电脉冲除冰系统电磁脉冲力仿真分析

为了获得更精确的电脉冲除冰(EIDI)系统中电磁力在飞机蒙皮上的分布及其随时间变化的情况,针对系统的工作原理与工作过程进行了仿真研究。计算分析了EIDI系统电路中电流随时间变化的关系;通过麦克斯韦方程组的求解完成了EIDI系统电磁场的仿真;计算分析了电磁力随时间变化的规律,获得了蒙皮上的磁感应强度分布、涡电流密度分布和瞬态电磁力密度分布。考虑线圈工作时蒙皮对其电感的影响,建立了更接近真实电路的激励加载方法,得到了准确的电磁力变化趋势;考虑趋肤效应对蒙皮厚度方向上涡电流密度、电磁力密度分布的影响,用有限元分析方法使蒙皮上电磁力分布的计算更为全面合理。      

基于自适应阈值的粒子滤波非线性系统故障诊断

针对实际非线性系统传统方法难以实现可靠故障诊断的问题,采用粒子滤波算法,利用对数似然函数和作为评价指标,并借助自适应阈值的设计,研究了非线性非高斯系统的故障检测和故障隔离。阈值的选取,是准确判别系统是否发生故障的标准,本文通过分析非线性系统残差的统计特性,在判定残差统计特性成正态分布的基础上,设计了一种基于粒子滤波故障诊断的自适应阈值方法,减少了故障诊断的漏报和误报。通过非恒温连续搅拌水箱式反应堆的仿真实例,验证了该方法在故障诊断中的准确性和有效性。      

基于权值分配及多特征表示的在线多示例学习跟踪

针对复杂环境下目标跟踪过程中由于遮挡、目标姿势及光照条件变化引起跟踪漂移的问题,提出一种基于多示例学习（MIL）框架的在线视觉目标跟踪算法。该算法针对多示例跟踪算法采用单一haar-like特征不能准确描述目标外观变化及在学习过程中对样本包中各正负样本示例采用相同权值,忽略不同正负样本示例在学习过程中对包的重要性不同的特点,采用多特征联合表示目标外观构造分类器,通过将多特征互补特性融入在线多示例学习过程中,利用多特征的互补属性建立准确的目标外观模型,克服在线多示例跟踪算法对目标外观变化描述不足的问题;同时,依据不同正负样本示例对样本包的重要程度进行权值分配,提高跟踪精度。实验结果表明,本文跟踪算法对场景光线剧烈变化、遮挡、尺度变化及平面旋转等干扰具有较强的跟踪鲁棒性,通过对不同视频序列进行测试,文中算法在5组测试视频序列上的平均中心位置误差远小于对比增量式学习跟踪,仅为10.14像素,其对比算法IVT、MIL和OAB的中心位置误差分别为17.99、20.29和33.64像素。      

Weibull分布参数估计值对细节疲劳额定强度的影响

将新材料、新工艺应用于民机结构设计时,细节疲劳额定强度（DFR）法仍是重要的评估方法。根据新型铝合金疲劳试验数据,全面分析了Weibull分布形状参数对DFR计算参数的影响;分析标准S-N曲线斜度参数对DFR的影响时,应考虑可靠性寿命的变化,采用低可靠度寿命计算曲线斜度参数可降低Weibull分布形状参数的影响;比较了采用不同分布参数估计值与传统上采用波音公司给定值进行DFR计算的差异。结果表明,对于通过符合性检验的试验数据,使用不同Weibull分布的参数估计值计算得到的DFR都大于按传统方法（用波音公司给定值）的计算结果,其中,三参数Weibull分布计算的DFR最大,至少增加10%以上。     

考虑喷注流强分布的纵向稳定性建模与分析

喷注器流强分布是除声学阻尼装置以外使液体火箭发动机稳定工作的重要措施,通过控制喷注流强分布使推进剂的燃烧尽量远离主要振型的波腹区,减少热声耦合振荡的能量源,从而达到抑制高频振荡的效果。因此,建立喷注流强分布与稳定性之间的综合分析模型,研究流强分布的不稳定性抑制特性具有重要实际意义。针对采用自击式喷嘴器、液滴蒸发作为燃烧速率控制过程的某自燃推进剂缩尺燃烧室高频纵向燃烧不稳定问题,近似采用蒸发速率峰值区代替集中燃烧释热区,引入燃烧室三维声学控制方程以考虑多喷嘴条件下燃烧响应空间分布,建立了针对喷注器流强分布条件下的高频纵向燃烧稳定性分析模型,并对喷注流强的稳定性抑制特性进行了分析,给出了不同分布流强下燃烧室一阶纵向信号的增长率变化规律。研究表明,喷注流强分布有利于燃烧室稳定,"驼峰区"喷注孔径的增大对改善高频纵向不稳定性更为显著,"驼峰区"流强增加30%,相应的增长率降低15%。     

Form-finding methods for deployable mesh reflector antennas

Deployable high-frequency mesh reflector antennas for future communications and obser- vations are required to obtain high gain and high directivity. In order to support these new missions, reflectors with high surface accuracy are widely required. The form-finding analysis of deployable mesh reflector antennas becomes more vital which aims to determine the initial surface profile formed by the equilibrium prestress distribution in cables to satisfy the surface accuracy requirement. In this paper, two form-finding methods for mesh reflector antennas, both of which include two steps, are pro- posed. The first step is to investigate the prestress design only for the cable net structure as the circum- ferential nodes connected to the supporting truss are assumed fixed. The second step is to optimize the prestress distribution of the boundary cables connected directly to the supporting truss considering the elastic deformation of the antenna structure. Some numerical examples are carried out and the simulation results demonstrate the proposed form-finding methods can warrant the deformed antenna reflector surface matches the one by design and the cable tension forces fall in a specified range.     

Design of face-hobbed spiral bevel gears with reduced maximum tooth contact pressure and transmission errors

The aim of this study is to define optimal tooth modifications, introduced by appropriately chosen head-cutter geometry and machine tool setting, to simultaneously minimize tooth contact pressure and angular displacement error of the driven gear (transmission error) of face-hobbed spiral bevel gears. As a result of these modifications, the gear pair becomes mismatched, and a point contact replaces the theoretical line contact. In the applied loaded tooth contact analysis it is assumed that the point contact under load is spreading over a surface along the whole or part of the ’’potential’’ contact line. A computer program was developed to implement the formulation provided above. By using this program the influence of tooth modifications introduced by the variation in machine tool settings and in head cutter data on load and pressure distributions, transmission errors, and fillet stresses is investigated and discussed. The correlation between the ease-off obtained by pinion tooth modifications and the corresponding tooth contact pressure distribution is investigated and the obtained results are presented.     

磁层中重离子O＋通量密度分布的理论研究

应用求解得到的分布函数，研究了北半球子午面内极光带区起源的重离子Ｏ＋在磁层中的通量密度定态分布及其特性．结果表明：（１）重离子Ｏ＋通量密度分布沿ＧＳＭＺ轴方向呈峰状结构，其峰值随地心距离增大而减小，在近地空间减小较快；（２）磁扰动时，Ｏ＋离子占据的空间范围较磁宁静时大，通量峰较不突出；（３）理论估算的磁尾等离子体片边界层附近重离子Ｏ＋通量密度与观测结果相一致．     

Improved interpretation of solar wind ion measurements via high-resolution magnetic field data

The Wind   spacecraft’s Faraday cups (FC) continue to produce high-quality, in situ observations of thermal protons (i.e., ionized hydrogen) and α$\alpha$-particles (i.e., fully ionized helium) in the solar wind. By fitting a Wind/FC ion spectrum with a model velocity distribution function (VDF) for each particle species, values for density, bulk velocity, and temperature can be inferred. Incorporating measurements of the background magnetic field from the Wind Magnetic Field Investigation (MFI) allows perpendicular and parallel temperature components to be separated. Prior implementations of this analysis averaged the higher-cadence Wind/MFI measurements to match that of the Wind/FC ion spectra. However, this article summarizes recent and extensive revisions to the analysis software that, among other things, eliminate such averaging and thereby account for variations in the direction of the magnetic field over the time taken to measure the ions. A statistical comparison reveals that the old version consistently underestimates the temperature anisotropy of ion VDF’s: averaging over fluctuations in the magnetic field essentially blurs the perpendicular and parallel temperature components, which makes the plasma seem artificially more isotropic. The new version not only provides a more accurate dataset of ion parameters (which is well suited to the study of microkinetic phenomena), it also demonstrates a novel technique for jointly processing particle and field data. Such methods are crucial to heliophysics as wave-particle interactions are increasingly seen as playing an important role in the dynamics of the solar wind and similar space plasmas.     

静止轨道卫星在轨温度参数变化规律研究

分析了静止轨道在轨三轴稳定卫星各面上温度参数的变化规律,并通过理论计算得到卫星各面上光强的变化曲线,研究了温度参数变化与对应面上光强的关系,建立了温度参数与光线的线性模型,结果表明模型与实际数据能较好地吻合,对温度参数的预测以及故障的判断具有一定的参考价值.