一种基于双模式成像的遥感图像去运动模糊方法

对地观测载荷大多工作在颤振环境之中,这种颤振造成光轴偏移、像面抖动,由此产生的运动模糊对高分辨率成像与高精度探测产生了极为不利的影响。对空间相机像面去模糊的工作,大致分为两种方案：一种为硬件实时探测加硬件实时补偿,另一种为硬件实时探测加事后软件补偿。文章提出通过主成像相机的双成像模式获得低信噪比无抖动图像和正常信噪比模糊图像,利用图像处理手段从这一对图像中求得抖动信息（模糊核）,并以此为先验知识指导模糊图像的复原,抑制像面抖动。这种方法既不需要补偿器件,也不需要探测元件和探测支路,并在图像迭代处理过程中不断修正模糊核,在初始模糊核有一定误差的情况下,同样可望取得良好的像面去模糊效果,对于遥感图像像质提高具有潜在的应用价值。     

AFM诱导氧化加工Si纳米氧化线的一致性和连续性的研究

研究了在不同的偏置电压和扫描速度下加工的Si氧化线的一致性和均匀性,得到了加工高质量的Si氧化线的实验条件为:偏置电压8V,扫描速度1 μm/s。     

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.     

美国IKONOS和QuickBird2卫星相机的主要性能和特点分析及看法

简述美国的IKONOS和QuickBird2卫星性能 ,重点分析卫星相机的主要性能和特点 ,结合我国研制的高分辨率空间相机提出几点看法     

线阵CCD相机试验室像质测试的配准方法研究

文章讨论了在线阵CCD相机整机静态和动态像质测试中,由靶标像和CCD像元间配准的不确定性所引起的测量结果的不确定性,推导了在奈奎斯特频率下测量其静态和动态像调制传函时,矩形线条状靶标像和CCD像元间的对准位错量所引起的位错MTF计算公式,并按此公式提出了一类位错靶标的设计方法和使用方法,该位错靶标可使配准简化,提高测量结果的确定性。     

利用GPS非差观测值的GRACE卫星精密定轨

参照GPS精密单点定位（PPP，Precise Point Positioning）模型设计了一种新的卫星定轨方法一组合星载加速度计测量数据和IGS提供的GPS精密星历及精密钟差数据进行低轨卫星的精密定轨。利用星载加速度计提高卫星受力模型准确性，使动力法定轨精度和可靠性都得到提升。同时，采用多种改正技术提高GPS非差观测值测量精度，保证最终高精度卫星定轨。本文建立了卫星定轨的轨道滤波模型，得出了有益的结论，即采用星载加速度计测量卫星非保守力可提高卫星定轨精度，在ITRF2000参考系下三轴精度优于18cm。这种方法不需要在全球建市基准观测站．定轨设备简单．费用低廉．     

中国星载CCD相机控温仪性能比较

星载CCD相机热设计中的主动控温加热器一般由控温仪来完成自动控制。中国卫星普遍采用的控温仪是常规电子开关型控温仪和智能型控温仪，文章对这两种控温仪的性能进行了多个方面的比较。     

CMOS相机在微小卫星上的应用

文章主要介绍了CMOS探测器件相对于CCD器件的优点 ,讨论了CMOS焦平面的的设计方案 ,最后给出了CMOS相机的实验室成像结果和外景成像结果。     

应用动态物像矢量共轭关系计算航天相机像移

首先建立了航天相机的坐标系，明确了物像矢量之间的几何对应关系，其次定义了航天相机中的作用矩阵关系式；最后根据静态以及动态的物像矢量共轭关系，进行了航天相机的像移计算分析，结果表明该方法概念乘法，公式意义明确，结果与齐次坐标变换方法结合一致。