Gravity wave propagation studies using the Indian MST radar observations

The Indian MST radar facility at Gadanki (13.5°N, 79.2°E) has been utilised to study the propagation of gravity waves from the troposphere/lower stratosphere to the mesosphere and their interaction with the radar backscattered signal variations. The main objective is to correlate vertically propagating gravity waves derived from the tropospheric velocity fields with the dynamics of mesospheric scattering centres. The tropospheric wind velocities and signal strengths over the entire height range have been subjected to power spectral and wavelet analysis to determine the predominant wave periods/amplitudes and the coupling between the lower atmosphere and mesosphere. Results show that (a) the gravity waves are clearly detectable near tropopause heights, (b) while relatively higher period gravity waves (20–50 min) interact with mesospheric scattering centres, the lower period waves (<20 min) are absorbed in the troposphere itself, (c) the mesospheric scattering layers are affected by gravity waves of complementary periods.     

基于联合参数建模的雷达辐射源识别方法

针对现代雷达采用复杂体制造成的不能正确识别辐射源问题,提出一种基于联合参数建模的雷达辐射源识别方法。该算法首先对辐射源进行脉冲等级和统计参数等级的联合建模,然后将联合参数模型用于识别过程中,基于特征参数的不同描述模型构建不同的识别算法,其中特征参数的联合建模思想是本方法的核心。仿真实验表明,本文方法能够实现对复杂体制雷达辐射源的建模和识别。     

美国海基导弹拦截卫星任务的毁伤分析

基于经验模型和基本假设,研究了航天器撞击的解体特性,计算了碎片的尺寸分布、面质比分布和速度分布,考虑生存高度和大气阻力的影响计算了各种碎片的轨道寿命,提出了碎片留轨比例及数量的计算公式,分析了不同尺寸的碎片的留轨特性.结果表明:这次任务产生的碎片将快速坠毁,对空间环境的影响有限.分析结果可以作为参考,更准确的结果有赖于根据实际观测数据进行深入、详细的分析.     

用于微波雷达动目标检测的回波模拟器的设计与实现

文章介绍了一种用于雷达动目标检测的回波模拟器的设计与实现,以FPGA和DDS器件为硬件核心、软硬件相结合的方式,设计了回波模拟器系统,可靠有效地完成了微波雷达的静态、动态实验室调试和测试。该回波模拟器能够满足对雷达运动目标进行回波模拟的要求,降低了系统调试成本,减小了外场实验难度。     

基于深度神经网络的空间目标结构识别

利用空间目标雷达散射截面(Radar Cross Section, RCS)序列开展空间目标结构识别是空间态势感知的重要组成部分。文章针对 RCS序列受目标物理特性、姿态特性影响大,序列信号非平稳特征明显的问题,利用深度神经网络（Deep Neural Network,DNN）算法解决空间目标结构特征识别的问题;针对特征提取不具区分度的问题,提出利用分形分析提取RCS序列的分数维特征,并利用Fisher判决率对传统特征进行选取;介绍了DNN算法以及数据处理过程;最后,利用一组仿真测试数据对算法进行了仿真验证。分析结果表明,DNN算法在解决利用RCS序列进行目标结构识别这一问题中具有鲁棒性强、识别准确的特点。     

弹体结构平方米级扇形区域脉冲外压加载技术

针对弹体外表面平方米级区域的高峰值、短脉宽压力加载难题,依据一维可压缩流设计了高压腔、膜片腔、试验腔的气腔加载系统,附加了与试验件随形、扩展加压面积、均化压力分布的水腔,实现了平方米级区域1 MPa峰值、10 ms上升沿的脉冲压力加载要求,建立了弹性水腔的两自由度压力分析模型,获得了水腔系统的动特性参数,计算拟合曲线与...     

Modeling of LEO orbital debris populations for ORDEM2008

The NASA Orbital Debris Engineering Model, ORDEM2000, is in the process of being updated to a new version: ORDEM2008. The data-driven ORDEM covers a spectrum of object size from 10 μm to greater than 1 m, and ranging from LEO (low Earth orbit) to GEO (geosynchronous orbit) altitude regimes. ORDEM2008 centimeter-sized populations are statistically derived from Haystack and HAX (the Haystack Auxiliary) radar data, while micron-sized populations are estimated from shuttle impact records. Each of the model populations consists of a large number of orbits with specified orbital elements, the number of objects on each orbit (with corresponding uncertainty), and the size, type, and material assignment for each object. This paper describes the general methodology and procedure commonly used in the statistical inference of the ORDEM2008 LEO debris populations. Major steps in the population derivations include data analysis, reference-population construction, definition of model parameters in terms of reference populations, linking model parameters with data, seeking best estimates for the model parameters, uncertainty analysis, and assessment of the outcomes. To demonstrate the population-derivation process and to validate the Bayesian statistical model applied in the population derivations throughout, this paper uses illustrative examples for the special cases of large-size (>1 m, >32 cm, and >10 cm) populations that are tracked by SSN (the Space Surveillance Network) and also monitored by Haystack and HAX radars operating in a staring mode.     

集中空调新风系统常见故障及排除方法

通过对空调新风系统重要性的分析,指出了影响集中空调系统新风量和新风品质的原因,提出了运用预埋法兰连接风管来保证新风量,在通风井底部设检查口清理新风竖井保证新风品质。     

磁暴期间的地磁导航精度分析

地磁导航是无源自主导航技术研究的新方向. 分析了地磁导航的基本原理, 描述了典型磁暴过程, 并针对地磁导航在磁暴环境中的适用性进行了研究. 在采用曲面样条方法对实测地磁场数据建立观测模型的基础上, 结合广义卡尔曼滤波方法讨论了磁暴不同阶段对地磁导航精度造成的影响. 分别采用理论典型磁暴数据以及实测磁暴数据进行仿真, 仿真结果表明, 在磁暴的初相、恢复相的中后时段以及中等强度以下的磁暴全过程仍然可以采用地磁来进行导航定位, 导航精度在200 m以内, 满足飞行器中程制导的精度要求.