基于极大似然估计器的GNSS矢量跟踪算法

矢量跟踪是一种将全球导航卫星系统(GNSS)接收机的信号跟踪与导航解算融为一体的跟踪算法。传统的基于矢量延迟/频率锁定环(VDFLL)的跟踪算法普遍采用延迟锁定环(DLL)和锁频环(FLL)鉴别器计算伪距和伪距率偏差观测量,由于锁频环鉴别器存在近似误差和一步延迟效应,在高动态环境下容易造成环路失锁。从直接估计卫星信号特征参数的角度出发,基于中频信号模型构建码相位和载波多普勒的极大似然代价函数,采用非迭代估计算法得到各通道码相位和多普勒频移的估计偏差,转换为卡尔曼滤波器的观测矢量,提出一种基于极大似然估计器(MLE)的矢量跟踪算法。理论分析和仿真结果表明:新算法结合了极大似然估计和矢量跟踪的优点,克服了FLL的延迟效应,与基于VDFLL的矢量环路相比,高动态环境下的跟踪稳定性更好,可以对被遮挡的卫星保持持续的跟踪。     

主动冷却燃烧室燃烧与传热耦合过程迭代分析设计方法

为了对主动冷却超燃冲压发动机进行研究与设计,采用实验与计算相结合的方法,对主动冷却超燃冲压发动机燃烧室内传热与燃烧的耦合过程进行了分析。该方法采用燃烧室静压分布的测量值作为输入条件,开展燃气-结构-燃料耦合传热分析,获得经过冷却系统后燃料的状态参数;将燃料的状态参数作为实验参数,开展直联式超声速燃烧实验,得到新的静压分布,如此反复迭代,直至燃料状态不再变化,最终确定主动冷却燃烧室的各种传热与燃烧特性参数。利用该分析方法,初步开展了不同飞行马赫数条件下主动冷却燃烧室闭环运行状态研究,得到了冷却煤油温度与燃烧室壁温同飞行马赫数的关系。     

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.     

喷嘴位置对脉冲爆轰发动机性能影响的试验研究

为了研究喷嘴位置对脉冲爆轰发动机性能的影响,设计加工了直径为80mm的汽油/空气两相脉冲爆轰发动机（PDE）,在PDE文氏管内不同位置安装喷嘴,进行了冷态雾化和热态燃烧转爆轰试验,分析了马尔文激光粒度仪测得的液滴尺寸分布和动态压力传感器测得的信号。试验结果表明：喷嘴的安装位置对脉冲爆轰发动机的性能具有显著影响;喷嘴安装在文氏管喉部时爆轰管内雾化混合效果最好,爆轰波峰值压力最大为3．5 MPa,工作频率最高为30Hz;喷嘴安装在文氏管入口时爆轰管内雾化混合效果最差,爆轰波峰值压力最小为0．9MPa,工作频率最低为15 Hz;在试验范围内,改善雾化混合效果有利于提高脉冲爆轰发动机的工作频率。研究结果对脉冲爆轰发动机的设计具有参考价值。     

激波聚焦诱导气液两相爆震燃烧的数值模拟

对以激波聚焦和增加障碍物方式诱导煤油-空气气液两相爆震燃烧的过程进行了数值模拟.采用欧拉-拉格朗日方法建立了脉冲爆震发动机(PDE)中气液两相流的喷射、雾化、掺混过程.研究发现环形爆震波在爆震管凹腔内经过反射、汇聚后能够引燃可燃混合物.而在障碍物处,激波的反射和再反射聚焦能够形成高温高压点(2700K,25MPa),产生局部爆炸,有助于形成稳定的脉冲爆震燃烧(波面速度为1900m/s,温度为2 950K),有效地缩短由缓燃向爆震转变(DDT)距离至0.45m.     

脉冲随机微分系统的均方指数稳定性分析

研究了脉冲随机时滞微分泛函方程的均方指数稳定性问题。利用Lyapunov-Razumikhin型方法及随机分析的一些技巧,建立了一类脉冲随机泛函微分方程的均方指数稳定性定理。     

脉冲雷达凝视模式下低轨碎片相对运动特征分析

脉冲雷达凝视模式是一种探测低轨小碎片的重要方式,其中低轨碎片与雷达的径向运动关系是碎片统计分析的基础.为推算碎片相对雷达的运动特征,基于坐标系的相互转换,先利用雷达测站信息,得到可见碎片在地惯坐标系下的轨道信息;再逆向将目标不同时刻的位置转换至测站坐标系下,得到目标的径向运动特征.在不同要素（雷达波束指向、雷达仰角、测站纬度、目标距离）下,仿真及对比分析了各个参数对速度模糊度、雷达可见性等的影响,得出在凝视模式下目标相对雷达近似做径向匀加速运动,这为后续试验工作提供有力的依据.     

高原机场终端区飞行闭环稳定性分析

分析了高原机场终端区飞行的特殊性和影响高原机场飞行闭环稳定性的各种不利因素,指出了在高原机场缺氧条件下对飞行员数学模型修正的必要性和修正方法.采用等效闭环系统方法分析飞机在高原机场环境下的闭环稳定性,利用该思路可以用常规的分析方法研究高原机场飞行员缺氧条件下的闭环稳定性.     

重复率电光调Q Nd3+:YAG激光器输出能量及激光器效率的测定

本文提出了一种在不同的泵浦电压下测量重复率电光调Q掺钕钇铝石榴石激光器输出能量的方法 ,实际测量了脉冲激光器静态输出和动态输出能量 ,并利用电光晶体激光调Q技术得到脉宽为亚毫微秒的激光脉冲 ,使得激光器动态输出功率达兆瓦量级     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.