我国空间电力线谐波辐射现象分析

研究了利用DEMETER卫星电磁场探测数据辨识电力线谐波辐射(PLHR,Power Line Harmonic Radiation)事件的方法,探讨了我国空间中PLHR事件的特点.通过采用时频分析和Welch功率谱估计法分析了2005-2010年6年我国空间中的全部卫星电场强度探测数据,共发现151例PLHR事件,给出了PLHR事件的统计分析和典型实例.结果表明我国空间PLHR事件的频率分布在1 000~4 500 Hz之间,多为50 Hz的奇数倍,间隔为50/100 Hz.PLHR事件与我国电网发展和变化有密切关系,与地磁活动水平无关,呈现出昼夜差异和季节差异.最后给出了影响PLHR事件探测的可能因素.     

Estimation of GPS instrumental biases from small scale network

With 4 GPS receivers located in the equatorial anomaly region in southeast China, this paper proposes a grid-based algorithm to determine the GPS satellites and receivers biases, and at the same time to derive the total electron content (TEC) with time resolution of 15 min and spatial resolution of 1° by 3.5° in latitude and longitude. By assuming that the TEC is identical at any point within a given grid block and the biases do not vary within a day, the algorithm arranges unknown biases and TECs with slant path TEC from the 4 receivers’ observations into a set of equations. Then the instrumental biases and the TECs are determined by using the least squares fitting technique. The performance of the method is examined by applying it to the GPS receiver chain observations selected from 16 geomagnetically quiet days in four seasons of 2006. It is found that the fitting agrees with the data very well, with goodness of fit ranging from 0.452 TECU to 1.914 TECU. Having a mean of 0.9 ns, the standard deviations for most of the GPS satellite biases are less than 1.0 ns for the 16 days. The GPS receiver biases are more stable than that of the GPS satellites. The standard deviation in the 4 receiver bias is from 0.370 ns to 0.855 ns, with a mean of 0.5 ns. Moreover, the instrumental biases are highly correlated with those derived from CODE and JPL with independent methods. The typical precision of the derived TEC is 5 TECU by a conservative estimation. These results indicate that the proposed algorithm is valid and qualified for small scale GPS network.     

On the observability of Mars entry navigation using radiometric measurements

A thorough observability analysis of the Mars entry navigation using radiometric measurements from ground based beacons is performed. This analysis involves the evaluation of the Fisher information matrix which is derived from the maximum likelihood estimation. A series of navigation cases with multiple beacons are investigated, and both range and range-rate measurements are considered. The determinant of Fisher information matrix is used to quantify the observability of navigation system, while the trace of Fisher information matrix is used to determine the lower-bound of estimation errors. For one and two beacon cases, the navigation system is unobservable. However, the eigenvectors of Fisher information matrix give the observable and unobservable component. When three or more beacon measurements are employed, the states of entry vehicle become observable. Some valuable analytic conclusions on the relationship between the geometric configuration of beacons and observability are obtained consequently. Finally, simulation results from two navigation examples indicate that our effort is useful for understanding and assessing the observability of the Mars entry navigation using radiometric measurements.     

基于流固耦合的充气翼内压对翼面变形影响分析

基于ABAQUS-FLUENT软件开展柔性充气翼流固耦合分析,采用反距离加权平均法实现耦合界面气动压力分布传递,采用常体积转换法实现变形数据传递,分析获得了充气翼翼面刚度和屈曲特性与翼面内外压差的关系;建立了充气翼模拟加载试验系统验证了分析方法的可行性.结果表明,流固耦合方法用于充气翼变形分析是可行的,分析结果与模拟试验结果能够较好地吻合.      

飞机侧壁部件装配调姿机构的设计与分析

分析了等曲率和变曲率2类飞机侧壁部件的几何特点以及对柔性装配调姿的功能需求,设计了一种新型的面向大型飞机侧壁部件数字化装配的柔性工装机构;该机构基于精密三坐标定位器对侧壁部件进行装配调姿,可等效为6自由度并联机构,通过4条支撑臂对侧壁部件进行夹持;定位器呈前后2排、前低后高布局,能够实现对侧壁部件空间6自由度位姿调整;对工装机构进行了位姿反解,根据侧壁部件的初始位姿和目标位姿反向求解出各支撑臂的关节变量,并利用计算机仿真模型进行了验证,证明了反解算法的正确性,为侧壁部件调姿运动的精确控制奠定了基础.      

端柱面组合密封气膜稳态特性数值仿真分析

针对航空发动机等高速流体机械中流体动密封部位的工况特点,提出一种新型的端柱面组合气膜密封形式.根据气膜密封的结构特点,建立了端柱面螺旋槽组合式密封气膜的数学分析模型.采用CFD分析软件Fluent对气膜三维流场模型以湍流流动形式进行数值模拟计算.研究了密封气膜几何结构参数变化对密封稳态特性（端面承载力F_d 、柱面承载力F_c 、泄漏量Q、摩擦转矩M）的影响.几何结构参数包括端面平均膜厚、端面槽深比、柱面平均膜厚、柱面偏心率、柱面槽深比、柱面槽宽比.      

气动负载模拟器的多余力矩分析

为了分析气动负载模拟器中多余力的形成及影响因素,介绍了气动负载模拟器的工作原理、结构框图及实验平台,推导了气动负载模拟器的数学模型,并通过实验和仿真对比模型进行了验证。采用线性化方法定性分析了影响气动负载模拟器多余力的3个因素——被动压差、惯性力矩以及摩擦力矩。采用非线性仿真定量分析了该3个因素分别对气动负载模拟器的多余力矩的影响。得出了在气动伺服加载系统中,摩擦力矩是引起系统多余力矩的重要因素。     

强不规则天体引力场中的动力学研究进展

小行星探测与彗星探测是深空探测的重要方面。一般来说,小行星和彗星因质量都不足以使得万有引力克服应力达到流体静力学平衡,而具有强不规则的外形。研究强不规则天体引力场中的动力学行为及其内在机制,是探测器被不规则天体捕获并对其形成近距离探测轨道的基础。从引力场模型和动力学行为两个方面综述了强不规则天体引力场中动力学的研究进展,在引力场模型的研究方面介绍了强不规则天体引力场建模的球谐函数摄动展开模型、简单特殊体模型及多面体模型的研究现状,在动力学机制的研究方面介绍了强不规则天体引力场中的周期轨道和拟周期轨道、平衡点、流形、分岔与共振以及混沌运动的研究现状,指出了这些方面研究的重点与难点。分析了强不规则体引力场中动力学的研究趋势。     

航空电子设备NSEE试验评价方法

本文定义了航空电子设备大气中子单粒子效应(NSEE)硬失效、硬错误与软错误等大气中子辐射可靠性表征参数,提出了一套航空电子设备抗大气中子单粒子效应危害能力的试验评价方法,包括试验应力终止条件与起始条件的确定方法、M_NSEE预估方法、试验程序、试验评价方法等,并通过某航空用卫星导航接收机试验案例证明了该方法在工程应用中的可操作性与有效性,通过掌握数字信号处理(DSP)、静态随机存储器(SRAM)、现场可编程门阵列(FPGA)的NSEE敏感特性,可为航空用卫星导航接收机NSEE危害防控提供针对性的技术支持.本文为我国航空电子产品大气中子单粒子效应试验评价奠定了理论与应用基础,同时也为其他电子信息产品在大气中子单粒子效应试验评价方面提供了重要依据和参考.