卫星星体对多波束天线的散射影响分析

地球静止轨道(GEO)移动通信卫星,多采用大反射面天线及多馈源组成的空间可展开多波束天线系统,具有更高的天线增益,并提高了整体系统性能,但由于过于庞大的天线反射面和馈源阵列,在整星结构构型布局中难免由于卫星星体或其它机构部件的存在而造成散射.文章主要针对GEO移动通信卫星星体对多波束天线散射影响问题,利用仿真分析软件,...     

卫星导航系统及其在空天安全中的重要作用

简要介绍了美国"全球定位系统"(GPS)、俄罗斯"全球导航卫星系统"(GLONASS)和欧洲正在建设的"伽利略"(Galileo)卫星导航系统的发展及其基本发展态势.详细介绍了中国自主建设的"北斗"(COMPASS)卫星导航系统的发展思路、系统组成和应用情况.分析总结了卫星导航系统在空天安全中的几项重要作用,如实现协同...     

卫星贮箱故障时液体燃料运动特性仿真分析

不少在轨卫星都使用半管理液体燃料贮箱,贮箱内的液体收集器上安装有表面筛网,可阻止贮箱内气体在发动机工作时通过收集器进入到液体燃料管路中.文章假设卫星液体燃料贮箱的底部收集器出现故障,无法阻止气体进入发动机管路.为确保卫星正常在轨运行,利用计算流体动力学数值仿真方法,对液体燃料贮箱在卫星姿态控制发动机工作时的运动规律进行...     

静止轨道卫星在轨温度参数变化规律研究

分析了静止轨道在轨三轴稳定卫星各面上温度参数的变化规律,并通过理论计算得到卫星各面上光强的变化曲线,研究了温度参数变化与对应面上光强的关系,建立了温度参数与光线的线性模型,结果表明模型与实际数据能较好地吻合,对温度参数的预测以及故障的判断具有一定的参考价值.     

终端区四维轨迹到达时间的控制与计算

研究的目的是使管制员通过飞行管理计算机计算的结果来较精确地预测飞机到达各航路点的时间范围,在同时有多架飞机进场的情况下合理安排进近顺序。利用向量分解法,分析了飞机在有风情况下,特别是风向风速改变时地速的变化。给出了实时地速的计算方式,指出了通过调节两个航路点间加速度变化的位置来控制飞机到达下一航路点的时间,并给出了到达各航路点时间范围的计算方式。通过计算,管制员不仅可以推测出到达各航路点的高度及时间范围,避免飞行冲突,还能够安全有序的引导飞机按预计时间着陆,减少航班延误量。     

飞行器轨迹优化方法综述

飞行器轨迹优化是飞行器总体设计的关键环节,特别是在现代空间飞行器和高超声速飞行器设计过程中发挥着重要作用.在全面调研国内外现有轨迹优化技术的基础上,提出了飞行器轨迹优化新的分类方式,概述了多种飞行器轨迹优化的原理和应用,并详细分析了各自的优缺点和发展趋势.最后介绍了现在实际应用的多种轨迹优化软件.     

DEMETER卫星探测到的强震前O^＋浓度变化

利用DEMETER卫星观测数据,采用level-2图像目视解译的方法和重访轨道对比方法,对2006年5月3日发生在汤加群岛的7．9级地震进行分析．从震前6天、震前2天、震前1天和震后2天的level-2图像可看到,电场和等离子体参量在震中上空偏北的位置出现扰动信号,震前的扰动信号幅度随地震时间临近有所增强,扰动持续时间也相应增加;震后2天扰动信号依然存在,其幅度并未减弱．通过对比震前1天的轨道在2006年至2008年内的重访轨道,发现O^＋浓度存在三类较规律的变化特征,即在夏季时,北半球的值高于南半球;冬季时则相反;二分季节时,南北半球含量相当．本文给出了地震和磁暴对O^＋浓度的不同影响,地震影响最靠近震中位置轨道上的O^＋浓度,而磁暴影响全球轨道上O^＋浓度分布．同时获取了DEMETER卫星上朗缪尔探针在上述重访轨道同步探测的电子浓度数据,发现电子浓度与O^＋浓度存在同步增加．等离子体浓度增加的现象可能与地震产生异常电场进而影响电离层结构有关．     

A feasibility study for the detection of the diurnal variation of tropospheric NO2 over Tokyo from a geostationary orbit

We have conducted a feasibility study for the geostationary monitoring of the diurnal variation of tropospheric NO₂ over Tokyo. Using NO₂ fields from a chemical transport model, synthetic spectra were created by a radiative transfer model, SCIATRAN, for summer and winter cases. We then performed a Differential Optical Absorption Spectroscopy (DOAS) analysis to retrieve NO₂ slant column densities (SCDs), and after converting SCDs into vertical column densities (VCDs), we estimated the precision of the retrieved VCDs. The simulation showed that signal-to-noise ratio (SNR) ? 500 is needed to detect the diurnal variation and that SNR ? 1000 is needed to observe the local minimum occurring in the early afternoon (LT13–14) in summer. In winter, the detection of the diurnal variation during LT08–15 needs SNR ? 500, and SNR ? 1000 is needed if early morning (LT07) and early evening (LT16) are included. The currently discussed sensor specification for the Japanese geostationary satellite project, GMAP-Asia, which has a horizontal resolution of 10 km and a temporal resolution of 1hr, has demonstrated the performance of a precision of several percent, which is approximately corresponding to SNR = 1000–2000 during daytime and SNR ? 500 in the morning and evening. We also discuss possible biases caused by the temperature dependence of the absorption cross section utilized in the DOAS retrieval, and the effect of uncertainties of surface albedo and clouds on the estimation of precisions.     

Dynamic orbit propagation in a gravitational field of an inhomogeneous attractive body using the Lagrange coefficients

The analytical methods have nearly been replaced by the numerical methods due to their higher accuracy and accessibility of computation facilities. The semi-analytical Lagrange method of orbit propagation using f and g series is a competitive alternative to the numerical integration technique if the Lagrange coefficients are derived in a full gravitational field. In this paper, a generalization of the Lagrange method of orbit propagation is introduced. In other words, we introduce a complete form of the Lagrange coefficients in all force fields developed in the spherical harmonics for example full gravitational field of the Earth. The method is numerically compared with the numerical integration technique. In order to show the numerical performance of the method, it has been implemented for orbit propagation of a GPS-like MEO and CHAMP-like LEO satellites. Discrepancy at centimeter level for CHAMP-like and sub-millimeter accuracy for GPS-like satellites shows relatively high performance of the developed algorithm. Compared to integration method, the proposed Lagrange method is nearly faster by a factor two for small Nmax and four for large Nmax.     

卫星导航系统天线阵接收机波束指向误差分析

研究表明：卫星导航系统阵元几何位置误差是影响波束指向误差的主要因素,而卫星和接收机位置误差则影响甚微,其中千米级的卫星位置误差以及接收机位置误差导致的波束指向误差不超过0.1°,而毫米级的阵元几何位置随机误差可导致典型7阵元天线阵波束指向误差达到几度。该研究成果可为卫星导航系统天线阵接收机的设计提供依据。