用于小幅值精确控制的纵向飞行品质准则

研究用于评定飞机小幅值姿态和航迹精确控制的纵向飞行品质准则,提出以线性化小扰动飞机方程和飞控系统为评定对象,用等效系统拟配法、系统稳定裕度、Ｎｅａｌ－Ｓｍｉｔｈ准则、姿态带宽准则、ＧＭ／ＰＭ准则和回落准则对整个飞机进行品质评价。综合分析这些准则的相互关系后,认为分别用上述６种方法评价飞机的飞行品质,可以得出该飞机的综合性能指标,而不至于得出一个片面的结论。     

捷联惯导系统动基座对准的可观测性分析

建立了SINS(捷联惯导系统)动基座对准的误差模型,首次应用PWCS(分段定常系统)可观测性分析理论对SINS动基座对准过程中的可观测性进行了全面研究.将载体的运动分解为平动和姿态变化两大类情形,深入研究和详细分析了载体的各种运动对系统可观测性的影响,指出在SINS动基座对准过程,无论载体的线运动还是角运动在一定条件下都能提高SINS的可观测性.定性地得出了不同运动对系统可观测性的影响结果,这为研究SINS的快速精确对准方法奠定了理论基础.      

企业生产系统综合评价的理论与方法研究

进入８０年代,企业生产系统所片环境的变化引起了与其相关的诸多方面的变化,也使传统的生产系统评价体系不再适应现代生产系统;发展适应现代环境的生产系统评价体系已成为当务之急,本文从生产战略角度论述了企业生产系统综合评价的重要意义及其内涵的发展与演变,对其现状进行了综述;并结合中国企业的实际情况,构造了适合现代企业生产系统的评价指标体系,提出利用模糊综合评判方法对生产系统进行评价,应用本文所述的评价指标     

混合系统的形式化验证

结合混合系统的研究对余度管理系统进行了形式化的分析和验证.采用的手段是时段演算技术及其扩展.首先进行形式化的需求分析,需求及其假设用时段演算表示,其次严格化地描述算法和参数的选取.在验证过程中,首先应用程序逻辑验证算法,算法的不变量以时段演算表示,最后在时段演算中验证整个系统的行为满足给定的需求.      

对8mm微波衰减参数计量的探讨

随着现代武器装备的更新换代和新型导弹的不断发展以及电子战中电子对抗的应用,对导弹制导雷达的要求越来越高.由于毫米波具有制导精确度高,抗干扰能力强、穿透性能好以及携带的信息量大等独特性能,因此被广泛应用于雷达、射频天线、通讯卫星、导弹等许多尖端领域.为了确保雷达的各项参数满足武器试验的要求,保障试验任务的顺利进行,对雷达的各项参数的计量检定是十分必要的.目前,"全自动8mm微波功率标准”已经建立,但8mm微波衰减参数的计量在军内还是一项空白,而衰减量值的准确与否直接影响到武器和装备性能的好坏,影响试验任务的成败.因此,我们提出了一种对8mm微波衰减参数的计量方法,以供广大从事微波计量工作的同行参考.     

一种星载GPS接收天线

根据星载 GPS接收天线的主要技术要求 ,给出了谐振式四臂螺旋天线用于星载 GPS天线的设计思路与设计过程 ,并给出了最后的测试结果。结果表明 :该天线具有十分优良的圆对称半球波束特性、良好的广角圆极化特性和优良的阻抗匹配 ,结构紧凑 ,集成度高 ,并通过了环境鉴定试验 ,为星载 GPS应用提供了一种性能优良的天线     

Interplanetary shocks and sudden impulses during solar maximum (2000) and solar minimum (1995–1996)

In this work a study is performed on the correlation between fast forward interplanetary shock parameters at 1 Astronomical Unit and sudden impulse (SI) amplitudes in the H-component of the geomagnetic field, for periods of solar activity maximum (year 2000) and minimum (year 1995–1996). Solar wind temperature, density and speed, and total magnetic field, were taken to calculate the static pressures (thermal and magnetic) both in the upstream and downstream sides of the shocks. The variations of the solar wind parameters and pressures were then correlated with SI amplitudes. The solar wind speed variations presented good correlations with sudden impulses, with correlation coefficients larger than 0.70 both in solar maximum and solar minimum, whereas the solar wind density presented very low correlation. The parameter better correlated with SI was the square root dynamic pressure variation, showing a larger correlation during solar maximum (r = 0.82) than during solar minimum (r = 0.77). The correlations of SI with square root thermal and magnetic pressure were smaller than with the dynamic pressure, but they also present a good correlation, with r > 0.70 during both solar maximum and minimum. Multiple linear correlation analysis of SI in terms of the three pressure terms have shown that 78% and 85% of the variance in SI during solar maximum and minimum, respectively, are explained by the three pressure variations. Average sudden impulse amplitude was 25 nT during solar maximum and 21 nT during solar minimum, while average square root dynamic pressure variation is 1.20 and 0.86 nPa^1/2 during solar maximum and minimum, respectively. Thus on average, fast forward interplanetary shocks are 33% stronger during solar maximum than during solar minimum, and the magnetospheric SI response has amplitude 20% higher during solar maximum than during solar minimum. A comparison with theoretical predictions (Tsyganenko’s model corrected by Earth’s induced currents) of the coefficient of sudden impulse change with solar wind dynamic pressure variation showed excellent agreement, with values around 17 nT/nPa^1/2.     

Research on a complex CME event including Hα, LASCO, radio and MDI observations

We present our research on a fast and decelerating partial halo coronal mass ejection (CME) event detected in multi-wavelengths in the chromosphere and the corona on 14 October, 1999. The event involved a whole complex active area which spanned more than 40° of heliolongitude. It included a strong solar flare (XI/1N) and a complex eruptive filament within an active region of the entire complex. Especially, several radio sources were detected in the decimetric range prior to the CME by the Nançay Radioheliograph (NRH). A linear force-free field extrapolation of the Michelson Doppler Imager (MDI) magnetogram was performed to calculate the magnetic topology of the complex prior to the triggering of the event. The presence of a coronal null point combined with the occurrence of two distant and nearly simultaneous radio sources put strong arguments in favor of the generalized breakout model for the triggering of the eruption. The analysis of the subsequent development of the event suggests that large interconnecting loops were ejected together with the CME.     

一种改善飞行员抗荷服性能的新方法

在管式抗荷服的腹囊和两侧管囊间分别装上分压装置和泄压活门,将腹囊内的压力降至管囊内压力的40%左右.在管式抗荷服研制中采用这种新型的分压技术,克服了飞行员穿着时的腹部压痛问题,改善了其舒适性,提高了飞行员的正向过载防护能力.具有分压装置的新型抗荷服进行了10人次的离心机生理试验,在过载增长率3 G/s、最大试验过载9 G条件下,分压装置工作正常,装备抗荷效果达到了3.5 G.对60名歼击机飞行员调查表明,分压装置和泄压活门的大小、安装部位及其舒适性均可接受.该技术已用于其它新型管式抗荷服的设计中.      

基于GPS遥感的延迟映射接收机关键技术

全球卫星定位系统GPS(Global Positioning System)广泛应用于定位和导航,还可利用海面对GPS信号产生的散射效应进行微波遥感,是一种新型微波遥感手段.首先介绍了GPS海洋遥感测风技术产生背景及特点,给出了GPS散射信号测量技术理论基础,重点分析了延迟映射接收机设计中提高采样信号信噪比、双射频前端电路设计、计算反射点延迟、接收机工作模式、内嵌软件处理等5项关键技术.设计的延迟映射接收机样机在天津近海完成了首次搭载飞行试验,试验结果表明,延迟映射接收机可同时接收直射和海面散射卫星信号并输出导航定位解,正确计算镜面散射点码延迟,准确接收海面散射的GPS卫星信号,且散射信号信噪比达到了14.9 dB以上,接收机输出为反演海面风场提供了准确的基础数据,这种方式可推广到遥感探测陆地土壤湿度、海冰厚度、海浪高度等领域.