空间大气成分探测傅立叶变换红外光谱仪

文章阐述了用于空间大气成分探测傅立叶变换红外光谱仪的国外发展状况,主要介绍了几种国外先进的高分辨率空间大气探测用傅立叶变换红外光谱仪的结构、应用范围和技术指标,比较了这几种设备的优缺点和技术特点。     

开发月球车用的月表环境的地面模拟方法研究

当前中国正在进行自己的探月工程,预计将会发射月球车登陆月球表面.在研制月球探测器过程中,为了在地面验证月球车的可靠性和各项功能(如着陆冲击、自主巡航和遥控),必须建立相应的地面试验中心.根据目前对月球表面环境的认识和现有的仿真技术,文章提出了实现月表综合环境模拟的试验设施的设想.由于月球表面环境非常恶劣并且月表的地形也非常复杂,文章提出了一种组合式月表环境模拟器的设想.主要部分是模拟各种月貌特征(如陨石坑、斜坡、沟壑等)的可移动单元.每个单元是一个用模拟月壤制作的小沙盘,其化学成分、组成颗粒分布和力学性能和已经获取的真实月壤样品相似.根据不同的试验要求,选择相应的单元按照一定的规律组合成为试验场.这样在有限的场地面积内可以按需实现对月表不同地域的地貌特征模拟.同时,可以选择少量单元的组合构成更小规模的试验场,以方便与其它环境模拟器(如落塔,热/真空容器等)联合,实现模拟月表的综合环境.     

面向对象技术的防空导弹Simulink建模与仿真

为防空导弹系统性能改进研究和优化设计,提出了一种新的方法,首先给出了一般防空导弹制导控制系统的数学模型,并采用面向对象建模技术结合动态仿真软件Simulink建立了仿真模型并进行了仿真研究,该模型具有容易理解,可重复使用,易于扩展等优点,即通过部分模块更换或改变参数等就可对该系统在其他条件下进行仿真,仿真结果和实际遥测数据基本吻合,表明了该模型和方法的有效性和实用性。     

谐振式加速度计自激振荡电路性能评价方法的研究

针对谐振式加速度计成品率不高、精度低等问题,以石英振梁加速度计为例,采用引进标准信号,将谐振电路作为"黑盒子",对其开展独立的评价.通过评价电路的驱动电压幅值稳定性、移相稳定性、全温幅值/相位对称性等指标,与加速度计实际指标建立了一一对应的关系,为加速度计研制与性能提升提供了有效依据.实际运用表明,电路噪声性能、温度性...     

快速阀控制电路

本文介绍快速阀控制电路的用途、技术指标、框图及电路原理。对克服严重现场干扰、使控制电路具有高度可靠性方面所采取的具体措施也进行了比较系统的介绍。     

高超声速飞行器二元进气道试验和计算

设计了一种吸气式面对称高超声速飞行器,针对进气道性能,分别在两座风洞开展通流试验研究。针对第1次风洞试验大攻角状态(α=8°)测量值偏离线性的问题,辅助采用数值模拟手段分析原因,并对试验方案进行改进设计,解决了首次试验出现的问题。结果显示,在典型状态(Ma=5~6)下,进气道起动正常,性能良好,具有一定的抗侧滑能力;随来流马赫数增加,进气道流量系数增大,总压恢复系数减小,计算结果和试验结果一致;试验结果和数值计算的差异主要表现为基本测压方案α>4°后,流量系数和总压恢复系数出现严重的非线性。数值模拟结果表明,主要原因为模型支撑方式及测压方式所引起的偏差,通过改进试验方案,解决了大攻角状态下测量值偏离正常趋势的问题。     

自适应天线抗干扰性能研究

分析了适用于雷达抗干扰的一些自适应天线波束形成算法,将子空间正交投影算法应用于雷达抗干扰,针对子空间分解过程中特征向量不能完全正交的问题,采用约束化子空间分解算法,来保证子空间特征向量的正交性.最后通过仿真证明:子空间跟踪算法相对于传统的一些自适应算法具有更强的抗干扰性能.     

地球同步卫星BSR硅太阳电池阵输出功率衰减规律分析

长期受粒子辐照、紫外辐照等因素的影响,地球同步卫星的太阳电池阵输出功率会出现较为明显的衰减。这里选取某地球同步卫星使用的背表面反射(BSR)硅太阳电池阵为研究对象,采用光强因子和温度因子修正太阳电池阵的输出功率,使用局部加权回归散点平滑法(LOWESS)分析了其在设计寿命期间的输出功率衰减规律;同时基于LOWESS建立了预测模型,用于硅太阳电池阵超寿运行期间的功率预测。实测数据表明:本文构建的预测模型可以满足超寿地球同步卫星在轨管理使用需求。     

Application in prestiction friction compensation for angular velocity loop of inertially stabilized platforms

To overcome the influence of the nonlinear friction on the gimbaled servo-system of an inertial stabilized platforms(ISPs) with DC motor direct-drive, the methods of modeling and compensation of the nonlinear friction are proposed. Firstly, the inapplicability of LuGre model when trying to interpret the backward angular displacement in the prestiction regime is observed experimentally and the reason is deduced theoretically. Then, based on the dynamic model of direct-drive ISPs, a modified LuGre model is proposed to describe the characteristic of the friction in the prestiction regime. Furthermore, the state switch condition of the three friction regimes including presliding, gross sliding and prestiction is presented. Finally, a composite compensation controller including a nonlinear friction observer and a feedforward compensator based on the novel LuGre model is designed to restrain the nonlinear friction and to improve the control precision. Experimental results indicate that compared with those of the conventional proportion–integration–differentiation(PID) control method and the PID plus LuGre model-based friction compensation method, the dwell-time has decreased from 0.2 s to almost 0 s, the position error decreased to 86.7%and the peak-to-peak value of position error decreased to 80% after the novel compensation controller is added. It concludes that the composite compensation controller can greatly improve the control precision of the dynamic sealed ISPs.     

A nonlinear background removal method for seismo-ionospheric anomaly analysis under a complex solar activity scenario: A case study of the M9.0 Tohoku earthquake

A precise determination of ionospheric total electron content (TEC) anomaly variations that are likely associated with large earthquakes as observed by global positioning system (GPS) requires the elimination of the ionospheric effect from irregular solar electromagnetic radiation. In particular, revealing the seismo-ionospheric anomalies when earthquakes occurred during periods of high solar activity is of utmost importance. To overcome this constraint, a multiresolution time series processing technique based on wavelet transform applicable to global ionosphere map (GIM) TEC data was used to remove the nonlinear effect from solar radiation for the earthquake that struck Tohoku, Japan, on 11 March, 2011. As a result, it was found that the extracted TEC have a good correlation with the measured solar extreme ultraviolet flux in 26–34 nm (EUV_26–34) and the 10.7 cm solar radio flux (F_10.7). After removing the influence of solar radiation origin in GIM TEC, the analysis results show that the TEC around the forthcoming epicenter and its conjugate were significantly enhanced in the afternoon period of 8 March 2011, 3 days before the earthquake. The spatial distributions of the TEC anomalous and extreme enhancements indicate that the earthquake preparation process had brought with a TEC anomaly area of size approximately 1650 and 5700 km in the latitudinal and longitudinal directions, respectively.