“T”型尾翼飞机的深失速特性研究

应用时间历程法讨论了“Ｔ”型尾翼飞机的深失速开环特性，分析了气动力矩特性和升降舵操纵规律对深失速改出特性的影响。建立了深失速闭环特性计算数学模型，分析了驾驶员数学模型参数变化对深失速特性的影响。研究结果表明，气动力矩特性，升降舵操纵规律和驾驶员模型参数的变化对“Ｔ”型尾翼飞机的深失速改出特性有显著的影响。     

雨流计数法及其在程序中的具体实现

根据雨流计数法的规则和在实际中应用的体会，介绍了雨流计数法在程序中实现的具体方法。它适合用各种语言编写，在计取循环数时采用的“四点法”使程序的实现比用其他方法更加准确可靠，简单明了。     

旋转同心双轴间流动的热态实验

某型发动机高、低压涡轮轴间环形气流通内的流动可以简化为两个独立旋转同心双轴环道内的流动问题。对其控制方程以及边界条件进行无量纲化，得出了实验准则，设计并建立了实验台，以实验方法研究了具有轴向通流的独立旋转同心双轴环道内的流动规律。结果表明，随着冷气雷诺数增大，阻力系数总体趋势减小；冷气雷诺数的影响远大于内轴和外轴旋转对流动的影响。     

一种低噪声和高精度的频率合成技术

介绍了锁相环(PLL)技术和直接数字式频率合成(DDS)技术的基本工作原理,给出了一种提高DDS输出频率精度及减小其相位截断误差的方法。     

卫星用两种单相流体回路方案对比研究

单相流体回路系统是航天器主动热控技术中的一种重要方式。文章概述了流体回路的工作原理及理论基础，总结了单相流体回路的设计思路，结合某卫星型号，设计了两种流体回路方案，在SINDA／FLUINT中建立数值仿真模型进行分析计算，并比较了两种方案的应用性能。结果显示，将单相流体回路系统应用于卫星，可取得较好的控温效果。     

烧结双多孔介质中沸腾换热的实验研究

对由铜粉烧结而成的三种双多孔介质结构进行了沸腾换热的实验。为了便于比较，同时对两种单多孔介质进行了沸腾换热实验。结果发现：当双多孔介质的微孔径和单多孔介质的孔径相同时，双多孔介质的换热系数和临界热流密度比单多孔介质高得多；对于同样微孔径的双多孔介质，存在最佳的粗孔径，其换热系数和临界热流密度最大；当逆静水压头减小的时候，换热系数和临界热流密度增加。     

可展开式辐射器热控对航天器轨道调整的适应性分析

为提高航天器热控系统对轨道调整的适应能力，本文研究了与流体回路耦合的可展开式辐射器热控方案在不同轨道高度下的热控性能，分析了不同轨道高度时辐射器面临的热环境的影响，在不同轨道高度下比较了固定辐射器与可展开辐射器的热控特性。结果表明，随着辐射器展开角度的变化，辐射器吸收的空间热流随之发生变化，从而对热控系统的散热能力带来直接影响，调节辐射器的角度可以扩大其对外散热能力。在工程应用中，基于热控流体回路，通过调节可展开式辐射器的展开角度，可以有效提高航天器的轨道热适应能力。     

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.     

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.     

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.