电磁环境监测系统设计

详细地介绍了电磁环境监测系统的研究设计，同时介绍了软件及计算机辅助测试设计。     

民机主制造商对MBD软件供应商工程监控过程研究

基于模型的软件开发技术(Model-Based Development,简称MBD)具有可视化建模与仿真、自动生成符合适航要求的代码等特点,已在民用飞机机载设备研发领域被逐渐推广应用。越来越多使用MBD技术开发的机载软件的涌现,给民机机载软件适航符合性工作带来了前所未有的挑战。为解决这一问题,美国航空无线电技术委员会于2011年底发布了DO-178C作为民用航空界认可的机载软件符合性方法,并在此基础上发布了DO-331作为专门针对机载软件MBD技术的适航符合性要求的补充说明。通过对DO-178C和DO-331标准中MBD软件适用目标的研究,结合工程实践,总结归纳了一套民用飞机主制造商对MBD软件供应商的软件研发过程管控要求,用于在向适航当局表明符合性时提高适航置信度,以期对主制造商和供应商在处理MBD软件方面提供参考。     

空域监视技术的新进展及应用

空域监视系统足对飞行器在空域内的飞行活动进行监视的所有设备的总称.空域监视技术是保障飞行安全、提高运行效率的重要手段.本文首先以机载航电设备的发展为主线,详细分析了空域监视技术的发展历程,指出协同式空域监视的发展离不开机载航电设备的支撑;然后针对协同式空域监视技术面临的新挑战,分析和综述了近年来面向协同式空域监视技术的...     

机载监测系统对地面通信网站空间特性参数的测量分析

基于机载监测系统对地面固定通信站电磁目标的测向定位,提出利用飞行航线上各观测点到辐射源的距离信息和相应的接收机输出电平,对目标有效辐射功率(EIRP)及天线的一些特性参数进行估计的方法。该方法对无线电管理具有一定的参考价值。     

天基海洋目标监视的系统分析及相关研究综述

天基海洋目标监视是现代卫星应用技术的重要发展方向。分析了海洋目标、海洋 监视环境的特点,介绍了天基海洋目标监视资源的分类和发展情况,分析了各种不同类型监 视平台及有效载荷的特点和适用性。综合评述了天基海洋监视中海洋目标检测、分类、识别 等目标信息处理技术,对监视任务的规划调度方法及其他相关研究,分析了这些技术手段 的 特点、适用性及发展现状。最后分析了当前天基海洋目标监视相关研究和应用的发展趋势。
     

基于多DSP技术的SSR实时信号处理机

以4片数字信号处理器(DSP)和2片现场可编程逻辑阵列器件(FPGA)为核心处理器,设计 实现了二次监视雷达SSR(Secondary Surveillance Radar)实时信号处理机.该系统基于2 块DSP+FPGA模式的实时信号处理板,实现了对原始二次监视雷达应答信号的各种处理:反同 步窜 扰处理,反非同步窜扰处理,计算目标的方位、距离,进行目标的高度、代号解码以及实时 产生航管询问编码,并生成各种信息的统计报告.      

航空公司工程管理外委监督体系的实践

针对维修工程管理外委的监督体系和监督实施方法进行了探讨,对同一航空集团下航空公司实施维修工程管理外委具有一定指导意义。     

An optimal beam alignment method for large-scale distributed space surveillance radar system

Large-scale distributed space surveillance radar is a very important ground-based equipment to maintain a complete catalogue for Low Earth Orbit (LEO) space debris. However, due to the thousands of kilometers distance between each sites of the distributed radar system, how to optimally implement the Transmitting/Receiving (T/R) beams alignment in a great space using the narrow beam, which proposed a special and considerable technical challenge in the space surveillance area. According to the common coordinate transformation model and the radar beam space model, we presented a two dimensional projection algorithm for T/R beam using the direction angles, which could visually describe and assess the beam alignment performance. Subsequently, the optimal mathematical models for the orientation angle of the antenna array, the site location and the T/R beam coverage are constructed, and also the beam alignment parameters are precisely solved. At last, we conducted the optimal beam alignment experiments base on the site parameters of Air Force Space Surveillance System (AFSSS). The simulation results demonstrate the correctness and effectiveness of our novel method, which can significantly stimulate the construction for the LEO space debris surveillance equipment.     

基于汇聚点观测的天基光学监视星座设计

针对地球静止轨道目标监视问题,提出了一种基于汇聚点观测的天基光学监视星座设计方法.研究分析了地球静止轨道目标分布特性,针对静止轨道目标在特定位置分布密度较大的特点,设计了监视星座对汇聚点区域进行重点观测的策略.分析了监视星座的轨道类型和传感器观测策略,提出采用太阳同步轨道设计监视星座和相应的汇聚点区域观测的方法.在满足对汇聚点观测要求及同步带重访周期为1d的条件下,对星座进行了设计.仿真结果表明：设计的4颗卫星组成的观测星座,对同步带目标的重访周期小于1d,24 h内的平均观测时间约为900 s,且能观测到更多的同步带目标.该方法可供工程应用参考.     

Ocean Tides in GRACE Monthly Averaged Gravity Fields

The GRACE mission will map the Earth's gravity fields and its variations with unprecedented accuracy during its 5-year lifetime. Unless ocean tide signals and their load upon the solid earth are removed from the GRACE data, their long period aliases obscure more subtle climate signals which GRACE aims at. In this analysis the results of Knudsen and Andersen (2002) have been verified using actual post-launch orbit parameter of the GRACE mission. The current ocean tide models are not accurate enough to correct GRACE data at harmonic degrees lower than 47. The accumulated tidal errors may affect the GRACE data up to harmonic degree 60. A study of the revised alias frequencies confirm that the ocean tide errors will not cancel in the GRACE monthly averaged temporal gravity fields. The S₂ and the K₂ terms have alias frequencies much longer than 30 days, so they remain almost unreduced in the monthly averages. Those results have been verified using a simulated 30 days GRACE orbit. The results show that the magnitudes of the monthly averaged values are slightly higher than the previous values. This may be caused by insufficient sampling to fully resolve and reduce the tidal signals at short wavelengths and close to the poles. This revised version was published online in August 2006 with corrections to the Cover Date.