基于加速度计和角速率陀螺的超小无人直升机姿态控制系统

设计了一种基于加速度计和角速率陀螺的超小型无人直升机姿态控制系统；由卡尔曼滤波算法融合加速度计和陀螺数据，实时估计最优的直升机姿态信号；根据最优的姿态反馈信号，飞行控制系统采用参数自整定的模糊PID控制方法得到舵机控制信号，从而实现了超小型无人直升机的姿态控制。     

战斗机的体系对抗分析(英文)

体系对抗分析是武器系统作战效能研究的最高层次。本文建立了空对空作战体系对抗的物理模型 ,基于多元兰彻斯特平方律方程 ,给出了不同空战武器战术交战的数学模型 ,考虑现代战争的高技术特征 ,发展了战役优势参数概念 ,使其更加准确地反映空对空作战的实质。以数学模型和战役优势参数为核心 ,采用随机分配目标战术和战斗机对空作战能力指数 ,完成优势评估、进程预测和配置优化等体系对抗问题的计算分析。结果表明 ,具有发展特征的经典作战理论仍能在新的应用中发挥重要作用。     

某型无人机拦阻网回收系统设计

介绍了无人机拦阻网回收系统的组成和工作原理，论述了系统的网体设计、涡轮阻尼器设计以及拦阻过程计算等关键技术问题，并给出某型无人机拦阻回收系统的性能计算结果。本文的研究成果为某型无人机拦阻网回收系统的工程设计提供了理论依据，并已成功应用于某型无人机系统的研制。     

无人机4D制导系统研究

基于逆运动学方法设计了无人机四维制导系统。基本姿态控制器采用基于在线神经网络的非线性动态逆控制器。动态逆控制器用来对消无人机的非线性，在线神经网络补偿对消不精确引起的状态误差。制导系统的任务就是由给定的三维航迹，解算出航迹角，并生成三个姿态角指令，同时设计发动机控制回路以控制航迹速度，最终实现精确的四维航迹跟随。     

高空高速无人飞行器热控制系统设计

针对飞行时间短、速度和高度变化快、表面温度波动大的无人飞行器UAV(Unmanned Aerial Vehicles)热控制系统设计难题,提出了一种可解决实际工程问题的热分析计算方法.即把热天工况、冷天工况和标准天工况作为设计/试验工况;采用参考温度法、高超音速工程预测法或计算流体动力学CFD(Computational Fluid Dynamics)数值模拟法,确定了飞行器表面温度分布,并把其作为后续热分析数学模型的外边界条件;分析结构热容量对瞬态热载荷的影响,建立与之相应的边值问题方程,并采用有限差分法求解;根据高空高速飞行特点及瞬态热载荷值,确定仪器设备舱调温系统方案.     

Modeling novel methodologies for unmanned aerial systems–Applications to the UAS-S4 Ehecatl and the UAS-S45 Bálaam

The rising demand for Unmanned Aerial Systems(UASs) to perform tasks in hostile environments has emphasized the need for their simulation models for the preliminary evaluations of their missions. The efficiency of the UAS model is directly related to its capacity to estimate its flight dynamics with minimum computational resources. The literature describes several techniques to estimate accurate aircraft flight dynamics. Most of them are based on system identification. This paper presents an alternative methodology to obtain complete model of the S4 and S45 unmanned aerial systems. The UAS-S4 and the UAS-S45 models were divided into four sub-models, each corresponding to a specific discipline: aerodynamics, propulsion, mass and inertia, and actuator. The‘‘aerodynamic" sub-model was built using the Fderivatives in-house code, which is an improvement of the classical DATCOM procedure. The ‘‘propulsion" sub-model was obtained by coupling a two-stroke engine model based on the ideal Otto cycle and a Blade Element Theory(BET) analysis of the propeller. The ‘‘mass and the inertia" sub-model was designed utilizing the Raymer and DATCOM methodologies. A sub-model of an actuator using servomotor characteristics was employed to complete the model. The total model was then checked by validation of each submodel with numerical and experimental data. The results indicate that the obtained model was accurate and could be used to design a flight simulator.     

多飞行器动态目标追踪协同控制研究

多飞行器追踪动态目标是一个协同控制问题,需要根据目标飞行状态,协同各个追踪飞行器的飞行状态,最终能够在某动态的最佳点实现同时到达。考虑到目标具有较强的机动性,轨迹通常为非线性的,设计了一种基于非线性轨迹预测的、以剩余时间为控制变量的一致性控制方案。仿真结果表明,提出的控制方案能够实现空间位置相距较远的多飞行器动态追踪,具有较好的灵活性和收敛性,目标轨迹的预测结果与实际轨迹误差较小,恰当的轨迹估计有助于缩短追踪时间,提高追踪效率。     

小型无人机气动参数辨识的新型HGAPSO算法

针对小型无人机(UAVs)研制中操稳特性和飞行控制律设计评估对气动参数辨识的需求,提出了一种混合遗传粒子群优化算法(HGAPSO)。该算法以粒子群优化算法(PSO)为主体,在粒子优化路径中,引入遗传算法(GA)的交叉变异操作,增强粒子群跳出局部最优的能力;同时采用Kent映射改进粒子种群的初始化,使初始种群在可行解空间内分布更加均匀,增强全局优化能力。基于仿真结果,依据辨识准度及辨识成功率,对比了HGAPSO、常规PSO和GA优化算法气动参数辨识的结果,然后用蒙特卡洛仿真测试随机观测噪声的影响,结果表明该算法兼备PSO算法高的搜索效率和GA算法的全局优化能力,对随机观测噪声不敏感。最后,通过设计小型UAV试飞示例进行综合应用评价,结果表明:HGAPSO算法基于真实试飞数据进行气动参数辨识取得了满意结果,具有良好的实用性。     

小型固定翼无人机绳钩回收过程动力学分析

绳钩回收作为小型固定翼无人机的一种精确定点拦阻无损回收技术,近年来在国内外得到迅速发展。本文以某型无人机的绳钩回收系统为研究对象,对绳钩回收系统进行了参数化处理并建立了两种动力学仿真模型。一是在考虑回收架柔性基础上建立了基于Lagrange方程的绳钩回收系统的动力学仿真模型,二是在考虑绳索变形和系统结构细节基础上建立了基于MSC.ADAMS的绳钩回收系统的多体动力学仿真模型。通过上述两种仿真模型的算例分析以及与某型无人机绳钩回收试验的测试数据作对比,验证了两种动力学仿真模型在绳钩回收系统不同设计阶段的适用性和有效性。     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.