一种基于EPLL技术的自适应正交解调技术研究

针对过零检测实现的全数字锁相环不仅锁相速度慢, 而且过零点的扰动会 直接影响锁相精度以及适合模拟电路实现的相干解调技术,在数字电路中实现则需要设 计高阶数字低通滤波器,将占用大量数字电路资源并且会显著增加系统功耗等问题,在 设计一种新型全数字锁相环(All-digital Enhanced Phase-lock Loop,EPLL)的基础上,结合自 适应正交解调技术,提出了一种基于EPLL 技术的自适应正交解调技术方案,并对该方 案进行了研究与仿真。仿真得到了满意的结果,验证了基于EPLL 技术的自适应正交解 调技术方案的可行性,并研究验证了算法的参数变化对其性能的影响,为今后算法在数 字系统中的实现以及其在各领域的应用研究奠定了坚实的基础。     

飞机机翼着陆滑跑动态性能分析

飞机着陆滑跑过程中,机翼结构将受到较大的冲击作用和振动激励。为预判结构局部危险部位,给结构强度设计提供参考,需对机翼着陆滑跑过程中的动态性能进行分析。创新性地考虑了飞机滑跑速度和气动力的变化,为有限元计算提供可靠的外载输入,并合理设置约束条件,建立半机体有限元模型,降低计算规模。最后提取机翼各站位处的载荷响应峰值,做出动响应包线,预判结构局部危险部位,如机翼根部,为结构强度设计提供参考。     

带升力风扇飞翼布局开口机翼气动特性研究

为获得带升力风扇飞翼布局飞机因开口对机翼气动特性的影响规律,对平飞状态下开口机翼的气动特性进行三维气动仿真,分析升力系数、阻力系数和力矩系数随来流速度和迎角变化的特性.结果表明:随着来流速度增大,阻力和力矩呈上升趋势;来流速度一定时,随着迎角加大,升力系数增大,阻力系数先减小后增大;随着迎角增大,力矩系数先减小后增大再减小,且一直产生低头力矩.     

相控阵超声检测技术在某型飞机撑杆焊缝检测中的试验研究

焊缝是飞机起落架承受交变应力和冲击力较多的部位,常常是疲劳裂纹的多发部位.根据起落架焊缝损伤特点,在比较多种检测方法的基础上,确定了相控阵超声检测方法,制作了与检测件完全一致的对比试块.经建模与试验,相控阵超声检测可以有效地检测焊缝疲劳裂纹,根据试验过程提出了在实践检测中需要解决的问题.     

梯形翼风洞试验模型数值模拟技术

基于雷诺平均Navier-Stokes (RANS)方程和结构网格技术,采用二阶空间离散精度的MUSCL格式,并结合k-ω剪切应力输运(SST)两方程湍流模型和γ-Re_θ转捩模型,研究了梯形翼风洞试验模型中前缘缝翼、后缘襟翼连接装置对气动特性的影响。简要介绍了本文采用的计算方法;介绍了梯形翼的风洞试验模型及风洞试验结果;在网格收敛性研究的基础上,采用"全湍流"方式和转捩模型研究了梯形翼试验模型连接装置对气动特性的影响。通过与不带连接装置的计算结果的对比,采用"全湍流"模拟方式,计算模型中考虑试验模型的连接装置引起升力系数下降、阻力系数下降、低头力矩减小以及失速迎角提前;通过与试验数据的对比,进一步考虑转捩影响可以提高梯形翼风洞试验模型气动特性的计算结果与试验结果的吻合程度,梯形翼风洞试验模型失速迎角附近的气动特性数值模拟技术还需要进一步的研究。     

基于矩阵填充的二维自适应波束形成算法

针对基于矩阵填充的二维自适应波束形成问题,提出一种基于奇异值门限(SVT)的特征分解线性约束最小方差(SVT-ELCMV)算法。首先建立二维自适应波束形成矩阵填充模型,其次验证接收信号矩阵满足零空间性质(NSP),并分析最小可恢复阵元数,最后以SVT算法将稀疏阵列信号恢复为完整信号,并通过修正的特征分解线性约束最小方差(LCMV)形成有效波束。算法解决了稀疏阵列平均副瓣大幅度上升的缺陷,且在平面阵列部分阵元无法正常工作时依然有效。计算机仿真表明:SVT-ELCMV算法可使稀疏阵列具有与完整阵列相同的二维波束形成能力,并可有效抑制干扰信号,验证了算法的有效性和优越性。     

充气机翼的褶皱与失效行为研究

在经典工程梁理论的基础上,结合张力薄膜的应力状态分析,提出充气机翼褶皱失稳的判据。计入表面薄膜褶皱引起的刚度退化效应,将机翼等效处理为一个变截面刚度的梁,建立了充气悬臂机翼的等效梁模型,并采用微分求积法进行充气机翼弯曲变形分析。计算结果与充气机翼的静力弯曲试验结果相吻合,验证了充气机翼弯曲变形分析方法的有效性。应用片条理论引入气动力模型,并与所建立的等效梁模型相耦合,建立充气机翼的静气动弹性耦合模型,并用迭代算法进行求解。考虑起皱和失稳两种判据,并计算获取了试验机翼的起皱动压和皱褶失稳动压形式,计算结果与风洞试验结果一致。根据所建立的充气机翼静气动弹性分析方法,可以预测充气机翼表面褶皱区的扩展和弯曲变形,进而绘制充气机翼的静气弹许用包线,为充气机翼的设计提供必要的安全边界参考依据。     

扩展酉矩阵束算法实现稀疏可重构天线阵的优化设计

针对方向图可重构天线阵列的稀疏布阵问题,提出一种基于扩展酉矩阵束算法的优化设计算法。首先建立以阵元位置和多组激励为变量的多方向图联合稀疏优化模型,并利用期望方向图采样数据构建Hankel块矩阵。然后通过centro-Hermitian化处理和酉变换将采样矩阵从复数域转换到实数域,舍弃实矩阵中较小的奇异值对可重构线阵进行稀疏。最后通过对等价矩阵束的广义特征值分解估计稀布阵元位置,进而得到每个方向图对应的激励。仿真验证了该方法能够以阵元非均匀稀疏分布的阵列形式有效实现多个方向图的精确重构。     

Streamwise-body-force-model for rapid simulation combining internal and external flow fields

A streamwise-body-force-model (SBFM) is developed and applied in the overall flow simulation for the distributed propulsion system, combining internal and external flow fields. In view of axial stage effects, fan or compressor effects could be simplified as body forces along the streamline. These body forces which are functions of local parameters could be added as source terms in Navier-Stokes equations to replace solid boundary conditions of blades and hubs. The val-idation of SBFM with uniform inlet and distortion inlet of compressors shows that pressure perfor-mance characteristics agree well with experimental data. A three-dimensional simulation of the integration configuration, via a blended wing body aircraft with a distributed propulsion system using the SBFM, has been completed. Lift coefficient and drag coefficient agree well with wind tun-nel test results. Results show that to reach the goal of rapid integrated simulation combining inter-nal and external flow fields, the computational fluid dynamics method based on SBFM is reasonable.     

Modelling of galactic Carbon in an asymmetrical heliosphere: Effects of asymmetrical modulation conditions

Observations of galactic cosmic rays (GCRs) from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that in addition to a possible global asymmetry in the north–south dimensions (meridional plane) of the heliosphere, it is also possible that different modulation (turbulence) conditions could exist between the two hemispheres of the heliosphere. We focus on illustrating the effects on GCR Carbon of asymmetrical modulation conditions combined with a heliosheath thickness that has a significant dependence on heliolatitude. To reflect different modulation conditions between the two heliospheric hemispheres in our numerical model, the enhancement of both polar and radial perpendicular diffusion off the ecliptic plane is assumed to differ from heliographic pole to pole. The computed radial GCR intensities at polar angles of 55° (approximating the Voyager 1 direction) and 125° (approximating the Voyager 2 direction) are compared at different energies and for both particle drift cycles. This is done in the context of illustrating how different values of the enhancement of both polar and radial perpendicular diffusion between the two hemispheres contribute to causing differences in radial intensities during solar minimum and moderate maximum conditions. We find that in the A > 0 cycle these differences between 55° and 125° change both quantitatively and qualitatively for the assumed asymmetrical modulation condition as reflected by polar diffusion, while in the A < 0 cycle, minute quantitative differences are obtained. However, when both polar and radial perpendicular diffusion have significant latitude dependences, major differences in radial intensities between the two polar angles are obtained in both polarity cycles. Furthermore, significant differences in radial intensity gradients obtained in the heliosheath at lower energies may suggest that the solar wind turbulence at and beyond the solar wind termination shock must have a larger latitudinal dependence.