薄板声——超声检测信号的时频分析研究

本文以兰姆波的群速度-频厚积频散曲线为基础,采用基于短时傅立叶变换的时-频分析方法,对薄板中传播的声-超声信号进行了处理分析。对厚度为2 mm薄钢板的声-超声检测实验结果证实,在声-超声检测形式下激发的超声波的主要成分是多模式的兰姆波。与现有文献中介绍的基于时间域识别的薄板声-超声信号分析方法相比,时-频分析方法不仅可以很好地识别兰姆波模式,而且可对各模式波的能量成分进行分析。     

一种紧凑型高效率毫米波整流天线

为了提高毫米波无线输能系统的接收端效率,设计了一款基于缝隙耦合馈电的紧凑型高效率毫米波整流天线,该整流天线通过划分子阵,每个子阵单独进行能量转换,采用直流合成的方式进行整合输出,具有尺寸小、剖面低、易共形等特点。天线采用缝隙耦合馈电,馈线和辐射贴片分别在地板的两侧,有效的减少天线电路之间的影响,同时增大了天线的有效辐射面积。后端整流电路采用单二极管并联整流拓扑,利用扇形枝节作为直通滤波器进行直流滤波。该整流天线工作频率为35GHz,天线阵列增益为23.4dBi,实测在17dBm接收功率下具有最高58.65%的整流效率,可广泛应用于毫米波无线输能系统中。     

天基低轨空间监视雷达密集短弧观测数据的定轨应用研究

当天基雷达采用多波束扫描时,每次与空间目标交会可获取类似跟踪的观测数据。本文讨论了这些密集短弧观测数据在目标轨道改进中的应用。在没有测量时,采用矩阵Ricatti方程计算状态误差;引入观测数据时,比较了EKF和UKF两种滤波算法的轨道改进效果。仿真表明,UKF的收敛速度优于EKF;天基短弧观测数据可以很好地抑制误差发散,满足监视任务需求。     

斜爆轰发动机燃烧机理试验研究

为了研究斜爆轰发动机的稳定燃烧机理,开展了飞行马赫数9的斜爆轰发动机的数值模拟研究和试验研究.设计了全尺度斜爆轰发动机模型,发动机的总长度为2.8m.采用两级进气道压缩,每级压缩角度均为15°.利用三个小支板在进气道前缘主流核心区中进行氢气的喷射和混合.采用带化学反应的雷诺平均N-S方程、SST k-ω模型以及9组分1...     

阻尼陀螺系统动力响应的有限元复模态分析方法

采用复模态分析方法研究了陀螺系统及具有粘性阻尼的陀螺系统的动力响应及其数值分析方法,提出了陀螺模态阻尼比的概念,实现了利用有限元结构分析软件对诸如薄壁旋转轴和转动薄壁壳体等各类形式的复杂旋转薄壁结构进行动力特性分析的目的,讨论了不同条件(单点旋转简谐激励和沿圆周呈周波型分布的激励)条件下转动薄壁壳体结构的行波振动特点.      

Strong interactions of incident shock wave with boundary layer along compression corner

The coherent structure and instability of the interaction of incident shock wave with boundary layer developing on a compression corner are experimentally studied. The experiments are carried out in a supersonic wind tunnel of Mach number 2. Particular attention is paid to shock patterns and unsteady shock motions induced by the separation bubble. The high-speed schlieren is used to visualize the flowfield evolution and to characterize the instability. The snapshot proper orthogonal decomposition of schlieren sequences is applied to investigate the primary coherent structure in the flowfield. Fast Fourier transform and continuous wavelet transformation are applied to characterize the instability. The results show that there are large-scale low-frequency oscillations of the shock waves and small-scale high-frequency pulsations in the separation region. The peak frequency of shock oscillation is mainly concentrated in the range of 100–1000 Hz. The pulsation of the small flow structure in the separation bubble is mainly concentrated above 12.5 kHz. Based on the results of experimental analysis, the preliminary mechanism of the large-scale instability of such interaction is obtained.     

On the occurrence and strength of multi-frequency multi-GNSS Ionospheric Scintillations in Indian sector during declining phase of solar cycle 24

This study presents unique perspectives of occurrence and strength of low latitude ionospheric scintillations on multiple signals of Global Navigation Satellite System (GNSS) and its frequency dependence using continuous observation records of 780 nights. A robust comparative analysis is performed using scintillation index, S4 and its variation during pre-midnight and post-midnight duration from a GNSS receiver located at Waltair (17.7°N, 83.3°E), India, covering period from July 2014 to August 2016. The results, generally exhibit the impact of declining phase of solar cycle 24 on occurrence and strength of scintillations, which, however, is evidently different over different frequencies transmitted from different GNSS systems. A deeper quantitative analysis uniquely reveals that apart from the solar cycle and seasonal effects, the number of visible satellites of a selected GNSS markedly affect the occurrence and also the strength. Processing scheme of adopting 6 hourly time windows of pre-midnight and post-midnight brought a novel result that the strength and occurrence of strong scintillations decrease with declining solar activity during pre-midnight hours but remarkably increase for moderate and weak scintillations during post-midnight. The physical processes that dominate the post-midnight equatorial ionosphere are invoked to explain such variations that are special during declining solar activity. Finally, inter-GNSS signal analysis in terms of the effect of strong, moderate and weak scintillations is presented with due consideration of number of satellite passes affected and frequency dependence of mean S4. The quantitative results of this study emphasize for the first time effect of low latitude scintillation on GNSS signals in Indian zone under changing background solar and seasonal conditions.     

美国天基靶场的开发

目前美国正在积极研究天基靶场并计划从地基靶场向天基靶场升级,这是美国靶场发展规划的一个重要目标。本文对美国天基靶场概念进行了分析,并与今天基于雷达的地基靶场进行了比较,最后介绍了美国实施天基靶场的一些演示实验方案。     

Oblique sounding of the ionosphere by powerful wave beams

The article is devoted to modeling the impact on the ionosphere powerful obliquely incident wave beam. The basis of this analysis will be orbital variational principle for the intense wave beams-generalization of Fermat’s principle to the case of a nonlinear medium (, ,  and ). Under the influence of a powerful wave beam appears manageable the additional stratification of the ionospheric layer F2. Explicit expressions show how the properties of the test beam, with a shifted frequency, released in the same direction as the beam depend on the intensity of a powerful beam and the frequency shift.