主成分分析法在地区综合实力评价中的应用

地区综合实力反映一个地区社会经济系统的发展水平。主成分分析法能够在保证原始数据信息损失最小的情况下,以少数的综合变量取代原有的多维变量,使数据结构大为简化,并且客观地确定权数,避免了主观随意性．因而是地区综合实力评价的一种有效方法。通过主成分分析,可以全方位地了解各个地区社会经济系统的发展水平及其差距。     

像元信息分解和决策树相结合的影像分类方法

该文提出了一种基于像元信息分解和决策树相结合的遥感自动分类方法。选择广州市番禺区作为研究区。用像元信息分解和多变量决策树法把TM影像分为水体、植被、水泥地、土壤4种基本组分,分离成4类树枝;分别以4种基本地物组分作为分类掩膜,采用BP神经网络分类、形状指数提取、光谱特征提取等复合方法进行分枝,并开展野外遥感调查,以提高和验证分类精度。结果表明：该方法保证了分枝时地物的纯洁度,有效地避免了地物提取时多余信息的干扰和影响,提高了分类精度。结合实地调查数据与最大似然分类算法进行对比实验,表明该模型比最大似然总体分类精度高16％。     

基于RS与GIS的三峡库区文物保护信息系统研究

举世瞩目的三峡水利枢纽工程的建设将为我国带来巨大的综合效益,同时由于水库水位的抬高,库区沿岸众多的文物古迹将部分或全部被永久淹没,为了研究文物保护工作的发掘技术与改进文物管理工作的手段,文章在分析三峡库区文物保护信息系统(TGRRPIS)的系统目标的基础上,探索了RS与GIS技术在文物保护领域应用的实用性,对三峡库区文物保护信息系统进行了尝试性的研究。     

GIS Platform-based Multi-source Information System for Evaluation of Cu, W and Au Resources in the Northern Qilian, China

Based on the information of geology, geochemistry, geophysics and remote sensing, the GIS of multi-source information is used to evaluate Cu, W and Au mineral resources in Northern Qilian, China. As the GIS evaluation system works out in the thinking of geological prospecting, its functions include file management, graph edition, database maintenance, information inquiry and comprehensive spatial analysis as well as prospecting target prognosis. Accordingly, the GIS evaluation system can be used directly and conveniently for inquiry and analysis of visual graphs or images.     

基于小波变换的遥感纹理信息提取

遥感纹理信息是地物空间特征的综合反映,综合纹理信息是进行专题信息提取获取的重要依据.遥感数据具有复杂性、统计性和随机性,同时,遥感图像中地学信息,如地质构造、蚀变信息及岩性分界等高频信息具有一定的方向性;小波变换具有"变焦性"、对称性、正则性等特点,可以较为快速地检测到奇变信号.利用小波变换可以快速、有效地提取遥感纹理高频奇变信息.     

On the extraction of extended structure from Herschel-SPIRE scanning observations in the presence of 1/f noise

We present results from a study of the impact of uncorrelated 1/ f noise on the extraction of spatial structure, on a range of scales, from sky mapping observations made using the Herschel-SPIRE (the spectral and photometric imaging receiver) photometer in the scan-map mode. These studies were carried out using a detailed instrument simulator, and the output reduced using the map-making algorithm to be implemented in the SPIRE data pipeline. The influence of source size scale, telescope-scanning rate and 1/ f noise knee frequency is investigated, and operational bounds to the expected losses are presented, using the case of zero 1/ f (white) noise as a benchmark. Both cross-linked and non-cross-linked observing options are studied. The results presented here represent the best current estimate of the sensitivity of the SPIRE photometer to emission on arbitrary scales. The data presented are general and scalable to any SPIRE observation made using the scanning mode.     

Periastron precession measurements in transiting extrasolar planetary systems at the level of general relativity

Transiting exoplanetary systems are surpassingly important among the planetary systems since they provide the widest spectrum of information for both the planet and the host star. If a transiting planet is on an eccentric orbit, the duration of transits T _D is sensitive to the orientation of the orbital ellipse relative to the line of sight. The precession of the orbit results in a systematic variation in both the duration of individual transit events and the observed period between successive transits,   P _obs  . The periastron of the ellipse slowly precesses due to general relativity and possibly the presence of other planets in the system. This secular precession can be detected through the long-term change in   P _obs  (transit timing variations, TTV) or in T _D (transit duration variations, TDV). We estimate the corresponding precession measurement precision for repeated future observations of the known eccentric transiting exoplanetary systems (XO-3b, HD 147506b, GJ 436b and HD 17156b) using existing or planned space-borne instruments. The TDV measurement improves the precession detection sensitivity by orders of magnitude over the TTV measurement. We find that TDV measurements over a approximately 4 yr period can typically detect the precession rate to a precision well exceeding the level predicted by general relativity.     

Observations of Low-Latitude Coronal Plumes

Using Fe ix/x 17.1 nm observations from the Extreme-Ultraviolet Imaging Telescope (EIT) on the Solar and Heliospheric Observatory (SOHO), we have identified many coronal plumes inside low-latitude coronal holes as they transited the solar limb during the late declining phase of cycle 23. These diffuse, linear features appear to be completely analogous to the familiar polar plumes. By tracking them as they rotate from the limb onto the disk (or vice versa), we confirm that EUV plumes seen against the disk appear as faint, diffuse blobs of emission surrounding a brighter core. When the EIT images are compared with near-simultaneous magnetograms from the SOHO Michelson Doppler Imager (MDI), the low-latitude, on-disk plumes are found to overlie regions of mixed polarity, where small bipoles are in contact with unipolar flux concentrations inside the coronal hole. The birth and decay of the plumes are shown to be closely related to the emergence of ephemeral regions, their dispersal in the supergranular flow field, and the cancellation of the minority-polarity flux against the dominant-polarity network elements. In addition to the faint polar and nonpolar plumes associated with ephemeral regions, we note the existence of two topologically similar coronal structures: the giant plume-like features that occur above active regions inside coronal holes, and the even larger scale “pseudostreamers” that separate coronal holes of the same polarity. In all three cases, the basic structure consists of open field lines of a given polarity overlying a photospheric region of the opposite polarity; ongoing interchange reconnection at the X-point separating the open field domains from the underlying double-arcade system appears to result in the steady evaporation of material from the closed into the open region.     

FITS图像处理技术荟萃及在太阳观测中的应用

针对FITS图像文件的特点,结合其在天文学领域的广泛应用,对其各种处理技术进行了简明扼要的介绍.包括FITS文件完整性的检查、文件头和数据内容的查看、图像特性的伪彩编码、文件格式的转换、数据的压缩及相关太阳物理信息的提取等内容.