Wave propagation analysis for a second strain gradient rod theory

In this work, an enriched model describing the longitudinal wave propagation is established based on Mindlin’s Second Strain Gradient (SSG) theory, which can describe the heterogeneity caused by the micro-structure interactions in the frame of continuum mechanics. The governing equation and associated boundary conditions are derived based on Hamilton's principle, then the dispersion relation of non-classical longitudinal wave together with the extra-waves appearing exclusively in SSG theory model are investigated. The investigations are based on the modal density, energy flow, and forced response of the rod. Wave transmission and reflection through planar interfaces based on the proposed model have been calculated. Finally, the results of the enriched model are well interpreted by comparing with the classical theory results, and some useful conclusions are derived on the SSG theory based model in the wave propagation characterization.     

基于边缘电流法近远场变换中的探头补偿

针对目前平面近远场变换中，探头H面方向图对天线远区副瓣引入误差较大的情况，研究了一种基于边缘电流法近远场变换的探头补偿。通过在微波暗室对某频段阵列天线测量，并分别用传统使用的stratton-chu积分法、E面电场法与边缘电流法进行近远场变换并进行比较。结果表明，此方法相比传统方法，副瓣精度基本接近国际先进水平，远远高于国内现有水平，证明了该方法的有效性和工程实用性，并填补了国内空白。     

Spatio-temporal structure of the wave packets generated by the solar terminator

Using long-term (1998--2009) total electron content (TEC) measurements from the GPS global network including dense network of GPS sites in USA and Japan, we have obtained the first data regarding the spatio-temporal structure and the statistics of medium-scale traveling wave packets (MS TWPs) excited by the solar terminator (ST). Total amount of the detected TWPs exceeds 565,000. There is no correlation between TWPs occurrence and geomagnetic and solar activity. We found that the diurnal, seasonal and spectral MS TWPs characteristics are specified by the solar terminator (ST) dynamics. MS TWPs are the chains of narrow-band TEC oscillations with single packet’s duration of about 1–2 h and oscillation periods of 10–20 min. The total duration of chain is about 4–6 h. The MS TWPs spatial structure is characterized by a high degree of anisotropy and coherence at the distance of more than 10 wavelengths. Occurrence rate of daytime MS TWPs is high in winter and during equinoxes. Occurrence rate of nighttime MS TWPs has its peak in summer. These features are consistent with previous MS travelling ionosphere disturbance (TID) statistics obtained from 630-nm airglow imaging observations in Japan. In winter, MS TWPs in the northern hemisphere are observed 3–4 h after the morning ST passage. In summer, MS TWPs are detected 1.5–2 h before the evening ST appearance at the point of observations, but at the moment of the evening ST passage in the magneto-conjugate point. The obtained results are the first experimental evidence for the hypothesis of the ST-generated ion sound waves.     

Estimated errors in a global gravity wave climatology from GPS radio occultation temperature profiles

In a previous paper by Schmidt et al. (2008), from CHAllenging Minisatellite Payload (CHAMP) Global Positioning System (GPS) radio occultation data, a comparison was made between a Gaussian filter applied to the “complete” temperature profile and to its “separate” tropospheric and stratospheric height intervals, for gravity wave analyses. It was found that the separate filtering method considerably reduces a wave activity artificial enhancement near the tropopause, presumably due to the isolation process of the wave component. We now propose a simple approach to estimate the uncertainty in the calculation of the mean specific wave potential energy content, due exclusively to the filtering process of vertical temperature profiles, independently of the experimental origin of the data. The approach is developed through a statistical simulation, built up from the superposition of synthetic wave perturbations. These are adjusted by a recent gravity wave (GW) climatology and temperature profiles from reanalyses. A systematic overestimation of the mean specific wave potential energy content is detected and its variability with latitude, altitude, season and averaging height interval is highlighted.     

波段探测率D_(△λ)~*替代峰值探测率D_(λp)~*的讨论

文中描述了波段探测率D_(Δλ)~*的定义和计算方法,通过对空间应用的长波红外探测器的波段探测率D_(Δλ)~*与目标辐射源温度T的关系讨论,来说明波段探测率D_(Δλ)~*(和波段响应率)替代峰值探测率D_(Δλ)~*(和峰值响应率)的优越性,文中还给出了波段探测率D_(Δλ)~*的测试方法和实验计算。     

Shock/shock interactions between bodies and wings

This paper examines the Shock/Shock Interactions (SSI) between the body and wing of aircraft in supersonic flows. The body is simplified to a flat wedge and the wing is assumed to be a sharp wing. The theoretical spatial dimension reduction method, which transforms the 3D problem into a 2D one, is used to analyze the SSI between the body and wing. The temperature and pressure behind the Mach stem induced by the wing and body are obtained, and the wave configurations in the corner are determined. Numerical validations are conducted by solving the inviscid Euler equations in 3D with a Non-oscillatory and Non-free-parameters Dissipative (NND) finite difference scheme. Good agreements between the theoretical and numerical results are obtained. Additionally, the effects of the wedge angle and sweep angle on wave configurations and flow field are considered numerically and theoretically. The influences of wedge angle are significant, whereas the effects of sweep angle on wave configurations are negligible. This paper provides useful information for the design and thermal protection of aircraft in supersonic and hypersonic flows.     

行波管放大器非线性特性对调幅信号边带压缩影响

为了更精确地测试星上功率放大器的饱和点,研究分析了TWTA(Travelling-Wave Tube Amplifier,行波管放大器)的非线性特性对AM(Amplitude Modulation,调幅)信号的边带压缩影响。文中基于Saleh模型描述TWTA,分析其在AM信号放大过程中的非线性特性,研究表明:随着输入AM信号的功率不断增大,放大后的输出信号畸变越来越严重;该变化主要体现在AM信号的边带上,与线性工作区相比,在TWTA的饱和点处,经放大后的AM信号的边带压缩程度达到最大。实验结果与理论分析结果完全一致。该研究为通信卫星星上功放饱和点测试提供了一种可行方法。     

宽带双极化天线测量探头的设计与仿真

天线测量探头的性能对提升天线平面近场测量效率、最终测量结果的精度具有重要意义。针对平面近场测量的需要,应用反向四脊和差分馈电技术,设计了宽带双极化天线测量探头。对测量探头模型进行仿真,分析了带宽、方向图、隔离度和交叉极化辨识度等探头性能,确定了高隔离度、高极化纯度的宽带双极化天线测量探头的最优设计,获得了更高精度和效率的天线测量。     

利用孤立导体建立等离子体探测载荷参考电位方法

研究讨论了一种利用孤立导体在空间等离子体环境中建立探测器参考电位的技术.将一个金属导体与航天器进行电隔离,利用电路将孤立导体电位引入探测器电源模块,为探测器建立参考电位.该技术可安全方便地应用于卫星等航天器,使探测器的地电位与空间等离子体电位基本一致,避免航天器本体电位对探测器的影响.该技术将应用于中国空间站等离子体原位探测器,通过测试验证了该技术方法可以建立-210～+210V的参考电位,满足空间站等离子体原位探测器-200～+200V的参考电位技术需求.      

电路参数随时间变化的介观LC电路的波函数和压缩效应

本文通过正则变换,采用路径积分的方法,得出了电路参数随时间变化的介观ＬＣ电路的严格波函数,研究了含时相干态下电路中电荷和电流的压缩效应。