某型制导雷达部分元器件失效模式的分析

对某型号制导雷达部分元器件进行了失效分析，找出了导致元器件失效的原因，指出设计是提高可靠性的关键，并根据有关元器件情况对生产方与使用方提出了建议。着重讨论了设计师应注意的问题和应该遵循的设计原则。针对失效情况，提出了一些具体的设计构想。     

飞行控制器的多学科综合环境研究

多学科分析与优化已成为近年来飞行器设计的重要研究方法。本文介绍了一个以飞行控制器设计与分析为目的、基于多学科综合的一体化仿真软件包,说明了它的组成、特点及其主要设计问题,并以某飞行控制器设计为例阐明其应用。     

燃烧火焰温度分布重建结果误差分析

分析了采用辐射型CT算法的燃烧火焰温度发布重建结果误差产生的原因,给出了解决方法。     

叉流管－管型换热器二维温度场的数值分析

建立并导出叉流管－管型换热器传热过程的二维数学模型及相应的差分格式,对比实验数据和性能计算结果,表明数值方法是有效可行的。据此编制的计算机程序已成功地用于组合发动机空气预冷换热器工作过程的预测。     

电子设备可靠性预计参数综合分析方法研究

如何调整元器件的参数以满足可靠性要求并达到最佳的效费比?传统的方法是绘制故障率随单个预计参数变化的曲线,然后根据变化的趋势分别进行调整,但该方法很难直观地反映出多参数对故障率的综合影响,为了达到优化的目的,设计人员需要根据经验反复地调整各类参数。为此,本文结合电子产品可靠性预计软件,给出了直观分析各参数对电子设备可靠性预计结果综合影响的方法。     

Accurate approximation of in-ecliptic trajectories for E-sail with constant pitch angle

Propellantless continuous-thrust propulsion systems, such as electric solar wind sails, may be successfully used for new space missions, especially those requiring high-energy orbit transfers. When the mass-to-thrust ratio is sufficiently large, the spacecraft trajectory is characterized by long flight times with a number of revolutions around the Sun. The corresponding mission analysis, especially when addressed within an optimal context, requires a significant amount of simulation effort. Analytical trajectories are therefore useful aids in a preliminary phase of mission design, even though exact solution are very difficult to obtain. The aim of this paper is to present an accurate, analytical, approximation of the spacecraft trajectory generated by an electric solar wind sail with a constant pitch angle, using the latest mathematical model of the thrust vector. Assuming a heliocentric circular parking orbit and a two-dimensional scenario, the simulation results show that the proposed equations are able to accurately describe the actual spacecraft trajectory for a long time interval when the propulsive acceleration magnitude is sufficiently small.     

应力极值分布、强度威布尔分布的可靠性

本文运用应力—强度干涉理论,推导了应力为Ⅰ型极小值分布,强度为威布尔分布的可靠度计算公式,并对冗长的计算公式进行简化,在简化公式的基础上,运用一定的数学技巧,改变积分公式中的积分变量和上下限。将被积函数化成在某一区域内的可积函数。采用de Boor编制的一种严谨的自适应Romberg外推格式的FORTRAN程序进行数值积分。对应予不同的组合参数,给出应力服从Ⅰ型极小值分布,强度服从威布尔分布的可靠度数值。本文最后讨论了服从这两种分布的组合参数的变化对可算度数值变化的影响。     

Comparison of vertical E × B drift velocities and ground-based magnetometer observations of DELTA H in the low latitude under geomagnetically disturbed conditions

In the present work, we analyzed the daytime vertical E × B drift velocities obtained from Jicamarca Unattended Long-term Ionosphere Atmosphere (JULIA) radar and ΔH component of geomagnetic field measured as the difference between the magnitudes of the horizontal (H) components between two magnetometers deployed at two different locations Jicamarca, and Piura in Peru for 22 geomagnetically disturbed events in which either SC has occurred or Dst_max < ?50 nT during the period 2006–2011. The ΔH component of geomagnetic field is measured as the differences in the magnitudes of horizontal H component between magnetometer placed directly on the magnetic equator and one displaced 6–9° away. It will provide a direct measure of the daytime electrojet current, due to the eastward electric field. This will in turn gives the magnitude of vertical E × B drift velocity in the F region. A positive correlation exists between peak values of daytime vertical E × B drift velocity and peak value of ΔH for the three consecutive days of the events. It was observed that 45% of the events have daytime vertical E × B drift velocity peak in the magnitude range 10–20 m/s and 20–30 m/s and 20% have peak ΔH in the magnitude range 50–60 nT and 80–90 nT. It was observed that the time of occurrence of the peak value of both the vertical E × B drift velocity and the ΔH have a maximum (40%) probability in the same time range 11:00–13:00 LT. We also investigated the correlation between E × B drift velocity and D_st index and the correlation between delta H and D_st index. A strong positive correlation is found between E × B drift and D_st index as well as between delta H and D_st Index. Three different techniques of data analysis – linear, polynomial (order 2), and polynomial (order 3) regression analysis were considered. The regression parameters in all the three cases were calculated using the Least Square Method (LSM), using the daytime vertical E × B drift velocity and ΔH. A formula was developed which indicates the relationship between daytime vertical E × B drift velocity and ΔH, for the disturbed periods. The E × B drift velocity was then evaluated using the formulae thus found for the three regression analysis and validated for the ‘disturbed periods’ of 3 selected events. The E × B drift velocities estimated by the three regression analysis have a fairly good agreement with JULIA radar observed values under different seasons and solar activity conditions. Root Mean Square (RMS) errors calculated for each case suggest that polynomial (order 3) regression analysis provides a better agreement with the observations from among the three.     

单航过单平台InSAR基线模型的敏感性分析

从单航过单平台InSAR系统对其自身基线的高精度需求出发,给出了光学测量方案下的基线模型,并针对模型中的各因素及其误差来源,进行了模型的敏感性分析,阐明了测量元素与位置修正矢量的基线矢量的误差传递关系,然后根据误差传递关系找出测量系统的优化安装部位。通过解析推导得出各类误差源在不同条件下对基线精度影响的理论结果,由仿真分析给出了不同安装部位的误差传递系数。通过敏感性分析可由测量环境的输入条件直接获得基线的误差量级,其结果可作为指导测量系统方案设计与精度分配的参考依据。     

基于嵌入式MATLAB函数编程的火星车能量平衡仿真系统

在以往航天器研制过程中,电源系统能量平衡分析是基于表格化计算的方法,其运算效率低、显示不直观。文章提出了一种可视性强、易编程、更通用的能量平衡分析方法,即采用嵌入式MATLAB函数对电源系统能量平衡分析的功能模块进行编程实现,以火星车电源系统为应用背景,在MATLAB/SIMULINK平台上搭建了一套用于能量平衡分析的仿真系统,并在特定实例下进行仿真分析,仿真结果采用图表曲线形式显示,能清晰、直观地反映能源利用的动态变化趋势,可为电源系统方案优化设计提供参考依据。