Cluster Ages Experiment (CASE): SX Phe stars from the globular cluster ω Centauri     

A. Olech  W. A. Dziembowski  A. A. Pamyatnykh  J. Kaluzny  W. Pych  A. Schwarzenberg-Czerny  I. B. Thompson 《Monthly notices of the Royal Astronomical Society》2005,363(1):40-48

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Spot activity in the RS CVn binary UX arietis     

M. B. K. Sarma  B. V. N. S. Prakasa Rao 《Journal of Astrophysics and Astronomy》1984,5(2):159-168

Photoelectric observations of the RS CVn type non-eclipsing binary UX Arietis obtained at Nizamiah Observatory during the observing seasons of 1975–76, 1981–82 and 1982–83 are presented. The light curve of UX Ari showed a distortion wave with an amplitude inV varying from 0.02 mag during 1975–76 to 0.15 mag during 1982–83. An analysis of the available data shows that the light maximum is almost constant. It is also evident that the light-curve minimum decreases as the wave amplitude increases. The constant light at maximum,V = 6.51 ± 0.03 indicates the unspotted photospheric brightness. It is also suggested that the variation in meanV brightness is mainly due to spot activity and not due to intrinsic variation.  相似文献   

Standard cumulative semivariograms of stationary stochastic processes and regional correlation     

Zekâi Sen 《Mathematical Geology》1992,24(4):417-435

The standard cumulative semivariograms (SCS), obtained analytically from the currently employed stationary stochastic processes, provide a basis for the model identification and its parameter as well as regional correlation estimations. The analytical solutions for different stationary stochastic processes such as independent (IP), moving average (MA), autoregressive (AR), and autoregressive integrated moving average ARIMA (1,0,1) processes give rise to different types of SCSs which can be expressed in terms of the autocorrelation structure parameters only. The SCSs of independent and MA processes appear as linear trends whereas other type of processes have SCSs which are nonlinear for short distances but become linear at large distances. Irrespective of the stationary stochastic process type the linear portions of SCSs have unit slopes. The vertical distance between these linear portions and that of the IP cumulative semivariogram (CS), provide an indicator for measuring the regional correlation. In the case of stationary processes, the straight line portions of any CS are parallel to each other. Hence, it is possible to identify the model from the sample CS. Finally, necessary procedures are provided for the model parameters estimation. The methodology developed, herein, is applied to some hydrochemical ions in the groundwater of the Wasia aquifer in central part of Kingdom of Saudi Arabia.  相似文献   

Elements of spin motion     

Toshio Fukushima  Hideharu Ishizaki 《Celestial Mechanics and Dynamical Astronomy》1994,59(2):149-159

For use in numerical studies of rotational motion, a set of elements is introduced for the torque-free rotational motion of a rigid body around its barycenter. The elements are defined as the initial values of a modification of the Andoyer canonical variables. A computational procedure is obtained for determining these elements from the combination of the spin angular momentum vector and a triad defining the orientation of the rigid body. A numerical experiment shows that the errors of transformation between the elements and variables are sufficiently small. The errors increase linearly with time for some elements and quadratically for some others.  相似文献   

因子分析中变量和样品空间的统一     

岑况 《地质科技情报》1994,13(4):93-97

以空间结构分析为基础，提出了一个统一的变量和样品空间，由此得到因子空间，依据因子空间中变量和样品的相关性，很容易确定样品点群的成因，还讨论了因子分析中变量坐标和样品坐标的概念，指出因子得分不是样品的坐标，因而把因子得分图看作为因子空间坐标图是不合适的。  相似文献   

岩土参数的空间变异性分析   总被引：4，自引：0，他引：4  

徐超  杨林德 《上海国土资源》1996,(4):16-19

岩土参数具有空间变异性和不确定性,本文将岩土参数视为具有随机性和结构性的区域化变量,利用区域化变量理论和地质统计方法分析上海地基土有代表性的抗剪强度指标的空间变异特性。结果表明该方法是可行的。  相似文献   

用多变量时间序列相关模型预测矿井涌水量   总被引：3，自引：0，他引：3  

杨永国  谢克俊 《煤田地质与勘探》1995,23(6):38-42

运用多变量时间序列分析方法，建立了南桐煤矿二井的涌水量与降雨量之间的相关模型，并将其用于矿井涌水量的预测，结果表明，南桐二井涌水量与降雨量呈滞后一个月、三个月和三年的关系，预测结果与实测值对比分析表明，本模型的预测结果精度较高。  相似文献   

大青沟国家自然保护区地面苔藓植物分布格局   总被引：1，自引：1，他引：0  

田桂泉  韩淑美  苏日古嘎 《中国沙漠》2018,38(3):545-552

用双向指示种分析（TWINSPAN）、除趋势对应分析（DCA）和典范对应分析（CCA）研究了大青沟国家自然保护区32个样地36种地面生苔藓植物分布格局。TWINSPAN和DCA分析结果显示,地面生苔藓植物群落可以分成双色真藓（Bryum bicolor）-小石藓（Weissia controversa）群落、西伯利亚瘤冠苔（Mannia sibirica）+小石藓（Weissia controversa）群落、密叶绢藓短柄变种（Entodon compressus var.zikaiwiensis）-密叶绢藓（Entodon compressus）+反扭藓（Timmiella anomala）群落、绒叶青藓（Brachythecium velutinum）-鳞叶藓（Taxiphyllum taxirameum）+尖叶匐灯藓（Plagiomnium cuspidatum）群落和地钱（Marchantia polymorpha）+曲肋薄网藓（Leptodictyum humile）-鳞叶藓（Taxiphyllum taxirameum）-柳叶藓（Amblystegium serpens）+平肋提灯藓（Mnium laevinerve）群落5组,对应分布在羊草（Leymus chinensis）草地、西伯利亚杏（Prunus sibirica）灌丛、大果榆（Ulmus macrocarpa）林、蒙古栎（Quercus mongolica）林和水曲柳（Fraxinus mandschuria）林。CCA分析结果显示,影响苔藓植物分布的主要因子有土壤水分、乔木盖度、空气湿度、凋落物盖度、草本层盖度等。  相似文献   

Evidence for pole switching in the magnetic cataclysmic variable BY Camelopardalis     

Paul A. Mason  Gavin Ramsay  Ivan Andronov  Sergey Kolesnikov  Nickolay Shakhovskoy  & Elana Pavlenko 《Monthly notices of the Royal Astronomical Society》1998,295(3):511-518

An analysis of X-ray and optical light curves of the magnetic cataclysmic variable (MCV) BY Cam is presented. This system is one of three MCVs in which the spin period of the white dwarf and the binary orbital period differ by ∼1 per cent. As such these 'BY Cam' stars are important objects with which to probe the field structure of the magnetic white dwarf and ultimately the nature of synchronization of AM Her binaries. We confirm asynchronous rotation of the magnetic white dwarf with respect to the binary. We find evidence that the accretion stream accretes directly on to the white dwarf as in AM Her systems, but further, the stream impacts on to different magnetic poles over the course of the beat period. We present evidence that the optical and hard X-ray light curves modulate in phase, but together they are out of phase with the soft X-ray light curve. We confirm the spin down of the white dwarf which is expected to lead to the synchronization of the spin and orbital periods of BY Cam.  相似文献   

Radiation-driven winds from luminous accretion discs     

Daniel Proga  James M. Stone  & Janet E. Drew 《Monthly notices of the Royal Astronomical Society》1998,295(3):595-617

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