一种单路开环对消电路设计

文中设计一种形式新颖的开环对消电路 ,用于提高收发天线的隔离度 .它由耦合器、衰减器、移相电路和加法器组成。具有宽频带 ,结构简单 ,体积小等特点。试验结果表明 ,此对消电路可在 40 0 MHz工作频段内实现 1 0 d B以上对消比     

一种新的基于粗集的辐射源信号识别模型

粗糙集理论作为一种新的处理含糊和不确定性问题的数学工具,已成为国际学术界的一个前沿的研究领域。在深入研究粗糙集理论的基础上,将其引入辐射源识别问题中,给出了一种基于粗糙集的辐射源信号识别模型。同时给出了一种不依赖先验知识确定辐射源识别权值的新方法,并提出了一种新的分类规则。最后,进行了计算机仿真实验,并与经典的模糊模式识别及统计模式识别方法进行了比较,实验结果证明了该方法的优势和有效性。     

四边形全天自主星图识别算法

讨论了一种新的无须任何先验知识的星图识别算法。该算法将四边形星图模式分解为两个具有公共边的三角形模式，使用三角形模式的特征，在保证自满计算量和星载星表的存储容量的前提下，使算法的识别成功率得以星著提高。Ｍｏｎｔｅ Ｃａｒｌｏ实验表明，在星等误差０．５星等（３σ），位置误差１０角秒（１σ）时，该算法的识别成功率接近１００％。     

飞机测高天线的设计

文章研究了微带天线的设计,论述了其结构及应用,介绍了设计流程和要求,并利用HFSS设计了一个用于飞机测高的天线,中心频率在444MHz。仿真结果表明,所设计的微带天线有较好的辐射特性,满足设计要求。     

深空通信天线组阵关键技术及其发展趋势

天线组阵是未来深空通信中的重要发展方向之一。本文介绍了天线组阵的发展历程,重点讨论了组阵中的关键技术,包括阵址选择、阵元口径和数量设计、阵构型设计以及信号处理的方法,分析了上述技术对组阵性能的影响。最后,探讨了天线组阵的发展趋势。
     

项目管理在航空售后服务体系中应用模式的研究

项目管理作为一种管理工具在许多领域中的使用已有非常悠久的历史，而现代项目管理起源于上世纪50年代，它一出现就引起举世瞩目。在理论上各国家或协会关于项目管理的概念仍有一些不同认识，不同经济领域中具体操作起来又有方法上的差别，但其精髓和原理却是一致的。本文根据现代项目管理精髓在其九大知识领域、五个过程组的模型上结合中国航空企业售后服务工作的特点，通过一些具体项目的操作应用，研究应用实践出可操作的售后项目管理模式。实践证明，此模式方法的使用可节省质量运行成本、提高工作效率，值得在今后售后工作包括类似工作中推广应用。     

Antenna pattern control of planar arrays for long distance communications

As an alternative to standard antennas and due to the advent of low-cost digital processors and materials, adaptive antenna arrays are increasingly considered for applications in long distance communications. The pattern beam control potentialities provide the performance improvement of the communication systems. In this context, this work presents a technique that permits to synthesize the antenna pattern of a planar array. Considering that the relationship between the array factor and the array excitations for the far field region is a Fourier transform in the appropriate variables, the non-uniform sampling procedure is extended for planar arrays. These arrays permit a further control of the antenna pattern since two dimensions of space are used. The technique considers a number of array factor points equal to the array size, which is used to impose appropriated values in the antenna pattern. The produced array factor passes through those points with the desired values, which allows the synthesis of antenna patterns with appropriated characteristics. The theory is presented in order to develop the necessary direct expressions to calculate the array excitation. The array factor can be obtained using the inverse Fourier transform. As application examples, with this technique it is possible to define the level of each sidelobe of the antenna pattern, to control the main beam and to impose nulls in prescribed directions of the pattern.     

天线雷达散射截面的分析与实验

本文利用天线散射的基本原理，以波导激励振子抛物面天线为例，计算并分析了天线的结构项散射雷达截面ＲＣＳｓ和模式项散射雷达截面ＲＣＳｅ，给出了此天线雷达截面的预估值。实验结果表明，理论预估值与实测值吻合较好，并且证明天线的模项ＲＣＳｅ大于结构项ＲＣＳｓ，天线总的雷达截面主要受天线模式散射的影响，减小模式项ＲＣＳｅ将有效地降低天线的雷达截面。本文结果为探索以克服天线模式散射为主的天线ＲＣＳ减缩技术提供了理论依据     

RF communications subsystem for the Radiation Belt Storm Probes mission

The NASA Radiation Belt Storm Probes (RBSP) mission, currently in Phase B, is a two-spacecraft, Earth-orbiting mission, which will launch in 2012. The spacecraft's S-band radio frequency (RF) telecommunications subsystem has three primary functions: provide spacecraft command capability, provide spacecraft telemetry and science data return, and provide accurate Doppler data for navigation. The primary communications link to the ground is via the Johns Hopkins University Applied Physics Laboratory's (JHU/APL) 18 m dish, with secondary links to the NASA 13 m Ground Network and the Tracking and Data Relay Spacecraft System (TDRSS) in single-access mode. The on-board RF subsystem features the APL-built coherent transceiver and in-house builds of a solid-state power amplifier and conical bifilar helix broad-beam antennas. The coherent transceiver provides coherency digitally, and controls the downlink data rate and encoding within its field-programmable gate array (FPGA). The transceiver also provides a critical command decoder (CCD) function, which is used to protect against box-level upsets in the C&DH subsystem. Because RBSP is a spin-stabilized mission, the antennas must be symmetric about the spin axis. Two broad-beam antennas point along both ends of the spin axis, providing communication coverage from boresight to 70°. An RF splitter excites both antennas; therefore, the mission is designed such that no communications are required close to 90° from the spin axis due to the interferometer effect from the two antennas. To maximize the total downlink volume from the spacecraft, the CCSDS File Delivery Protocol (CFDP) has been baselined for the RBSP mission. During real-time ground contacts with the APL ground station, downlinked files are checked for errors. Handshaking between flight and ground CFDP software results in requests to retransmit only the file fragments lost due to dropouts. This allows minimization of RF link margins, thereby maximizing data rate and thus data volume.     

低轨卫星缺失时序数据的模式识别方法

在航天应用中，低轨卫星经常会由于原始数据缺失而影响卫星时序数据模式识别结果，降低准确率。针对该问题提出了一种新型MR-GRU模型，可有效处理缺失时序数据，并获得较好的模式识别准确率。区别于传统模型的补全缺失数据的方法，MR-GRU模型直接在缺失时序数据上运用循环神经网络进行训练，对传统门控循环单元结构进行了改进，增加了两个新变量：掩蔽项和衰减项。掩蔽项作用于输入，衰减项作用于输入和隐层单元输出。MR-GRU模型不仅能够保持时序数据固有的时间特性，还能有效提高模式识别精度。在卫星时序数据上的模式识别试验表明，MR-GRU模型准确率优于传统模型。