基于数字地价模型的地价监测点配置研究   总被引：1，自引：0，他引：1  

胡石元  李德仁  刘耀林 《武汉大学学报(信息科学版)》2007,32(9):838-841

从数字地价模型的建立、格网数字地价模型向TIN转化、TIN节点与宗地图层叠加拟合完成地价监测点的定位配置、结合市场比较法的监测点地价更新、TIN数字地价模型更新等几个方面详细阐述了数字地价模型运用于地价监测点配置的具体方法。并将这一配置模式与以标准宗地为载体的配置模式进行了比较分析。  相似文献   

基于决策树的高光谱数据特征选择及其对分类结果的影响分析   总被引：2，自引：0，他引：2  

王圆圆  李京 《遥感学报》2007,11(1):69-76

本文利用OM IS高光谱数据,研究了决策树算法（Decision Tree,DT）特征选择的特点以及特征选择对决策树分类结果的影响。设计了三种特征选择方法：SEP,MDLM和RELIEF,将它们与DT特征选择的结果以及特征选择后的分类精度（考虑了三种分类器：最大似然法、后向传播神经网络、最邻近法）进行对比,并分析了这三种特征选择方法对决策树结构和分类精度的影响。结果显示,DT是一种比较好的特征选择方法;经过特征选择后再生成的决策树比直接生成的决策树,用到更少的特征（平均减少了43.36%）、有更多的节点（平均增加了18.61%）和更高的分类精度（平均提高了0.35%）,当样本数量少时,分类精度的提高幅度最大,而树的大小却基本没有增加。  相似文献   

MODIS与TM冬小麦种植面积遥感测量一致性研究——小区域实验研究   总被引：5，自引：1，他引：5  

顾晓鹤  潘耀忠  朱秀芳  张锦水  韩立建  王双 《遥感学报》2007,11(3):350-358

针对大范围冬小麦种植面积遥感测量业务化运行中所存在的不同空间分辨率遥感影像的获取能力、空间分辨率与测量精度之间相互制约的现实问题,选择典型实验区,采取全覆盖的多时相低分辨率MODIS数据与中高分辨率TM样区数据相结合的方法,以支持向量机（SVM）为主要技术手段,通过选取不同比例的TM样本量,对MODIS进行混合像元分解,并对MODIS冬小麦测量结果与TM测量结果进行一致性分析,进而提出了一套可用于大范围冬小麦种植面积遥感测量业务化推广的识别和精度检验方法。研究结果表明：当TM样本量大于5%时,相对于TM识别结果而言,MODIS像元精度可以稳定在82%以上;当TM样本量大于40%时,区域精度可以稳定在97%。因此,从理论上讲,在实际业务化运行中,只要能够获得监测区40%的中高分辨率的影像,采用本研究提出的多尺度冬小麦种植面积测量方法,基本上可以满足业务化运行的精度要求。  相似文献   

武汉台形变观测与降雨参数之间的定量分析与研究          下载免费PDF全文

吕琳  杨艳芳  舒德亮 《地震工程学报》2020,42(1):136-142

基于“前兆台网(站)观测数据跟踪分析平台”,对武汉台形变观测资料进行了系统分析,提取出观测曲线受降雨干扰影响的事件,采用降雨总量、初始驱动降雨量和瞬时降雨量最大值等降雨参数对降雨干扰事件进行统计分析。结果表明:降雨总量达40 mm、初始驱动降雨量为0.3 mm或瞬时降雨量最大值达0.6 mm时,DSQ型水管倾斜仪易受降雨干扰;SSY型铟瓦棒伸缩仪当降雨总量超60 mm或瞬时降雨量最大值大于0.5 mm时易受降雨干扰;VS型垂直摆倾斜仪受降雨干扰与降雨总量、初始驱动降雨量和瞬时降雨量最大值无显著相关关系;降雨总量对形变仪器观测物理量的影响基本呈现线性;而形变仪器观测物理量与初始驱动降雨量、瞬时降雨量最大值无显著相关关系。认为武汉台形变观测受降雨影响主要来自降雨渗透影响和周边水体荷载变化影响两个方面。  相似文献   

DO WE NEED TO MODEL PLATES AT ALL?   总被引：2，自引：0，他引：2  

Morrison  Smart  & Taff 《Monthly notices of the Royal Astronomical Society》1998,296(1):66-76

The historical method of obtaining equatorial coordinates for stars observed via astronomical photography has been to convert the measured coordinates to equatorial coordinates with the aid of a plate model which corrects for a variety of effects. However, we now have at our disposal novel smoothing techniques, of considerable generality, which in conjunction with modern star catalogues can reproduce the essence of the plate model while dramatically minimizing both the fortuitous and systematic errors of observation. In this paper we demonstrate that, with this technique and extant catalogues, one can obtain, with at least the same precision and better accuracy, the information necessary to transform the measured coordinates successfully into standard coordinates by a process that involves no sophisticated model for the plate. Using external checks we estimate the increase in accuracy to be of the order of 25 per cent.  相似文献   

An optimal extraction algorithm for imaging photometry     

Tim Naylor 《Monthly notices of the Royal Astronomical Society》1998,296(2):339-346

This paper is primarily an investigation of whether the 'optimal extraction' techniques used in CCD spectroscopy can be applied to imaging photometry. It is found that using such techniques provides a gain of around 10 per cent in signal-to-noise ratio over normal aperture photometry. Formally, it is shown to be equivalent to profile fitting, but offers advantages of robust error estimation, freedom from bias introduced by mis-estimating the point spread function, and convenience. In addition some other techniques are presented, which can be applied to profile fitting, aperture photometry and the 'optimal' photometry. Code implementing these algorithms is available at http://www.astro.keele.ac.uk/~timn/.  相似文献   

Non-parametric reconstruction of distribution functions from observed galactic discs     

C. Pichon  & E. Thiébaut 《Monthly notices of the Royal Astronomical Society》1998,301(2):419-434

A general inversion technique for the recovery of the underlying distribution function for observed galactic discs is presented and illustrated. Under the assumption that these discs are axisymmetric and thin, the proposed method yields a unique distribution compatible with all the observables available. The derivation may be carried out from the measurement of the azimuthal velocity distribution arising from positioning the slit of a spectrograph along the major axis of the galaxy. More generally, it may account for the simultaneous measurements of velocity distributions corresponding to slits presenting arbitrary orientations with respect to the major axis. The approach is non-parametric, i.e. it does not rely on a particular algebraic model for the distribution function. Special care is taken to account for the fraction of counter-rotating stars, which strongly affects the stability of the disc. An optimization algorithm is devised — generalizing the work of Skilling &38; Bryan — to carry this truly two-dimensional ill-conditioned inversion efficiently. The performance of the overall inversion technique with respect to the noise level and truncation in the data set is investigated with simulated data. Reliable results are obtained up to a mean signal-to-noise ratio of 5, and when measurements are available up to 4  R _e. A discussion of the residual biases involved in non-parametric inversions is presented. The prospects of application of the algorithm to observed galaxies and other inversion problems are discussed.  相似文献   

Automated classification of stellar spectra — II. Two-dimensional classification with neural networks and principal components analysis     

Coryn A. L. Bailer-Jones  Mike Irwin  & Ted von Hippel 《Monthly notices of the Royal Astronomical Society》1998,298(2):361-377

We investigate the application of neural networks to the automation of MK spectral classification. The data set for this project consists of a set of over 5000 optical (3800–5200 Å) spectra obtained from objective prism plates from the Michigan Spectral Survey. These spectra, along with their two-dimensional MK classifications listed in the Michigan Henry Draper Catalogue, were used to develop supervised neural network classifiers. We show that neural networks can give accurate spectral type classifications (σ₆₈= 0.82 subtypes, σ_rms= 1.09 subtypes) across the full range of spectral types present in the data set (B2–M7). We show also that the networks yield correct luminosity classes for over 95 per cent of both dwarfs and giants with a high degree of confidence.   Stellar spectra generally contain a large amount of redundant information. We investigate the application of principal components analysis (PCA) to the optimal compression of spectra. We show that PCA can compress the spectra by a factor of over 30 while retaining essentially all of the useful information in the data set. Furthermore, it is shown that this compression optimally removes noise and can be used to identify unusual spectra.   This paper is a continuation of the work carried out by von Hippel et al. (Paper I).  相似文献   

西南极菲尔德斯半岛地壳形变监测的数据处理与分析          下载免费PDF全文

陈春明  鄂栋臣  邱卫宁 《极地研究》1998,10(1):74-79

为了研究南极现代地壳运动,中国在西南极菲尔德斯海峡地区布设了形变监测网,并用ＤＩ－２０测距仪和ＧＰＳ定位仪对该网进行了监测。同时,中国也参加了ＳＣＡＲ组织的全南极ＧＰＳ联测。本文讨论了将形变参数纳入误差方程的水平形变数据处理方法,并对刚体平移、旋转、均匀应变几种典型形变模型在测边网平差中的运用进行了讨论。通过对经典自由网与秩亏自由网的基准分析,提出对形变参数以及其它附加参数和点位参数分别给定参考基准的方法。相应于上述方法,编制了一系列数据处理程序并将之应用于对西南极菲尔德斯海峡形变监测网的数据分析。本文还利用监测网应变分析原理,对ＧＰＳ监测数据进行了讨论和分析,结果表明,菲尔德斯断裂地区存在微小的断裂剪切运动,但位移量不大。  相似文献   

GIS中多幅地图的缩放漫游及其数据组织   总被引：1，自引：0，他引：1  

赵仁亮 《四川测绘》1998,21(4):151-155

本文在分析现存GIS软件中处理多幅不同比例尺或相同比例尺地图的放缩漫游时的不足及其原因的基础上,提出了一种使用地理逻辑窗口动态裁剪快速而安全的多幅地图无级缩放和全区域自由漫游的方法,并对其数据组织和管理作了探讨。  相似文献