Estimate of the alpha parameter in an oat crop under rain‐fed conditions     

Facundo Carmona  Raúl Rivas  Vicente Caselles 《水文研究》2013,27(19):2834-2839

In this article, we estimated the alpha parameter of the Priestley–Taylor model under rain‐fed conditions. This study was conducted in an oat crop, from 7 September to 22 October 2009, in a region of subhumid plains (Tandil, Argentina). An energy balance station was installed within the experimental field to monitor its development. The alpha parameter value obtained was 1.41 ± 0.01, which led to an overestimation of the evapotranspiration of just 2% and a relative error in estimating evapotranspiration of 8%. The results suggest that the alpha parameter obtained is adequate in estimating the evapotranspiration of oat crops or similar crops in subhumid plains of Buenos Aires, Argentina. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

The Austin Chalk-Taylor Clay succession in Texas and the Santonian-Campanian boundary     

P. Marks  B. Stam 《Cretaceous Research》1983,4(3):271-279

Re-evaluation of samples from several Texas localities over the Austin Chalk-Taylor Clay boundary for planktic Foraminifera, and comparison with recent work on European and North African successions confirms the general correlation of the Texan formations with the European Stage succession. The sedimentary hiatus indicated by Pessagno (1967) does not appear to be present: the Late Santonian-Early Campanian zonal marker Globigerinita elevata (Brotzen) occurs in the Lower Taylor Clay associated with late representatives of Marginotruncana. The Lower Taylor Clay may belong to the Late Santonian in some localities.  相似文献   

The effects of buoyant crust on the gravitational instability of thickened mantle lithosphere at zones of intracontinental convergence   总被引：1，自引：0，他引：1  

Peter Molnar  Gregory A. Houseman 《Geophysical Journal International》2004,158(3):1134-1150

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1980年代中国地磁正常场图及其数学模式   总被引：6，自引：13，他引：6       下载免费PDF全文

夏国辉  郑双良  吴莉兰  张凤玉  魏宏 《地球物理学报》1988,31(1):82-89

本文介绍了1980.0年中国地磁正常场图的编绘和地磁正常场数学模式的建立使用不同年代观测的地磁三要素资料2000余个,经过通化改正,统统改正到1980.0这个特定年代。采用泰勒多项式和最小二乘法,分别建立1980.0年中国地磁正常场和地磁场长期变化数学模式,并计算其网格值,用于编绘1980.0年中国地磁正常场图。本文在建立地磁正常场数学模式时,采用三个独立的地磁要素建立模式的方法,解决了地磁场模式在地磁倾角为零的地方、而垂直强度不为零的问题。  相似文献   

A survey of numerical methods for stochastic differential equations     

P. E. Kloeden  E. Platen 《Stochastic Environmental Research and Risk Assessment (SERRA)》1989,3(3):155-178

The development of numerical methods for stochastic differential equations has intensified over the past decade. The earliest methods were usually heuristic adaptations of deterministic methods, but were found to have limited accuracy regardless of the order of the original scheme. A stochastic counterpart of the Taylor formula now provides a framework for the systematic investigation of numerical methods for stochastic differential equations. It suggests numerical schemes, which involve multiple stochastic integrals, of higher order of convergence. We shall survey the literature on these and on the earlier schemes in this paper. Our discussion will focus on diffusion processes, but we shall also indicate the extensions needed to handle processes with jump components. In particular, we shall classify the schemes according to strong or weak convergence criteria, depending on whether the approximation of the sample paths or of the probability distribution is of main interest.  相似文献   

东亚地磁场模型的计算与分析   总被引：4，自引：0，他引：4       下载免费PDF全文

安振昌  N.M.Rotanova 《地球物理学报》2002,45(1):34-41

根据中国、前苏联和蒙古等地区的地磁复测点和地磁台站资料,使用泰勒多项式方法和冠谐分析方法,计算东亚地磁场(X,Y,Z)的泰勒多项式模型和冠谐模型,以及东亚剩余磁场(ΔX,ΔY,ΔZ)的冠谐模型和泰勒多项式模型,并绘制了相应的理论地磁图. 泰勒多项式模型的展开原点位于45°N和100°E,截断阶数为7.地磁场泰勒多项式模型的均方偏差为:X分量是133.0nT,Y分量是107.4nT,Z分量是14.0nT. 球冠极点位于45°N和100°E,球冠半角为42°,冠谐模型的截断阶数为10. 剩余磁场冠谐模型的均方偏差分别为131.2nT(ΔX),112.6nT(ΔY)和13.7nT(ΔZ). 对比分析了上述两种模型. 提出了确定区域模型截断阶数的判据.  相似文献   

2003年中国及邻区地磁场模型的计算与分析   总被引：11，自引：3，他引：8  

顾左文  安振昌  高金田  詹志佳  姚同起  韩炜  陈斌 《地震学报》2006,28(2):141-149

根据2003年中国地区的135个测点和35个台站的地磁数据, 建立了2003年中国及邻区地磁场泰勒多项式模型和球冠谐模型. 在模型计算过程中, 细致地分析了模型的截断阶数和边界约束对模型计算的影响. 结果表明, 所使用的地磁观测资料是准确可靠的, 模型截断阶数的选取是合理的. 本文所建立的中国区域地磁场球冠谐模型与泰勒多项式模型具有良好的一致性.   相似文献   

Experimental investigation of stratorotational instability using a thermally stratified system: instability,waves and associated momentum flux     

T. Seelig  M. Gellert 《地球物理与天体物理流体动力学》2018,112(4):239-264

Stratorotational instability (SRI) has been proposed as a mechanism for outward angular momentum transport in Keplerian accretion disks. A particular designed Taylor–Couette laboratory experiment with axial stratification is suitable for studying the instability. Bottom endplate is cooled and top endplate is heated to achieve axial stratification. Due to constructive constraints, endplates are visually unamenable and quantitative measurement techniques in the co-rotating frame can only be done by looking through the outer cylinder. For this purpose, we built a co-rotating mini-PIV (Particle Image Velocimetry) system with a camera having a tilted viewing angle regarding the horizontal laser sheet. The aim of this study is (i) to quantify the uncertainty of the mini-PIV together with the used calibration technique and (ii) to compare experimental findings on SRI with theoretical predictions.

We perform measurements of the azimuthal and radial component of the velocity in axial stably stratified Taylor–Couette flows, consider velocity profiles and do frequency-filtering and flow decomposition. The absolute error of the mini-PIV system is 2% and we realised that stratified Taylor–Couette flows have smaller Ekman endwall effects than homogeneous ones. Still, Ekman pumping has an impact of the flow and might be responsible for differences between the data and theoretical models ignoring the endwalls. Here we focus on the flow structure during transition to SRI, the drift rate of SRI modes and the radial momentum flux as a function of the Reynolds number. Whereas the structure in form of trapped boundary Kelvin modes and the drift rate corresponds well with earlier predictions, the momentum flux shows a nonlinear dependency with respect to the Reynolds number. Away from the region of transition, theoretical models show a linear relationship. Several possible reasons for the mismatch between the experimental and theoretical models are discussed. Most important, we experimentally demonstrated that in the Rayleigh stable flow regime the SRI can provide a significant amount of outward momentum flux which makes this instability interesting in the context of accretion disks and also of atmospheric vortices where rotation and stratification also play a significant role.  相似文献   

Pleistocene ice and paleo-strain rates at Taylor Glacier, Antarctica     

S.M. Aciego  J.L. Kavanaugh 《Quaternary Research》2007,68(3):303-313

Ice exposed in ablation zones of ice sheets can be a valuable source of samples for paleoclimate studies and information about long-term ice dynamics. We report a 28-km long stable isotope sampling transect along a flowline on lower Taylor Glacier, Antarctica, and show that ice from the last glacial period is exposed here over tens of kilometers. Gas isotope analyses on a small number of samples confirm our age hypothesis. These chronostratigraphic data contain information about past ice dynamics and in particular should be sensitive to the longitudinal strain rate on the north flank of Taylor Dome, averaged over millennia. The imprint of climatic changes on ice dynamics may be discernible in these data.  相似文献   

青藏高原地磁场模型的研究   总被引：9，自引：6，他引：3       下载免费PDF全文

安振昌 《地球物理学报》2000,43(3):339-345

根据青藏高原地磁三分量绝对测量资料,使用泰勒多项式方法和冠谐分析方法,计 算了青藏高原地磁场（Ｘ, Ｙ,Ｚ ）的泰勒多项式模型和青藏高原地磁剩余场（△Ｘ,△Ｙ,△Ｚ）的冠谐 模型,并绘制了相应的理论地磁图．分析了磁异常点对地磁场模型的影响,对比分析了地磁 场的多项式模型和冠谐模型,讨论了地磁场模型的边界效应问题．  相似文献