基于小波变换的周跳探测与修复   总被引：2，自引：1，他引：1  

张金华  胡伍生 《测绘工程》2009,18(4):24-27

探测和修复周跳一直是GPS定位中的关键问题。利用小波变换对相位减伪距观测量进行周跳探测。首先介绍小波变换周跳探测的一般方法，然后在此基础上提出改进。改进方法可以对周跳进行探测和直接修复，进而探测和修复多次周跳，同时有效地克服一般方法可能出现探测失误的缺点。这种改进方法的效果在实验中得到验证。  相似文献   

风场反演中距离圈上速度退模糊方法研究   总被引：3，自引：0，他引：3  

周鑫  汤志亚  郭在华 《成都信息工程学院学报》2009,24(3)

在深入分析速度模糊的特点后,根据在距离圈上不模糊点到模糊点的不连续性,以及对模糊跳变处风速差和最大不模糊速度间关系的判定,从零方位开始在距离圈上逐点进行速度模糊的判定,并引入模糊标记的形式以确定退模糊处理的区间.然后通过实例分析,证明了方法的可用性和正确性.最后利用经过该方法处理的低仰角基本速度资料成功反演了雷达风场.  相似文献   

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张凌空  牛安福 《大地测量与地球动力学》2009,29(5):33-37

?о??????Sacks??????????????????????????????????????о??й????????????????????????о???????????????????????????????????о????????????????????????????6?Sacks??????????ε?????????????????????????????伫??????????????????????????????  相似文献   

船舶监控系统中航迹线动态绘制算法应用研究     

张峰  李四海  刘金 《海洋测绘》2008,28(3):68-71

在船舶监控系统中应用3S技术，实现了船只航迹线的动态绘制，系统能够根据船只航行方向动态显示航行轨迹，程序开发过程中涉及到偏转角度算法和距离插值两个核心算法。实践表明，这两个算法的合理应用，在航迹线可视化表现方面取得了良好的效果。  相似文献   

IDM模型分析及其影响力改进算法     

石矛  方勇  曾祥平  王长辉 《成都信息工程学院学报》2008,23(1):69-72

影响力传播模型IDM用于挖掘和分析BBS上观点领袖以及热门话题,它主要以影响力作为衡量标准。通过简化影响力运算法则,对IDM模型进行改进,使其更加直观。此改进后的IDM模型可运用到社会网络中,能更深刻的揭示出社会网络中各通信个体间的相互影响和距离,从而更好地了解和研究社会网络。  相似文献   

基于地理信息的大型场馆区域人员疏散模型设计     

王若晶  蔡先华 《测绘信息与工程》2009,34(2):23-25

采用了Geodatabase空间数据模型，建立了地理信息数据库，设计了基于地理信息的人员疏散模型。  相似文献   

Velocity Distance of the Open Cluster M11     

Jun-Liang Zhao Li Chen 《中国天文和天体物理学报》2007,7(4):572-578

On the reasonable hypothesis that the internal motions of member stars of a cluster are random and isotropic, a method which can be used to estimate the velocity distance of the cluster and its uncertainty is developed. The velocity distance so determined is an absolute distance estimate, and is completely independent of the (widely used) luminosity distance, which is a relative distance estimate. Using the published high-accuracy observational data of radial velocities and proper motions of the stars in the open cluster M11 region, we have determined the distance of M11 to be 1.89 ± 0.52kpc. This is in quite good agreement with the published luminosity distances of the cluster. We briefly discuss the problems concerned, including the sources of errors in the method and its applicable range.  相似文献   

Hydroclimatic teleconnection between global sea surface temperature and rainfall over India at subdivisional monthly scale     

Rajib Maity  D. Nagesh Kumar 《水文研究》2007,21(14):1802-1813

It is well established that sea surface temperature (SST) plays a significant role in the hydrologic cycle in which precipitation is the most important part. In this study, the influence of SST on Indian subdivisional monthly rainfall is investigated. Both spatial and temporal influences are investigated. The most influencing regions of sea surface are identified for different subdivisions and for different overlapping seasons in the year. The relative importance of SST, land surface temperature (LST) and ocean–land temperature contrast (OLTC) and their variation from subdivision to subdivision and from season to season are also studied. It is observed that LST does not show much similarity with rainfall series, but, in general, OLTC shows relatively higher influence in the pre‐monsoon and early monsoon periods, whereas SST plays a more important role in late‐ and post‐monsoon periods. The influence of OLTC is seen to be mostly confined to the Indian Ocean region, whereas the effect of SST indicates the climatic teleconnection between Indian regional rainfall and climate indices in Pacific and Atlantic Oceans. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

光栅栅距检测与线阵CCD细分技术研究     

杨博雄  周云耀  刘海波  陈志高  欧同庚  郑勇 《大地测量与地球动力学》2007,27(Z1):143-145

利用线阵CCD分辨率高、像素均匀等特点对光栅莫尔条纹进行细分是目前广泛采用的一种新技术。由于CCD具有自扫描能力，能将光强随空间分布的莫尔条纹信号转换成随时间变化的电信号，从而可以对光栅刻线的像的移动进行精确定位和直接数字化，改变传统莫尔条纹位相细分方法，实现对光栅栅距进行高倍数的细分。  相似文献   

Cepheid parallaxes and the Hubble constant   总被引：1，自引：0，他引：1  

Floor van Leeuwen  Michael W. Feast  Patricia A. Whitelock  Clifton D. Laney 《Monthly notices of the Royal Astronomical Society》2007,379(2):723-737

Revised Hipparcos parallaxes for classical Cepheids are analysed together with 10 Hubble Space Telescope ( HST )-based parallaxes. In a reddening-free V , I relation we find that the coefficient of log  P is the same within the uncertainties in our Galaxy as in the Large Magellanic Cloud (LMC), contrary to some previous suggestions. Cepheids in the inner region of NGC 4258 with near solar metallicities confirm this result. We obtain a zero-point for the reddening-free relation and apply it to the Cepheids in galaxies used by Sandage et al. to calibrate the absolute magnitudes of Type Ia supernova (SNIa) and to derive the Hubble constant. We revise their result for H ₀ from 62 to 70 ± 5 km s⁻¹ Mpc⁻¹. The Freedman et al. value is revised from 72 to 76 ± 8 km s⁻¹ Mpc⁻¹. These results are insensitive to Cepheid metallicity corrections. The Cepheids in the inner region of NGC 4258 yield a modulus of 29.22 ± 0.03 (int.) compared with a maser-based modulus of 29.29 ± 0.15. Distance moduli for the LMC, uncorrected for any metallicity effects, are 18.52 ± 0.03 from a reddening-free relation in V , I ; 18.47 ± 0.03 from a period–luminosity relation at K ; 18.45 ± 0.04 from a period–luminosity–colour relation in J , K . Adopting a metallicity correction in V , I from Macri et al. leads to a true LMC modulus of 18.39 ± 0.05.  相似文献