具有几何和光照不变性的不变矩构建研究

为了解决现有的光照变化条件下仿射不变矩识别不稳健的问题,提出了一种归一化光照仿射不变矩,即采用一种光照模型,基于Jan Flusser仿射不变矩,推导出一种归一化光照仿射不变矩,并且从理论上证明了该方法在各种仿射变换下的稳健性,然后通过对比实验验证了该方法在光照强度、方向和颜色改变下的不变性.实验结果表明,与当前主流的光照不变矩方法相比,该方法不仅适合灰度图像也适合彩色图像,在光照方向改变下,图像的倾斜运动中识别度提高了35％;在线性光照强度改变下,图像的倾斜运动中识别度提高了85％;在光照颜色改变下,图像的平移和旋转运动中识别度提高了7.8％;以多种卫星模型图像为实验对象,在光照改变下,彩色图像和灰度图像的识别度平均提高了36％以上,且计算简单,更适合于航天器目标的识别.     

航空发动机离心式喷嘴宏观喷雾特性

为探究航空发动机离心式喷嘴的喷雾宏观特性,通过将该喷嘴在高温高压定容弹中进行喷雾过程的实验,并结合阴影法与纹影法进行光学测量.首先以水作为射流工质,观察不同喷射压力下水进入大气环境中的雾化角变化,发现喷嘴结构对雾化角有着重要影响,最大雾化角与喷嘴出口的导流结构夹角相等.其次以正癸烷作为工质,通过不同环境压力和温度下的多...     

月球南极着陆区关键特性分析

与月球中低纬度着陆区不同,月球南极地区地形地貌条件较为恶劣,太阳高度角低,对地可见与不可见周期较长,这些关键特性都对南极着陆探测任务提出了挑战。文章结合国内外已开展的研究工作,对南极地区的光照条件、对地可见、地形地貌等方面进行了分析和总结,得到了上述关键特性的规律。南极地区不存在永久光照区,但存在一些几百米尺度的4~9个月的准连续光照区,着陆器的光照条件与着陆器高度密切关联;南极地区光照条件和对地可见受地形影响较大;在50m基线情况下,备选着陆区域平均坡度比较平缓(0°~5°);着陆器尺度5m基线情况下,不同备选着陆区域平均坡度相差较大,最大平均坡度可以达到25°。根据上述分析,对我国开展月球南极探测的任务规划和探测器系统设计提出了建议,主要包括着陆区的选择及探测器主要功能组成等。     

Effects of in-track maneuver on Sun illumination conditions of near-circular low Earth orbits

By developing approximate analytical models considering the J₂ perturbation, the effects of an in-track maneuver on the orbital Sun illumination conditions of near-circular low Earth orbits are analyzed. First, two approximate models for the variations in orbital sunshine angles are developed, one for variations at a given time and the other for variations at a given argument of latitude. Next, two approximate models for variations in orbital arc in Earth shadow are developed, one considers the small eccentricity and the other uses the zero eccentricity. Finally, the developed approximate models are applied to analyzing the Sun illumination conditions of a typical in-track maneuver mission on a near-circular low Earth orbit. From the results obtained, three major conclusions can be drawn. First, the variations in orbital sunshine angles at a given time may reach tens of degrees when the drifting time reaches hundreds of orbital periods, and the approximate model for that situation cannot effectively approach the numerical results. Second, the variations in orbital sunshine angles for any given argument of latitude are only a couple of degrees even when the drifting time reaches 500 orbital periods, and the approximation model developed can effectively approach the numerical results. Third, for variations in orbital arc in Earth shadow, the approximate model considering the small eccentricity has simple expressions and can effectively approach the numerical results; in contrast, the approximate model using the zero eccentricity has relatively worse precision.     

基于光照模糊相似融合不变矩的航天器目标识别

针对航天器目标识别中现有的光照变化和图像模糊条件下几何仿射不变矩识别不稳健问题,根据灰度光照模型,结合图像模糊和不变矩的基本理论,提出了一种光照模糊不变量,与几何仿射不变矩进行融合,构建出一种新的光照模糊相似融合（CIBA）不变矩,并从理论上证明了光照、模糊和相似变换（平移、缩放和旋转）不变性。对3种不同的航天器目标的识别实验表明,光照模糊相似融合不变矩在最小距离分类器中的识别准确率达到了86.37%,比几何仿射不变矩提高了94.00%,比具有光照不变性的几何仿射不变矩提高了24.54%,有效地解决了对不同位姿、不同光照模糊条件下的航天器目标识别问题,提高了基于矩的目标识别鲁棒性。     

Influence of lunar topography on simulated surface temperature

The surface temperature of the Moon is one of the essential parameters for the lunar exploration, especially to evaluate the Moon thermophysical features. The distribution of the temperature is heavily influenced by the Moon topography, which, however, is rarely studied in the state-of-art surface temperature models. Therefore, this paper takes the Moon topography into account to improve the surface temperature model, Racca model. The main parameters, such as slopes along the longitude and latitude directions, are estimated with the topography data from Chang’E-1 satellite and the Horn algorithm. Then the effective solar illumination model is then constructed with the slopes and the relative position to the subsolar point. Finally, the temperature distribution over the Moon surface is obtained with the effective illumination model and the improved Racca model. The results indicate that the distribution of the temperature is very sensitive to the fluctuation of the Moon surface. The change of the surface temperature is up to 150 K in some places compared to the result without considering the topography. In addition, the variation of the surface temperature increases with the distance from the subsolar point and the elevation, along both latitude and longitude directions. Furthermore, the simulated surface temperature coincides well with the brightness temperature in 37 GHz observed by the microwave sounder onboard Chang’E-2 satellite. The corresponded emissivity map not only eliminates the influence of the topography, but also hints the inherent properties of the lunar regolith just below the surface. Last but not the least, the distribution of the permanently shadowed regions (PSRs) in the lunar pole area is also evaluated with the simulated surface temperature result.     

航天器仪表与照明分系统设计和发展

航天器仪表与照明分系统承担着飞行器与航天员信息交互的任务,为航天员在轨工作、生活提供支持。分系统功能包括信息显示提示、越限报警提示、手动操作、工作生活照明、休闲娱乐等。文章给出了航天器仪表与照明分系统设计思路及分系统设计组成;分析了分系统技术应用情况;对应航天器设计和应用结果,提出了后续航天器的技术发展思路和设想。     

基于CCD摄像法进行液位测量的研究

建立了用于液位测量的CCD摄像测量系统。在散射照明的条件下,液位图像成像到高分辨力的电荷耦合器件上,然后通过对传感器信号进行分析和处理,可以精确地计算出液位的高低。利用CCD摄像法实现液位精确测量,处理电路采用C8051F060单片机为核心器件对传感器输出信号进行处理,通过单片机串口将采集的数据传输给计算机。系统具有非接触、实时性、高准确度以及自动化的特点。     

一种相变热图的图像处理方法

相变热图技术中,为了得到风洞试验模型表面的热流分布,必须对相变热图序列进行相变线提取.首先通过特殊的时-空变换,将所有原始序列图像的直接分割转化为对少量合成图像的分割,在减小计算量的同时较好地解决了原始图像中由于相变区域模糊而难以分割的问题.同时,为了解决由于模型表面存在镜面反射造成的模型头部区域相变线提取不准确,引入镜面反射模型,并通过分割和参数求取过程的迭代执行计算出反射模型各参数,对合成图像进行整体性亮度补偿并最终得到良好的分割结果.最后根据提取出的相变线位置和材料相变温度,完成热流值的计算.通过比较表明本文结果更为准确合理,也验证了所提出分割方法的有效性,促进相变测温技术的广泛应用.