NSCT变换域PCNN彩色图像增强算法

为了改善由于光照不均对真彩色图像的影响,根据人类对颜色的感知特性,利用YCbCr彩色模型空间,提出了一种基于非抽样Contourlet变换（ NSCT）的PCNN模型的图像增强算法。首先,将图像从RGB彩色空间转换到YCbCr彩色空间;然后对亮度分量进行NSCT分解,得到低频子带系数和高频方向子带系数,对低频子带,利用PC－NN增强,对高频子带采用非线性变换进行增强;最后,使用NSCT逆变换重构图像的亮度分量,并将图像从YCbCr色彩空间模型还原到RGB空间得到增强后的图像。实验结果表明,算法增强效果明显优于同态滤波、空域PCNN及NSCT域的PCNN算法,不仅增加了彩色图像的明亮度,而且图像保真性好,纹理更清晰。     

基于噪声函数描述颜色纹理的方法

目前,对真实感图形的研究大多集中在物体的表面细节上。物体表面细节的表现,即纹理技术,是实现物体真实感的一个有效手段。纹理映射技术是描述颜色纹理最常用的方法。但是,当二维纹理映射到三维物体上时,会产生很大的变形。为此引入三维纹理技术,提出基于噪声函数描述颜色纹理的方法。此方法利用噪声扰动技术描述的颜色纹理与要表现对象的表面复杂性无关,解决了二维纹理映射所产生的纹理变形现象,使得要表现的对象在细节上更接近真实,最终取得整体上较佳的效果     

基于波形检测和颜色空间的车牌分割方法

车牌识别是智能交通中关键技术之一,车牌分割是车牌识别的基础。本文提出一种利用波检测和颜色空间相结合的车牌分割方法,克服了传统边缘检测阈值难以选择的缺点,并且不受光照变化和车牌掉色及磨损的影响,提供了车牌分割准确率     

中国海洋卫星技术成就与展望

利用卫星探测海洋已经成为国际海洋环境与生物资源探测的最有效手段。文章介绍了我国成功发射的海洋一号A星和B星的主要技术指标以及获得的重要应用成果,并展望了未来我国海洋卫星的后续发展。     

遥感卫星多光谱图像模拟真彩色算法研究

地球资源遥感卫星ZY-1 02C和CBERS-04搭载的全色多光谱相机缺少蓝光波段,需要通过波段模拟方法首先生成蓝波段,进而合成模拟真彩色图像。根据多光谱数据特点,提出一种基于波段线性关系模型的模拟真彩色方法。首先用具有蓝色波段的多光谱数据作为参考图像进行回归分析,计算得到相关系数,将结果作为参数应用于待模拟图像生成蓝波段。然后按照地物类别进行单景图像局部区域颜色畸变矫正。最后按特定顺序合成模拟真彩色图像。试验表明,该算法简单快速,减少了偏色现象,能够获得较好的模拟效果。     

姿控推进系统发动机关机的管路瞬变特性

从一维液体瞬变管路方程出发，采用有限差分格式的特征线方法，针对某姿控推进系统发动机真实氧化剂管路的关机瞬变特性进行了数值研究，对系统不同部位的动态特性进行了计算，喷注前的最大瞬变压力达到储箱压力的3倍，得到的结果与试车数据是一致的，对液体发动机管路工程设计具有参考价值，表明该方法可以方便地对包括许多管路，阀门和推力室的复杂系统进行动态特性分析。     

低温热水地板辐射采暖施工要点与能效分析

以中国矿业大学教师公寓小高层住宅项目为例,介绍了低温热水地面辐射采暖系统的特点及施工要点,并进行了能效分析,根据实际运行情况对该系统进行了分析和总结。达到了预期的设计目的,提高和改善了供暖使用功能,具有较高的推广价值。     

Investigation of Formation Process of the Chrome-free Passivation Film of Electrodeposited Zinc

The feasibility was investigated to substitute chrome-free passivation treatment of electrodeposited zinc in a titanium bath for chromate passivation treatment. The formation mechanism of the chrome-free passivation film was further analyzed. The surface mor- phologies and the elemental compositions of the treated samples with varied immersion times were observed by scanning electron mi- croscopy (SEM) and determined by energy dispersion spectrometry (EDS), respectively. The electrode potential of the sample surface was recorded in the film formation process. The changes of the electrode potential are in accordance with that of SEM and EDS of the sample surface. The results of X-ray photoelectron spectroscopy (XPS) show the chrome-free passivation film composed of ZnO, SiO2, TiO2, Zn4Si2O7(OH)2, and SrF2. The anode zinc dissolution and the local pH value increase due to the cathode hydrogen ion reduction process result in the formation of the chrome-free passivation film. The macro-images of the chrome-free passivation films formed on electrodeposited zinc show that the color of the film changes from blue to iridescence with the increase of the immersion times.     

Development of a GNSS water vapour tomography system using algebraic reconstruction techniques

A GNSS water vapour tomography system developed to reconstruct spatially resolved humidity fields in the troposphere is described. The tomography system was designed to process the slant path delays of about 270 German GNSS stations in near real-time with a temporal resolution of 30 min, a horizontal resolution of 40 km and a vertical resolution of 500 m or better. After a short introduction to the GPS slant delay processing the framework of the GNSS tomography is described in detail. Different implementations of the iterative algebraic reconstruction techniques (ART) used to invert the linear inverse problem are discussed. It was found that the multiplicative techniques (MART) provide the best results with least processing time, i.e., a tomographic reconstruction of about 26,000 slant delays on a 8280 cell grid can be obtained in less than 10 min. Different iterative reconstruction techniques are compared with respect to their convergence behaviour and some numerical parameters. The inversion can be considerably stabilized by using additional non-GNSS observations and implementing various constraints. Different strategies for initialising the tomography and utilizing extra information are discussed. At last an example of a reconstructed field of the wet refractivity is presented and compared to the corresponding distribution of the integrated water vapour, an analysis of a numerical weather model (COSMO-DE) and some radiosonde profiles.     

Report of the COSPAR mars special regions colloquium

In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > −25 °C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conservative nature of planetary protection, the following features constitute Mars Special regions: Gullies and bright streaks associated with them, pasted-on terrain, deep subsurface, dark streaks only on a case-by-case basis, others to be determined. The parameter definition and the associated list of physical features should be re-evaluated on a regular basis.