'Etudes Spatiales). CNES SSR products also enable RT-PPP with integer ambiguity resolution. In GNSS related literature, PPP with ambiguity resolution (PPP-AR) in real-time is often referred as PPP-RTK (PPP – Real Time Kinematic). PPP-WIZARD (PPP - With Integer and Zero-difference Ambiguity Resolution Demonstrator) is a software that is made available by CNES. This software is capable of performing PPP-RTK. It estimates slant ionospheric delays and other GNSS positioning parameters. Since ionospheric effects are spatially correlated by GNSS data from active networks, it is possible to model and provide ionospheric delays for any position in the network coverage area. The prior knowledge ionospheric delays can reduce positioning convergence for PPP-RTK users. Real-time ionospheric models could benefit from highly precise ionospheric delays estimated in PPP-AR. In this study, we demonstrate that ionospheric delays obtained throughout PPP-AR estimation are actu ally ionospheric observables. Ionospheric observables are biased by an order of few meters caused by the receiver hardware biases. These biases prohibit the use of PPP-WIZARD ionospheric delays to produce ionospheric models. Receiver biases correction is essential to provide ionospheric delays while using PPP-AR based ionospheric observables. In this contribution, a method was implemented to estimate and mitigate receiver hardware biases influence on slant ionospheric observables from PPP-AR. In order to assess the proposed approach, PPP-AR data from 12 GNSS stations were processed over a two-month period (March and April 2018). A comparison between IGS ionospheric products and PPP-AR based ionospheric observables corrected for receiver biases, resulted in a mean of differences of −39 cm and 51 cm standard deviation. The results are consistent with the accuracy of the IGS ionospheric products, 2–8 TECU, considering that 1 TECU is ~16 cm in L1. In another analysis, a comparison of ionospheric delays from 5 pairs of short baselines GNSS stations found an agreement of 0.001 m in mean differences with 22 cm standard deviation after receiver biases were corrected. Therefore, the proposed solution is promising and could produce high quality (1–2 TECU) slant ionospheric delays. This product can be used in a large variety of modeling approaches, since ionospheric delays after correction are unbiased. These results indicate that the proposed strategy is promising, and could benefit applications that require accuracy of 1–2 TECU (~16–32 cm in L1).