一种Ku频段全向高增益天线设计

提出了一种工作于Ku频段的宽频带、高增益和H面全向的新型共面波导（CPW）的中心导体和左右地板交叉连接耦合馈电天线结构设计。csTMws。软件仿真结果表明,该结构在具有较小尺寸的同时,能够有效展宽工作频带和提高增益,并保持天线的全向性。利用CSTMWS。软件对天线表面电流的仿真,解释了天线具有宽带和全向高增益辐射的原因：终端加载的三角形单极天线引起CPW中心带条的电流为行驻波电流,使天线获得了较宽的阻抗带宽;10个天线辐射单元的表面电流近似等幅同相,使天线获得了全向高增益的性能。研制出了工作在Ku频段的CPW交叉连接耦合馈电天线并进行了测试。天线印刷于厚度为0．5mm的FR-4环氧树脂板上,其反射系数低于-10dB时的频带为12．4～13．5GHz,相对带宽达8．5％,H面全向最大增益为6．6dBi,表明测试结果与仿真结果吻合较好。整个天线的尺寸仅为81mm×6．1mm,可应用于Ku频段的通信系统中。     

基于数值微分方法的卫星陀螺故障诊断(英文)

提出一种基于数值微分的卫星陀螺故障诊断方法。通过引入代数可观测的概念,将故障诊断问题转化为求解数值微分问题。并根据卫星姿态运动学方程证明了陀螺故障的代数可观性。然后通过高增益观测器的方法来近似姿态敏感器测量输出的数值导数,并利用李雅普诺夫理论分析和设计高增益观测器。基于陀螺故障的代数可观性和星敏感器测量输出的数值微分,可以直接得到陀螺组件的故障估计值。最后,通过突变、缓变和并发故障等仿真算例验证了算法的有效性,仿真结果表明所提出的方法不仅可以检测故障的发生,而且能够估计故障幅值。     

调频多普勒引信抗调幅干扰性能分析

为提高调频多普勒引信抗调幅干扰性能,定量研究了调幅干扰对其作用机理,以信干比(SJR)增益作为表征参量定量研究了不同调幅干扰作用下调频多普勒引信的抗干扰性能。详细推导了正弦波调幅、方波调幅和三角波调幅干扰作用下调频多普勒引信的信干比增益,并对其进行了仿真验证。定量分析、仿真与引信实验测试结果表明:在调幅干扰下调频多普勒引信总信干比增益在10 d B量级;调频多普勒引信抗各种调制样式调幅干扰能力相当,对调幅干扰调制样式不敏感;调幅指数对调频多普勒引信抗干扰性能基本无影响;减小多普勒滤波器带宽可以一定程度提高调频多普勒引信系统抗干扰性能。     

伞衣透气性对翼伞气动特性的影响

为了提高翼伞的飞行性能,需要研究伞衣织物透气性对翼伞气动特性的影响。使用不可压雷诺时均Navier-Stokes(RANS)方程模拟伞衣外部流场,建立了包含附加动量源项的多孔介质域控制方程模拟伞衣,对2种透气性材料模型和无透气性影响传统模型的气动特性和流场分布进行了二维和三维定常数值模拟。数值结果表明,求解多孔介质域控制方程可以得到较准确的伞衣透气速度,伞衣表面的湍流度急剧增加;使用较大透气量材料制作伞衣时,升力系数大幅下降,阻力系数大幅上升,同时会造成内腔泄压影响翼伞的外形保持;使用微透气量材料制作伞衣时,升力系数在小迎角时小于不透气模型,在大迎角时大于不透气模型,较小的透气速度能在大迎角时延缓边界层分离。     

带校正的机电集成超环面传动最优控制

基于某型机电集成超环面传动的机电耦合动力学模型,得到该传动的速度传递函数,推导了加入校正后系统的状态空间表达.考虑该系统的工程实际要求,建立了最优控制理论模型,求得了最优控制律.解得黎卡提矩阵方程,得到反馈增益矩阵,应用Matlab软件对跟踪响应情况和最优控制输入进行了仿真,明显改善了系统的动态性能,实现了比例积分(PI)控制与最优控制的结合.研究结果对该类型传动的实际应用具有指导意义.      

有限推力椭圆轨道近距离拦截方法

针对椭圆轨道近距离飞行器确定时间最小能量拦截问题,研究了有限推力一次机动作     

机载火控雷达在中远距空战中的抗干扰方法

根据机载火控雷达的性能特点,针对中远距空战面临的电子干扰环境,首先分析和探讨了机载火控雷达的抗干扰技术措施,给出了抗噪声干扰、距离欺骗干扰、速度欺骗干扰、角度欺骗干扰和消极干扰的一些具体方法。然后,从战术使用的角度探讨了机载火控雷达的抗干扰方法,提出了机载火控雷达与欺骗干扰协同、编队协同以及电子防护的战术抗干扰措施。     

Investigation of longitudinal aerodynamic parameters identification method for fly-by-wire passenger airliners

The flight control system of a fly-by-wire （FBW） passenger airliner with a complex frame-work and high feedback gain augmentation would change the original characteristic of a loaded signal and suppress the excitation of an airplane＇s pertinent motion modes. Taking a research example of an FBW passenger airliner model with longitudinal relaxed-static-stability, a new method of signal type selection and signal parameter design is proposed, through analysis of signal energy distribution and plane body＇s frequency response. According to CCAR60--the Appraisal and Use Regulation of Flight Simulator Device, the simulation validation of the FBW passenger airliner＇s longitudinal aerodynamic parameters identification is put forward. The validation result indicates that the designed signal could excite the longitudinal motion mode of the FBW passenger airliner adequately and the multiparameter comparison in simulation meets the objective test request of CCAR60. Meanwhile, the relative errors of aerodynamic parameters are less than 10%.     

光纤陀螺开环增益的实时估计与补偿

开环增益是影响闭环光纤陀螺控制稳定性及控制精度的重要参数。从光纤陀螺的数学模型出发推导了开环增益的计算公式。在数字闭环光纤陀螺相关检测的基础上提出了一种开环增益的估计方法,通过在积分控制环节前施加一个方波抖动信号,然后在信号处理器中进行相关解调,实现了开环增益的在线实时估计。同时利用数字逻辑中比例控制系数的可操作性,通过实时调整比例控制系数K来补偿硬件部分增益G的变化,从而实现陀螺开环增益的自补偿。最后通过实验证明了该方法的正确性。     

Possible physical properties of the flow in the vicinity of the heliopause

An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath.