A transient bulk flow model with circular whirl motion for rotordynamic coefficients of annular seals

Bulk flow model with perturbation simplification has been used to calculate rotordynamic coefficients in annular seals which have significant influences on the dynamic behavior of rotors in turbomachinery. In this work, a transient bulk flow model with arbitrary rotor motion is developed, and the boundary conditions and friction factor in the model are calibrated with steady Computational Fluid Dynamics (CFD) analysis. The numerical solution scheme is developed based on the finite element method to obtain the transient reaction force in the seal clearance. With a periodic circular rotor orbit, the transient forces at multiple whirling frequencies are used to evaluate the rotordynamic coefficients. The leakage flowrate of CFD analysis has good agreement with experimental results and the calibrated parameters in bulk flow model are dependent on operating conditions. Although CFD calibration improves the accuracy of the perturbed bulk flow model, the direct damping is overestimated and the cross-coupled damping is underestimated. Compared with the perturbed model, the predictions of the transient bulk flow model are more agreeable with the experiment.     

Interface flux reconstruction method based on optimized weight essentially non-oscillatory scheme

Aimed at the computational aeroacoustics multi-scale problem of complex configurations discretized with multi-size mesh, the flux reconstruction method based on modified Weight Essentially Non-Oscillatory (WENO) scheme is proposed at the interfaces of multi-block grids. With the idea of Dispersion-Relation-Preserving (DRP) scheme, different weight coefficients are obtained by optimization, so that it is in WENO schemes with various characteristics of dispersion and dissipation. On the basis, hybrid flux vector splitting method is utilized to intelligently judge the amplitude of the gap between grid interfaces. After the simulation and analysis of 1D convection equation with different initial conditions, modified WENO scheme is proved to be able to independently distinguish the gap amplitude and generate corresponding dissipation according to the grid resolution. Using the idea of flux reconstruction at grid interfaces, modified WENO scheme with increasing dissipation is applied at grid points, while DRP scheme with low dispersion and dissipation is applied at the inner part of grids. Moreover, Gauss impulse spread and periodic point sound source flow among three cylinders with multi-scale grids are carried out. The results show that the flux reconstruction method at grid interfaces is capable of dealing with Computational AeroAcoustics (CAA) multi-scale problems.     

Super-resolution reconstruction of astronomical images using time-scale adaptive normalized convolution

In this work, we describe a new multiframe Super-Resolution (SR) framework based on time-scale adaptive Normalized Convolution (NC), and apply it to astronomical images. The method mainly uses the conceptual basis of NC where each neighborhood of a signal is expressed in terms of the corresponding subspace expanded by the chosen polynomial basis function. Instead of the conventional NC, the introduced spatially adaptive filtering kernel is utilized as the applicability function of shape-adaptive NC, which fits the local image structure information including shape and orientation. This makes it possible to obtain image patches with the same modality, which are collected for polynomial expansion to maximize the signal-to-noise ratio and suppress aliasing artifacts across lines and edges. The robust signal certainty takes the confidence value at each point into account before a local polynomial expansion to minimize the influence of outliers. Finally, the temporal scale applicability is considered to omit accurate motion estimation since it is easy to result in annoying registration errors in real astronomical applications. Excellent SR reconstruction capability of the time-scale adaptive NC is demonstrated through fundamental experiments on both synthetic images and real astronomical images when compared with other SR reconstruction methods.     

弹道反舰导弹靶场飞行试验安全分析

反舰导弹靶场飞行试验中,为了确保试验方案可实施,必须进行试验安全性量化分析,以确保故障弹对保护目标的威胁概率最小。根据弹道反舰导弹特点,给出量化分析基本思路,归纳导弹故障模式,分析不同故障模式下导弹落点散布,并给出量化分析计算方法。通过实例,验证计算方法的正确性和科学性。     

光纤陀螺本征频率对准误差引起的零偏漂移抑制方法

在温度环境下,光纤环的伸缩及光折射率的变化等会引起光纤陀螺本征频率发生变化,产生光纤陀螺本征频率与陀螺调制频率对准误差,进而导致探测器信号中的“尖峰脉冲”信号发生变化,使光纤陀螺产生零偏漂移。通过分析光纤陀螺本征频率的变化,提出了一种调制频率自动跟踪本征频率的方法,从而减小了温度条件下光纤陀螺的零偏漂移。试验验证结果表明,采用该方法的光纤陀螺在-40℃～+60℃的温度范围内固定温度点下的零偏极差减小了50%。     

谐振式光子晶体光纤陀螺信号检测及处理技术研究

谐振式光子晶体光纤陀螺是一种具有小型化、高精度等潜在技术优势的新型光纤陀螺,是国内外惯性器件研究的一个重要发展方向。针对谐振式光子晶体光纤陀螺的结构和信号检测原理进行了详细的叙述,确定了基于FPGA的陀螺信号检测总体方案,陀螺信号处理及控制模块主要由频差信号解调、复合拍频检测、闭环反馈控制、数据编码输出以及调制信号模块组成;随后重点介绍了窄线宽半导体激光器的驱动控制方案,在调制解调及频率偏差检测方案上采用数字相敏检波器实现频率偏差检测,在谐振频率闭环跟踪锁定方案上采用数字PI控制器实现环路光频率控制;最后进行了谐振式光子晶体光纤陀螺实验测试系统搭建,以及谐振曲线测试和谐振频率闭环锁定测试。     

R-T-S平滑算法与抗差Kalman在数据后处理中的应用

为了提高组合导航系统后处理精度和数据稳定性,将R-T-S最优固定区间平滑算法引入数据后处理中,在前向Kalman滤波的基础上,进行了后向R-T-S最优固定区间平滑处理,并针对GPS观测值中存在异常的问题,将抗差Kalman滤波算法引入数据后处理中,并对该算法进行实物仿真。结果表明,与传统Kalman滤波相比,R-T-S平滑算法不仅可以提高位置、姿态精度,而且在卫星信号失锁的情况下精度也得到显著改善,并且在不丢星的时刻,抗差Kalman滤波可以有效处理GPS信号中的异常观测值,遏制滤波发散,是一种有效的数据处理方法。     

电力机车PMSM自适应模糊滑模控制

为研究牵引工况下电力机车永磁同步电机(PMSM)的转速控制精度,考虑轮轨接触不平顺及车体静载荷在轮对径向产生的未知时变负载转矩,建立了机车PMSM在dq坐标系下的数学模型。针对该耦合非线性系统中存在的负载转矩,设计非线性转矩观测器对其实际值进行估计,对观测误差采用自适应模糊逻辑系统进行逼近;为考察d轴电压过零跳变对转速控制及转矩观测性能的影响,在d轴电压控制器设计中引入Nussbaum函数,并依据Lyapunov稳定性理论,构造了基于转矩观测器的自适应模糊滑模控制器。理论分析及仿真结果表明,当转矩时变或d轴电压过零时,机车PMSM闭环转速控制系统跟踪误差一致有界,转矩观测误差收敛于0。     

主动冷却通道内正庚烷热裂解与换热过程的数值模拟 *

为了深入研究碳氢燃料在主动冷却通道中的传热特性,采用详细基元反应机理对微小通道内正庚烷热解反应耦合流动换热过程进行了数值模拟。根据燃料的热裂解反应和壁面传热特性可将通道分为三个换热区域。通过对不同的入口温度、运行压力、壁面温度和通道直径等典型工况进行模拟,探索了正庚烷的热裂解反应和流动换热过程耦合的基本规律。研究结果表明,入口温度对通道整体的换热性能影响不大;保持其它参数不变,通道直径从2mm减小到0.5mm,其整体换热量降低约10%,单位面积的换热量提升约4倍。     

水分解微推力器脉冲燃烧过程实验研究

水分解推进系统是一种特别适用于微小卫星应用需求的技术方案,其性能与推力器燃烧过程和工作时序的匹配密切相关。为了优化设计、提高性能,使用快速响应的压力传感器对水分解推力器燃烧室内的定容预混燃烧过程进行了测量。典型信号显示,典型燃烧过程包括缓燃、爆燃及爆燃波反射、未烧完气体缓燃、燃气冷却及吸附等五个阶段。在氢氧混合气体的初始压力从30k Pa逐渐升高到90k Pa时,爆燃导致的压力最大值出现的时间从355μs缩短到172.5μs,爆燃强度逐渐增大,缓燃完成的时间基本不变,缓燃导致的最大压力逐渐增大,但是明显低于绝热定容燃烧,燃烧过程受散热和表面吸附的影响显著。燃烧和冷却的特征时间均为毫秒量级,推力器的排气时间精度应优于亚毫秒量级,以保证工作时序与燃烧及冷却吸附过程相匹配。