某类跨大气层飞行器全航程红外辐射特性分析

针对某类跨大气层飞行器飞行过程中需要进出大气层,且飞行速度跨度大等特点,建立了不同空域、不同飞行速度下的机体头部受热模型。当在大气层内飞行时分别使用经验公式和Lees公式计算马赫数小于5和大于5时头部受热情况,当在大气层外飞行时建立了考虑太阳直射、地球反照和地球红外加热情况下的受热模型。利用普朗克定律得到了相同温度下不同波段的红外辐射能量占比情况。最后利用本方法对某类跨大气层飞行器进行了温度和红外辐射计算,得到的计算结果能够大致反映全航程头部温度和红外辐射变化情况。     

模型烧蚀对尾迹电子特性影响的计算和实验研究

 基于气动物理研究的需要,针对高焓风洞的来流特点,采用计算和实验相结合的方法研究聚丙烯烧蚀对尾迹电子密度的影响。结果表明：计算结果可以有效模拟实验状态,电子密度的模拟精度有很大提高,误差在一个量级内;聚丙烯烧蚀可以降低尾迹的电子密度,但幅度不大,在2倍左右,其与选择模型材料的催化特性降低幅度相当;对电弧风洞的成功改进和非稀薄流静电探针诊断技术的应用,是尾迹电子密度测试的前提保障。     

Study of maximum electron density NmF2 at Karachi and Islamabad during solar minimum (1996) and solar maximum (2000) and its comparison with IRI

The monthly hourly medians of maximum electron density, N_mF₂, at two Pakistani ionospheric stations, Karachi and Islamabad, have been determined for solar minimum (1996) and solar maximum (2000) and compared with IRI predictions using the URSI coefficients. At night and pre-noon period the N_mF₂ values at both stations are almost equal during the 2 years. However, at post-noon the values at Karachi are considerably larger than those at Islamabad due to the equatorial or geomagnetic anomaly. Karachi (geomag. coord. 16.44°N, 139.08°E) lies near the region of the equatorial anomaly (+20 and −20 geomagnetic latitude), so most of the N_mF₂ values at Karachi are larger than those at Islamabad (geomag. coord. 24.46°N, 145.67°E). The maximum monthly values of N_mF₂ show a semi-annual variation at Karachi and Islamabad both during 1996 and 2000 as predicted by IRI.     

微纳InSAR卫星总体技术研究

微纳合成孔径雷达干涉(Synthetic Aperture Radar Interferometry, InSAR)卫星是对地定量化遥感的重要手段。开展了微纳InSAR卫星系统总体技术研究,给出了使得干涉测量覆盖范围最大的双星编队构型设计方法,建立了低燃料消耗双星轨道参数设计准则,提出高功能密度比InSAR卫星系统的设计方法,包括载荷平台一体化、卫星高集成模块化等总体设计方法,并给出了相应的设计实例。     

GNSS Satellite Autonomous Integrity Monitoring (SAIM) using inter-satellite measurements

Integrity is the ability of Global Navigation Satellite Systems (GNSS) to detect faults in measurements and provide timely warnings to users and operators when the navigation system cannot meet the defined performance standards, which is of great importance for safety of life critical applications. Compared with both Receiver Autonomous Integrity Monitoring (RAIM) and ground based GNSS Integrity Channel (GIC) methods which are widely adopted nowadays, the Satellite Autonomous Integrity Monitoring (SAIM) method can be used to monitor orbit/ephemeris and clock errors, and has advantages in monitoring orbit and clock quality and providing instantaneous responses when faults happen.     

A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements

With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements.     

中、高密度Nomex蜂窝力学性能研究

研究了航空用三种中、高密度Nomex蜂窝的力学性能 ,并讨论了纸的厚度、浸渍溶液浓度、环境湿度和渗透剂对Nomex蜂窝力学性能的影响。结果表明 ,选择厚度合适的Nomex纸 ,严格控制湿度 ,并在浓度为 35 %～5 0 %范围内浸渍胶液中加入适量的渗透剂可以制作出与国外同类产品性能相当的高性能中、高密度Nomex蜂窝     

相关系数平稳过程时频分析方法

相关系数平稳过程是从非平稳过程中分离出的一类工程上常见且便于研究的随机过程,其均值和方差都可随时间变化,传统的平稳随机过程是它的一个特例。本文提出了相关系数AR(p),MA(q)和ARMA(p,q)序列的概念,建立了相关系数平稳过程的时频分析方法。该方法首先在时域进行全程分析,得到相关系数平稳过程的均值函数、方差函数和相关系数函数,然后可以对其进行傅里叶变换、短时傅里叶变换或小波变换,给出相关系数平稳过程的谱密度,同时提出了随机项谱密度和趋势项谱密度的概念。文中还讨论了线性系统对相关系数平稳过程输入的响应。     

飞机燃油密度实时测量及其实现方法

主要讨论了飞机燃油量实时测量的有关问题，并就其中燃油密度测量这一关键环节进行了重点论述，对密度测量的重要性、测量方法和国内外的研究状况进行了探讨。     

横向互击型层板喷注器的喷雾特性

利用激光粒子动态分析仪 (PDA)对 180°互击型层板式喷注器的喷雾特性进行了试验研究 ,测量了喷雾典型区域的液滴速度、直径、体积通量密度等参数。分析了喷注器的雾化过程和喷雾特点 ,同时重点研究了喷口槽宽、推进剂流道面积比以及推进剂喷注速度比等参数对喷雾特性的影响。试验结果表明 :喷雾沿喷口展向可分为三个明显区域 ,中间区域流量较小但雾化较细 ,从槽两端喷出的液雾流量较大但液滴尺寸较大。对于一定的流道截面比γd 和喷注速度比γv,存在一个最佳的喷嘴槽宽w使雾化质量最优。同时 ,在喷嘴槽宽合适时 ,流道截面比γd 和喷注速度比γv 的适当增大有利于改善雾化