FY-1C/D极轨气象卫星10通道扫描辐射计及其在轨运行

介绍了风云一号(FY-1)C，D极轨气象卫星10通道扫描辐射计的总体构成。给出了扫描辐射计性能的在轨测试结果，概述了研制中的技术创新点。与国内外同类仪器比较的结果表明，两星扫描辐射计寿命期初和期末的性能均满足任务书要求，其主要性能指标与美国NOAA卫星相当，甚至更佳。     

基于地球椭球特性的红外地球敏感器测量值的修正算法

基于地球的椭球特性，讨论了对扫描式红外地球敏感器的测量值进行修正的问题。利用地球椭球的小扁率特性，给出了相应的一阶修正算法。与现有文献中的方法相比，给出的算法计算简单，具有较高的精度，仿真结果表明，对于中、低轨道而言该算法的精度优于0．01°     

海上舰船目标的宽带雷达散射特征信号仿真

提出一种将目标高频电磁（EM）散射计算多径回波模型与不同海况条件下粗糙海面前向复反射系数模型相结合的方法,对海上舰船目标宽带雷达回波进行仿真和分析。简要分析了目标-海面相互作用的多径回波模型,给出了目标体的电磁散射计算方法,研究了不同海况条件下海面前向复反射系数随频率和擦地角的变化特性,并通过仿真分析了海面对舰船目标雷达回波的影响。对比分析舰船目标体直接散射及在不同海况条件下考虑多径效应时的雷达散射截面（RCS）变化特性,并在不同海况条件下对目标进行二维逆合成孔径雷达（ISAR）成像仿真,验证了本文方法的有效性。     

一种考虑地球扁率的卫星自主导航方法研究

研究用2个红外地球敏感器和1个星敏感器实现卫星自主导航的方法,地心矢量的测量精度是影响导航精度的重要原因之一,而地心矢量的测量又受到地球扁率的影响.研究地球扁率对地心矢量测量的影响,并提出一种零姿态扁率误差补偿方法,通过仿真验证了这种导航方法及扁率误差补偿算法的有效性.     

Kinetic temperature and carbon dioxide from broadband infrared limb emission measurements taken from the TIMED/SABER instrument

The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) experiment is one of four instruments on NASA’s Thermosphere–Ionosphere–Energetics and Dynamics (TIMED) satellite. SABER measures broadband infrared limb emission and derives vertical profiles of kinetic temperature (Tk) from the lower stratosphere to approximately 120 km, and vertical profiles of carbon dioxide (CO₂) volume mixing ratio (vmr) from approximately 70 km to 120 km. In this paper we report on SABER Tk/CO₂ data in the mesosphere and lower thermosphere (MLT) region from the version 1.06 dataset. The continuous SABER measurements provide an excellent dataset to understand the evolution and mechanisms responsible for the global two-level structure of the mesopause altitude. SABER MLT Tk comparisons with ground-based sodium lidar and rocket falling sphere Tk measurements are generally in good agreement. However, SABER CO₂ data differs significantly from TIME-GCM model simulations. Indirect CO₂ validation through SABER-lidar MLT Tk comparisons and SABER-radiation transfer comparisons of nighttime 4.3 μm limb emission suggest the SABER-derived CO₂ data is a better representation of the true atmospheric MLT CO₂ abundance compared to model simulations of CO₂ vmr.     

A new window on the cosmos: The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint US/German Project to develop and operate a gyrostabilized 2.5-m telescope in a Boeing 747-SP. This observatory will allow astronomical observations from 0.3 μm to sub-millimeter wavelengths at stratospheric altitudes as high as 45,000 ft where the atmosphere is not only cloud-free, but largely transparent at infrared wavelengths. The dynamics and chemistry of interstellar matter, and the details of embedded star formation will be key science goals. In addition, SOFIA’s unique portability will enable large-telescope observations at sites required to observe transient phenomena and location specific events. SOFIA will offer the convenient accessibility of a ground-based telescope for servicing, maintenance, and regular technology upgrades, yet will also have many of the performance advantages of a space-based telescope. Initially, SOFIA will fly with nine first-generation focal plane instruments that include broad-band imagers, moderate resolution spectrographs that will resolve broad features from dust and large molecules, and high resolution spectrometers capable of studying the chemistry and detailed kinematics of molecular and atomic gas. First science flights will begin in 2010, leading to a full operations schedule of about 120 8–10 h flights per year by 2014. The next call for instrument development that can respond to scientifically exciting new technologies will be issued in 2010. We describe the SOFIA facility and outline the opportunities for observations by the general scientific community with cutting edge focal plane technology. We summarize the operational characteristics of the first-generation instruments and give specific examples of the types of fundamental scientific studies these instruments are expected to make.     

红外热像仪在喷焰羽流微波衰减测试中的应用

基于发动机喷焰羽流对微波信号衰减的机理和等离子体的电子碰撞速度和电子数与温度的关系,根据喷焰羽流的红外图像,可以将喷焰羽流分成几层。通过透镜天线和对衰减多通道同时测试的方案,可以得到喷焰羽流衰减分布,并计算微波信号不同角度穿越喷焰时的衰减。     

叠氮聚氨酯弹性体(1)分子间作用力对力学性能的影响

研究了加强分子间作用力对提高叠氮聚氨酯弹性体力学性能的影响。以 HDI三聚体为固化剂的 GAP聚叠氮缩水甘油醚弹性体的拉伸强度 /断裂伸长率为 0 .66MPa/ 1 2 7.2 %。 GAP与含强极性基团的叠氮聚醚 APP共混 ,弹性体的拉伸强度随 APP用量增加而增加。红外谱图显示 ,氢键作用越强 ,弹性体力学性能越好     

红外隐身涂料的研究进展

介绍了红外隐身材料国内外研究进展情况,包括构成红外隐身材料的填料、树脂及其红外性能的各种影响因素,最后还介绍了与雷达隐身材料的兼容性问题。     

对接机构真空热试验外热流模拟方案研究

根据对接机构的结构特点和真空热试验要求,提出了红外笼、电加热片,以及红外笼+加热片组合3种对接机构外热流模拟方案.仿真计算了在真空罐模拟环境中各方案对接机构构件的稳态温度分布,并与轨道环境进行了比较.确定了最大温差构件.结果表明:红外笼方案较简单,适于正样飞行产品;电加热片和红外茏+加热片方案的地面模拟准确性较佳,适于初样地面产品试验.