Point-block covariance: A general solution for the two-dimensional stationary random functions     

T. R. P. Singh 《Mathematical Geology》1976,8(6):627-634

The application of the theory of random functions to problems of ore evaluation may involve computations of the covariance between the mean value of a given block and the functional value at a given point. However, an analytical solution for such a covariance does not exist for nonspherical blocks and for commonly applied models of covariance functions. Further, because this covariance is a function of the spatial arrangements of the block and the point, it has to be evaluated numerically each time for given point—block arrangements. This paper presents a readily available general solution to this problem in the form of a series of graduated curves which, together with some geometric manipulations, may be used to compute the covariance between a pointand a two-dimensional block for all possible point—block arrangements. The availability of the graph thus eliminates the necessity of using the time-absorbing programs on computers for such computations. Finally, many of the approximations that are made in order to avoid cumbersome covariance evaluations are no longer necessary due to the ease of such computations with the help of the graph provided.  相似文献   

Some methods for statistical analysis of multimodal distributions and their application to grain-size data   总被引：1，自引：0，他引：1  

Malcolm W. Clark 《Mathematical Geology》1976,8(3):267-282

Some of the methods used in the resolution of mixed normal distributions are discussed under three headings: analytical, graphical, and numerical methods. Attention is given to their applicability in the analysis of grain-size data as derived from sieving. Comparisons are made by applying several methods to published data. It is concluded that the numerical methods offer most scope, especially the method of nonlinear least squares. Some analyses of beach sediments, using this method, are presented. The adoption of a convention for the number of individuals in the sample increases ease of interpretation.  相似文献   

Correlations among color,morphology, and luminosity for the luminous red galaxy (LRG) sample of the SDSS data release 5     

Xin-Fa Deng  Ji-Zhou He  Peng Jiang  Ping Wu  Xiao-Xia Qian 《Astrophysics》2007,50(3):273-282

We have investigated the correlations among color, morphology and luminosity for all LRGs, cut I LRGs, cut II LRGs, and Main galaxies that are also classified as LRGs. It is found that the morphology of LRGs is tightly correlated with luminosity. The rest-frame u-g color of cut I LRGs and cut II LRGs is nearly independent of luminosity, but the color of Main galaxies is correlated with luminosity. For cut I LRGs and Main galaxies, the early type proportion apparently changes with color: at the rest-frame u-g < 1.3 it increases strongly with increasing color, while at the rest-frame u-g > 1.3 it decreases with increasing color. We also notice that the morphology of cut II LRGs is only a weak function of color. Published in Astrofizika, Vol. 50, No. 3, pp. 335–345 (August 2007).  相似文献   

Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in the Spitzer First Look Survey Field     

Xiao-Qing Wen    Hong Wu  Chen Cao  Xiao-Yang Xia  Department of Physics  Tianjin Normal University  Tianjin National Astronomical Observatories  Chinese Academy of Sciences  Beijing   《中国天文和天体物理学报》2007,7(2):187-198

We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506.  相似文献   

Thermodynamics of rare events and impulsive relaxation events in the magnetospheric substorm dynamics     

Giuseppe Consolini  Matthieu Kretzschmar 《Planetary and Space Science》2007,55(15):2244-2250

The magnetosphere dynamics shows fast relaxation events following power-law distribution for many observable quantities during magnetic substorms. The emergence of such power-law distributions has been widely discussed in the framework of self-organized criticality and/or turbulence. Here, a different approach to the statistical features of these impulsive dynamical events is proposed in the framework of the thermodynamics of rare events [Lavenda, B.H., Florio, A., 1992. Thermodynamics of rare events, Int. J. Theor. Phys. 31, 1455–1475; Lavenda, B.H., 1995. Thermodynamics of Extremes. Albion]. In detail, an application of such a novel approach to the magnetospheric substorm avalanching dynamics as monitored by the auroral electroject index is discussed.  相似文献   

Statistical analysis of galaxy surveys – III. The non-linear clustering of red and blue galaxies in the 2dFGRS     

Darren J. Croton  Peder Norberg  Enrique Gaztañaga  Carlton M. Baugh 《Monthly notices of the Royal Astronomical Society》2007,379(4):1562-1570

We present measurements of the higher order clustering of red and blue galaxies as a function of scale and luminosity made from the two-degree field galaxy redshift survey (2dFGRS). We use a counts-in-cells analysis to estimate the volume-averaged correlation functions,     , as a function of scale up to the order of   p = 5  , and also the reduced void probability function. Hierarchical amplitudes are constructed using the estimates of the correlation functions:     . We find that (i) red galaxies display stronger clustering than blue galaxies at all orders measured; (ii) red galaxies show values of   S _p   that are strongly dependent on luminosity whereas blue galaxies show no segregation in   S _p   within the errors; this is remarkable given the segregation in the variance; (iii) the linear relative bias shows the opposite trend to the hierarchical amplitudes, with little segregation for the red sequence and some segregation for the blue; (iv) faint red galaxies deviate significantly from the 'universal' negative binomial reduced void probabilities followed by all other galaxy populations. Our results show that the characteristic colour of a galaxy population reveals a unique signature in its spatial distribution. Such signatures will hopefully further elucidate the physics responsible for shaping the cosmological evolution of galaxies.  相似文献   

激光雷达点云电力线自动提取算法     

李德友  李彩林  李祥珅  王柏涛 《测绘通报》2021,(6):33-38

针对当前电力线提取方法自动化程度和精度不高的问题,本文从点云数据的空间分布特征出发,提出了一种高效的电力线自动提取方法。首先基于自然裂点法,将点云数据按高程分类后去除地面点;然后对数据进行空间划分,基于子空间的点密度及空间结构特征的差异化,利用地物分割算法去除电塔点和残留的植被点;最后利用基于欧氏距离分割的电力线自动检测算法,实现单根电力线的快速、高精度提取。提取结果和拟合试验表明,该方法能在复杂地形下实现电力线的自动提取,极大提高了电力线的提取效率和精度。  相似文献   

黄淮地区夏季日降水分区概率预报方法研究     

赵琳娜  董航宇  吴亮  王彬雁  白雪梅  党皓飞 《气象》2015,41(12):1503-1513

利用我国黄淮地区1961—2010年50年6—8月的日降水资料,采用REOF和t检验的方法,将中国黄淮地区夏季降水分成Ⅰ—Ⅴ区。5个区域进行差异性t检验表明5个区域之间（彼此）差异显著,说明了区域划分的正确性。在此基础上利用1999—2007年6—8月站点日降水资料以及CFSv2模式后预报的日降水资料建立了5个区域内共5个代表站点的夏季日降水概率预报方程,并进行了确定性、概率性预报检验和业务试用检验。对各区域内5个代表站日降水量的确定性预报检验表明：Logistic回归降水概率预报方程的TS评分要高于CFSv2模式预报和T213的集合预报平均,空报率也低于CFSv2模式预报和T213集合预报平均,但是漏报率却略高。各区域代表站日降水量的概率预报Brier评分检验表明：Brier评分均不超过0.2,大大低于T213集合预报所得概率预报的Brier评分分值,说明本文Logistic回归方程的概率预报较为可靠。Brier技巧评分表明：Logistic回归降水概率预报方程各站的BSS技巧评分都大于0.0,说明各站的预报技巧高于检验样本气候概率的预报技巧,且高于T213集合预报的Brier技巧评分,说明在分区基础上建立Logistic回归降水概率预报方程的方法是有预报意义的。  相似文献   

The evolution of the z distribution of normal neutron stars in the Galaxy     

Y.‐C. Wei  C.‐M. Zhang  Y.‐H. Zhao  Q.‐H. Peng  X.‐J. Wu  J. Wang  Y.‐Y. Pan  H.‐X. Yin  Y. Yan  T.‐S. Yan  H.‐J. Tian  A. Esamdin  A.L. Luo  Y. Cai  A. Taani 《Astronomische Nachrichten》2010,331(8):817-831

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

洪水频率分析的次序统计量   总被引：1，自引：1，他引：0       下载免费PDF全文

刘九夫  谢自银  鲍振鑫  朱元甡 《水科学进展》2010,21(2):179-187

系统阐述了洪水频率分析涉及的洪水次序统计量和广义次序统计量及其抽样分布,并通过数学实验和统计试验两种途径研究了洪水次序统计量、频率次序统计量和重现期次序统计量抽样分布的统计特征及其关系。研究得到的次序统计量和广义次序统计量抽样分布的期望值和中值关系为系统分析和评价适线法奠定了理论基础。  相似文献