Ka波段高增益圆极化机载微带天线阵的设计与实现

设计、分析、制作了一种工作在Ka波段的4单元高增益、圆极化机载微带天线阵列。利用顺序旋转阵列和串并馈方式的微带线网络馈电,显著改善了天线的轴比带宽和驻波带宽,减少了馈线损耗,实现了高增益。采用L型微带调配枝节对贴片单元进行匹配,便于组阵,解决了阵列空间布局不合理的难题;馈电网络和天线单元集成在同一介质基板上,易于加工和制作。测试结果表明:该天线阵具有高增益和良好的圆极化特性,从而证实了该方法的正确性和实用性。本文所设计的天线由于具有体积小、质量轻、结构紧凑、易于集成等优点,在机载相控阵雷达以及卫星通信系统中具有很好的应用前景。     

微波测量技术在表面粗糙度测量中的应用

根据电磁波在金属表面反射的理论,提出了利用微波测量技术测量表面粗糙度的新方法。利用微波技术理论分析了测量原理,给出了测试装置图,介绍了系统的工作原理,最后,给出了实验结果和误差分析。这种方法具有非接触测量的优点。     

宽波束圆极化微带天线设计

为了提高天线导航信号的有效覆盖面积,研究了应用于全球卫星定位系统(GPS)的宽波束圆极化微带天线。采用四个半径不同的非对称扇形切角实现天线辐射方向图的宽波束特性,天线的整体尺寸为0.395λ0×0.395λ0×0.016λ0(λ0为天线中心频率1.575GHz对应的工作波长)。应用商用仿真软件HFSS对天线进行了仿真设计,结果表明,该天线的圆极化带宽为13MHz(1.566~1.579GHz),阻抗带宽为78MHz(1.556~1.634GHz),增益大于5.9dBic,天线在中心频率1.575GHz时方向图的3dB轴比波束宽度为165°。在仿真设计的基础上,制作天线的工程样机,样机测试结果与设计结果吻合良好,说明了设计方法的有效性。     

微波推力器独立系统的三丝扭摆推力测量

为了探究微波推力器的推力性能,采用三丝扭摆推力测量方法对微波推力器独立系统开展推力测量实验,同时分析三丝扭摆推力测量装置的数理模型并实验测定其不确定度,由此判断实验测量结果的可信度。推力测量结果表明,现有实验条件下三丝扭摆推力测量装置能测出不低于3mN的推力,其相对不确定度为14%;在三丝扭摆推力测量装置的推力测量范围内,没有测出微波推力器独立系统显著的推力,而是在230W微波功率输出条件下测出推力在±0.7mN范围内波动,相对不确定度大于80%。     

微波暗室反射率电平自动校准方法及测量不确定度

通过开展1~40 GHz微波暗室性能自动校准技术研究,研制了低反射8维度空间测试支架,降低了测试装置微波干扰;开发了基于Labview 8.6环境的测试系统控制软件,实现信号调整和收发天线的相对运动;本文就微波暗室自动校准系统静区反射率电平测量不确定度进行了分析和评定。     

扫频RCS测量技术及应用

简要地介绍了扫频法测量目标RCS的原理,并构建了一种基于矢量网络分析仪的测量系统,利用时域相减法消除了系统的隔离误差,最后给出了在微波暗室中的一些实际测量结果.     

导弹天线罩IPD单喇叭测量仪机械系统的研究与实现

从电磁波的传输特性出发,分析了导弹天线罩IPD单喇叭测量原理。根据天线-天线罩电性能综合测试系统对测试转台的要求,明确了测量仪应具备的功能。通过研究单喇叭与天线罩的相对运动原理,提出了喇叭相对天线罩运动的结构布局,并设计了模块化的微波测量结构。试验表明,该系统能满足某型号导弹天线罩IPD的测量要求。     

扫频RCS测试系统原理及应用

本文介绍了我国第一台室内扫频ＲＣＳ测量与微波成像测量两种功能兼容的测试系统，简述了其基本结构和工作原理；展示了关于ＲＣＳ测量和成像测量的实用信号处理方法；并例举了某些实测结果。     

波导系统中后置极化器的失配效应

众所周知，后置极化器阻抗的失配，对于圆极化波导系统的工作性能有不良的影响。本文对此影响进行了分析。     

全红外光激发里德堡原子微波电场测量

基于高激发里德堡原子的微波电场测量技术与传统金属天线相比有诸多优越性,是未来微波电场高精度测量的重要方案之一。采用全红外光激发里德堡原子的方案不再依赖复杂而昂贵的短波长激光器,大大减小了激光器系统的体积与能耗。在三红外光级联激发里德堡铷原子的过程中,发现了中间态对应的双光梯形电磁诱导透明光学参数对三光激发里德堡态电磁诱导吸收峰信噪比具有重要影响,因此采用光失谐方法能很好地优化三光EIA光谱。利用微波场下的Autler-Townes分裂效应和标准天线方法对微波喇叭天线发射的微波电场实现精确的校准,并以此为基础通过超外差接收技术成功探测到本地场与信号场所形成的拍频信号,得到了拍频光电信号与信号场强度之间的线性关系。最终通过实验噪声基底的噪声功率谱得到三红外光里德堡铷原子微波测量的极限灵敏度为37.5(5.5) nV·■。采用三束红外光激发的方法为研制小型里德堡原子微波电场探测仪器奠定了物理基础。     

煤油/氧气预爆器爆震波特性研究

为了解决液态煤油旋转爆震发动机短距离快速起爆问题,进行了煤油/氧气预爆器方案设计。此方案包括双级轴向旋流和离心喷嘴匹配方案、半圆轴向垂直预爆管和圆管切向预爆管等设计,建立了液态煤油/氧气预爆器爆震波特性试验台。探讨了不同工作时序、当量油气比、预爆管结构等对预爆器爆震燃烧特性的影响。结果表明预爆器产生的爆震波压力达到4.0MPa以上,爆震波传播速度高于1300m/s,液态煤油/氧气最佳当量油气比存在于0.6-0.73之间一点。对比半圆轴向垂直预爆管和圆管切向预爆管,圆管模型爆震波压力明显高于半圆管模型,而传播速度却低于半圆管模型,圆管模型整体存在着前导激波的生成,而半圆管模型却在生成的爆震波后方有明显的压力波动现象     

不同截面机身的RCS及气动特性研究

对三个“板块”多边形截面机身及圆截面机身模型进行了RCS隐身特性和低速气动特性的测试与研究,发现多边形截面机身不但具有良好的隐身性能,特别是机身侧面,无论是水平极化或是垂直极化,其RCS值均比相同截面面积的圆截面机身降低一个数量级,而且其气动特性不比圆截面机身差,其升力特性与最大升阻比均比圆截面机身好。最后还给出了考虑多边形侧边缘夹角的横向绕流粘性效应的经验修正公式,可供多边形截面机身的气动特性估算参考。     

高功率微波极化方式与入射方向对微带线耦合特性影响分析

针对高功率微波（HPM）耦合效应分析需求,采用时域多分辨分析法（MRTD）模型,给出了微带线端口电压和电流方程,验证了模型的适用性。基于MRTD,仿真分析了HPM作为入射波时其极化方式、入射方向对微带线电磁耦合特性的影响。结果显示：垂直线极化波和平行线极化波耦合系数峰值出现在不同的频率,且峰值相差约15 dB,采用圆极化波时耦合系数最大;入射方向变化时,耦合系数以水平入射最小,垂直入射时最大,高频段微带线边缘有绕射现象产生。该分析采用了分析计算电大尺寸HPM耦合效应的MRTD数学模型,提高了HPM与复杂结构的耦合计算效率。     

Containment ability and groove depth design of U type protection ring

High-energy rotor uncontained failure can cause catastrophic damage effects to aircraft systems if not addressed in design. In this paper, numerical simulations of three high-energy rotor disk fragments impacting on U type protection rings are carried out using LS-DYNA. Protection rings with the same mass and different groove depths are designed to study the influence of the groove depth. Simulation results including kinetic energy and impact force variation of single fragment are presented. It shows that the groove depth infects both the axial containment ability of the protection ring and the transfer process of energy. The depth of groove ought to be controlled to an appropriate value to meet both the requirement of axial containment and higher safety factor. Verification test on high-speed spin tester has been conducted and shows that protection ring with appropriate U structure can resist the impact of the disk burst fragments. The ring is inflated from a circular to an oval-triangle shape. The corresponding simulation shows good agreement with the test.     

Statistical Characteristics ics of the Polarization Power Ratio for Radar Return with Circular Polarization

In this paper, the radar return from a clutter target illuminated by acircularly polarized wave is investigated statistically. The ratio of theenvelope of the left circular component to that of the right circularcomponent of the return signal is formed, and the probability densityfunctions and cumulative distributions of this ratio are found forlinear, square, and logarithmic law detectors. Plots of all densities anddistributions are given for several statistically modeled clutter-typetargets with typical depolarizing and back-scattering characteristics.The probability density functions for the ratio signal from a logaritmicic detector are compared for the cases of circularly and linearlypolarized waves incident on the same clutter-type target. Linearpolarization produces the worst case of spreading of the probabilitydensity function from its median value. Plots are given which indicatethat changes in the amount of depolarization by the clutter cause moresignificant changes in the median value of the polarizationration forlinear than for circular polarization.     

Polarizing gas at small optical depths around Algols

The origins of visible-band linear polarimetry of Algols and objects related to them are reviewed. It is pointed out, not for the first time, that the polarization signals of these systems can vary sporadically by significant amounts. The difficulty of evaluating the interstellar component of the observed polarization is discussed and these components are evaluated anew for each object studied in this paper. With one possible exception, the polarization signals intrinsic to these binaries derive from electron scattering. A well-defined model is applied to the constant and variable (but phase-locked) polarization signals. Limits to the mass associated with a scattering disk in each binary are derived. Within broad limits, concentrations of scattering mass within and above or below the orbital plane are also developed as are the centroid longitudes of these concentrations within the system. It is pointed out that very few measures of visible-band, circular polarization have been made but that cm-wavelength measures of Algol itself have been very informative.     

Polarizing gas at small optical depths around Algols

The origins of visible-band linear polarimetry of Algols and objects related to them are reviewed. It is pointed out, not for the first time, that the polarization signals of these systems can vary sporadically by significant amounts. The difficulty of evaluating the interstellar component of the observed polarization is discussed and these components are evaluated anew for each object studied in this paper. With one possible exception, the polarization signals intrinsic to these binaries derive from electron scattering. A well-defined model is applied to the constant and variable (but phase-locked) polarization signals. Limits to the mass associated with a scattering disk in each binary are derived. Within broad limits, concentrations of scattering mass within and above or below the orbital plane are also developed as are the centroid longitudes of these concentrations within the system. It is pointed out that very few measures of visible-band, circular polarization have been made but that cm-wavelength measures of Algol itself have been very informative.     

旋转弯管内粘性流动特性的研究

基于工业上的应用,本文利用摄动方法求解了小曲率旋转变管内的粘性流动,系统地分析了主流速度、二次流动、流量和摩擦力在科氏力（Ｃｏｒｉｏｌｉｓ ｆｏｒｃｅ）和离心力共同作用下特性的变化情况;表明由于旋转的效应,旋转弯管内的流动状况较弯管内的流动状况复杂;同时还发现当科和和离心力之比Ｆ≈－１．２２时,二次流强度最弱,此时该流动近似为非旋转直管内的流动（Ｐｏｉｓｅｕｉｌｌｅ流）。     

Microwave spectrum analysis as solar energy release diagnostics

The possibilities of using spectrographic observations of microwave radio emission as a solar flare plasma diagnostic are discussed. The spectral fine structure of the emission is interpreted in the context of plasma emission mechanisms. The balance equations for particles and plasma turbulence together with the transfer equations for electromagnetic waves in a plasma are solved for a model containing a diverging magnetic loop. As a result of the analysis of the blip-type spectral feature, the structure of energy release region and the unperturbed plasma concentration in the preflare loop are evaluated. The number of accelerated electrons and the intensity of the plasma turbulence in the source region are estimated using the properties of the weak continuum emission following the blip. Based on the degree of circular polarization of both the narrow band and the continuum emission, estimates for the external magnetic field strength and the angular width of the radiating plasma turbulence have been obtained.     

应用计算机绘图研制螺旋天线

本文介绍的是为有源雷达回波增强器研制的阿基米德平面螺旋和等角平面螺旋天线,并给出方向性图,电压驻波比和圆极化等电参数从S波段到X波段的测试结果。 在研制过程中用SKG语言（配DJ-052微机和绘图仪）进行编程并自动画出各种天线的精确形状,它捂言简练,工效很高。