基于线阵CCD的航空相机镜头焦面的自动定位系统

介绍了一种基于单片机的利用步进电机控制线阵CCD固态传感器来自动准确对镜头焦面定位的一种新方法 ,系统从根本上克服了人为因素在焦距测量中的影响 ,实现了焦距的自动测量 ,具有一定的实用价值。     

激波风洞温敏热图技术初步试验研究

介绍了可用于激波风洞等高超声速脉冲设备复杂外形模型表面热流分布显示与测量的温敏热图技术。该技术利用温敏材料发光特性随温度变化的特点实现对模型表面的温度测量,进而分析获得其表面热流分布。由于有效运行时间一般只有10ms左右,在激波风洞中采用温敏热图技术在材料温敏响应、图像采集等方面均存在困难,导致此技术还很不成熟。介绍了近期在CARDC 0.6m激波风洞中开展温敏发光热图技术研究的情况,包括发光材料的研制、材料喷涂、图像处理及标定等方面的研究工作。验证试验采用了平板加钝舵模型,获得了与理论分析及传感器测量结果较一致的平板干扰区热图结果。热图与薄膜传感器测量数据差异大致在5%~25%之间。     

航空CCD侦察相机系统研究

根据世界航空CCD相的发展概况，讨论了航空CCD侦察相机系统的技术指标、采用的技术方案和系统实现的技术途径。     

Advanced Technologies Demonstrated by the Miniature Integrated Camera and Spectrometer (MICAS) Aboard Deep Space 1

MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding the need for multi-octave spectrometers. It was flown on DS1 to validate technologies derived from the development of PICS (Planetary Imaging Camera Spectrometer). These technologies provided a novel systems approach enabling the miniaturization and integration of four instruments into one entity, spanning a wavelength range from the UV to IR, and from ambient to cryogenic temperatures with optical performance at a fraction of a wavelength. The specific technologies incorporated were: a built-in fly-by sequence; lightweight and ultra-stable, monolithic silicon-carbide construction, which enabled room-temperature alignment for cryogenic (85–140 K) performance, and provided superb optical performance and immunity to thermal distortion; diffraction-limited, shared optics operating from 80 to 2600 nm; advanced detector technologies for the UV, visible and short-wavelength IR; high-performance thermal radiators coupled directly to the short-wave infrared (SWIR) detector optical bench, providing an instrument with a mass less than 10 kg, instrument power less than 10 W, and total instrument cost of less than ten million dollars. The design allows the wavelength range to be extended by at least an octave at the short wavelength end and to ∼50 microns at the long wavelength end. Testing of the completed instrument demonstrated excellent optical performance down to 77 K, which would enable a greatly reduced background for longer wavelength detectors. During the Deep Space 1 Mission, MICAS successfully collected images and spectra for asteroid 9969 Braille, Mars, and comet 19/P Borrelly. The Borrelly encounter was a scientific hallmark providing the first clear, high resolution images and excellent, short-wavelength infrared spectra of the surface of an active comet’s nucleus.     

红外成像制导及其目标背景特性分析

结合对目标和背景的红外特性研究,阐述了在复杂背景条件下防空导弹对目标的红外成像寻的制导的组成和原理。详细分析了地面杂散背景的辐射和散射特征。综合分析了军用飞机被防空导弹攻击时的红外辐射特性。其分析结果对研究防空导弹红外成像导引头如何从复杂背景中将目标的典型特征信息提取出来并进行有效的识别具有重要的参考意义。     

星载TDI CCD相机成像仿真系统的实现

以VC++ 6.0为开发环境, 基于航天TDI (Time Delay and Integration) CCD相机地物点与像点的映射模型, 开发了TDI CCD相机成像仿真软件系统, 建立了由卫星单轴气浮姿态控制仿真台和地面星载TDI CCD相机成像仿真软件系统构成的实时航天TDI CCD相机成像仿真平台, 可动态模拟航天TDI CCD相机在进行标称偏流角调节后卫星姿态角速度误差对航天TDI CCD相机成像的影响, 仿真结果与实际成像结果基本一致.     

三维激光扫描测量技术

介绍了三维激光扫描测量系统的技术构成、测量原理,并简要地介绍了法国MENSI三维激光测量系统的技术特点;三维激光扫描测量技术在航空、航天工程中所具有的极其重要的应用价值。