排序方式： 共有39条查询结果，搜索用时 875 毫秒
1.
W. H. Jefferys G. F. Benedict P. D. Hemenway P. J. Shelus R. L. Duncombe 《Celestial Mechanics and Dynamical Astronomy》1985,37(3):299-305
The Hubble Space Telescope (HST), a large optical telescope having an aperture of 2.4 meters and a length of 8.8 meters, is being developed by the National Aeronautics and Space Administration. This telescope will be placed into earth orbit by the space shuttle. Astrometric observations with the HST are made using a Fine Guidance Sensor which is capable of measuring the position of one object relative to another with an accuracy of ±0.002 arcseconds. The astrometric user of HST will be provided with an Astrometric Data Reduction Software package (ADRS). The variety of astrometric problems to be investigated with HST is discussed. 相似文献
2.
E.R. Jefferys 《Applied Ocean Research》1983,5(3):145-149
The solution to the problem of calculating the hydrodynamic forces on multiple floating bodies is summarised. The complex coefficients which characterise the forces at each frequency of oscillation are expensive to compute; interpolation of intermediate values and extrapolation to high frequencies appear difficult since the coefficients seem to vary arbitrarily with frequency. Interpolation and extrapolation schemes based on a novel representation of the coefficients are proposed and tested. The excellent numerical results indicate that the values of the coefficients at a few frequency points can characterise the hydrodynamics at all frequencies. These techniques can save economically significant amounts of computer time and permit investigations which would otherwise be prohibitively expensive. 相似文献
3.
E.R. Jefferys 《Applied Ocean Research》1984,6(1):31-39
Classical frequency and time domain models of a single degree of freedom wave power device are presented. In the time domain, a convolution integral is conventionally used to represent the fluid dynamic radiation force, characterised by added mass and damping in the frequency domain. This integral is replaced by an approximate ordinary differential equation (ODE) model which is faster and more convenient in simulations. A time domain model of the fluid dynamics of an oscillating water column (OWC) device is derived to illustrate the technique. Digital simulations of the OWC are used to compare the accuracy of the classical and ODE models. The simulation of the ODE model runs about six times as fast as the classical model based on convolution, yet characterises the fluid dynamics accurately. 相似文献
4.
A survey of diffraction/radiation analyses has been performed on behalf of the International Ship and Offshore Structures Congress, Committee I.2. This paper presents the results from the survey, including data from 17 organisations plotted in a common format. The variability of the computed hydrodynamic loads and responses is discussed, and it is concluded that there is a degree of uncertainty in results predicted on the basis of commonly used idealisations. Even in long period waves the variability between the computed results is considerable. To obtain reliable results at the shorter periods associated with heave, pitch and roll resonances of a deep water TLP, much finer meshes than those used by most of the participating organisations would be required. 相似文献
5.
碎屑岩与火山岩混积岩系层序地层学研究初探——以准噶尔盆地西北缘佳木河组为例 总被引：1，自引：0，他引：1
准噶尔盆地西北缘前陆冲断带是剖析西准噶尔地区盆山耦合关系、沉积体系发育的关键地段。该区二叠系佳木河组为火山岩、火山碎屑岩、碎屑岩组成的混积地层。火山岩与碎屑岩组成的地层单元有广义上的成因联系,因为它们都属于史密斯地层,并均具有旋回特征。针对不同的岩性区:碎屑岩岩性区、火山岩与碎屑岩共存区、纯火山岩区,找出由于构造火山活动、相对湖平面变化等因素形成的可作为层序界面的不整合面。碎屑岩岩性区不整合面在地震剖面上主要表现为削蚀、底超、双向下超、顶超、下切谷等;共存区为同时发育火山岩与碎屑岩的削蚀带,不整合面类型较复杂;纯火山岩区表现为相对湖平面下降形成的削蚀不整合面。故可以通过地震、钻测井资料识别各类不整合面,并依据火山喷发方式、火山旋回、沉积旋回,按照不同对比原则进行经典层序地层学划分。 相似文献
6.
为了明确松辽盆地三肇凹陷扶余油层储层致密化与油气充注相关性,利用微米CT、流体包裹体显微分析、盆地模拟等方法,研究了该储层微观孔喉特征,且定量分析了其成藏期。根据储层孔隙演化信息分析了研究区储层致密化过程和油气成藏的关系。结果发现:三肇凹陷扶余致密储层岩石类型以长石岩屑砂岩和岩屑长石砂岩为主,孔喉特征表现为窄喉道、宽孔隙、孔喉配置差、微细喉道总体积大等特征。压实作用和胶结作用为储层致密化重要成因,储层致密时间应该在嫩江组末之前。流体包裹体分析结果表明三肇凹陷扶余储层油充注分为早期和晚期,相应的充注时间分别距今77~74 Ma、67~65 Ma,分别对应于嫩江组沉积期和明水组沉积末期。综合对比扶余油层油气成藏历史和储层孔隙演化特征,认为原油充注发生储层致密化之后,即先致密后成藏。 相似文献
7.
Directional seas should be ergodic 总被引：1，自引：0，他引：1
Directional seas are often modelled as a double summation of plane sinusoidal waves from different directions at a set of discrete frequencies. Unfortunately, this model is commonly used in a way which produces unrealistic standing wave phenomena and hence is not ergodic. Consequently, time averages of variables are not necessarily the same as space averages and averages over different realisations. The resulting point spectrum is randomly distributed about the target point spectrum as required, but the time history generated is only representative of a short record of the target sea. In this note, the basis of the phenomenon and its consequences for both wave tank and computer simulation work are described. Two alternative techniques of directional wave generation are discussed.
Standing waves also occur near reflectors in the sea and test tanks; their effects on point and directional wave measurements are discussed. 相似文献
8.
重力驱动作用——滦平盆地下白垩统西瓜园组沉积时期主要的搬运机制 总被引：3，自引：0，他引：3
通过对冀北滦平盆地下白垩统西瓜园组沉积地层的实地考察,发现盆地内发育丰富的重力驱动作用沉积物。文中描述西瓜园组发育的滑动和滑塌现象,指出露头剖面中存在的挤压变形现象并非构造成因,而是由于滑动块体和滑塌块体前端的挤压应力环境造成的。在介绍西瓜园组重力流沉积发育环境的基础上,对露头中存在的若干重力流沉积进行了描述,并使用砂质碎屑流这一概念对这些现象进行了较为合理的成因解释。通过对滑动和滑塌(重力块体运动)和砂质碎屑流—浊流(重力流)沉积物研究,结合前人对该地区冲积扇—扇三角洲的研究成果,认为重力驱动作用是滦平盆地下白垩统西瓜园组沉积时期主要的搬运机制。 相似文献
9.
ZHAO Jingzhou CAO Qing BAI Yubin ER Chuang LI Jun WU Weitao and SHEN Wuxian 《《地质学报》英文版》2015,89(Z1):303-306
<正>1 Introduction Petroleum accumulations from the Earth’s crust can be grouped into conventional and unconventional ones.The history of the world’s petroleum exploration is a history from the exploration of conventional accumulations to that of unconventional ones.Nevertheless,petroleum accumulation is actually a contrary process starting from 相似文献
10.
W. H. Jefferys M. J. Fitzpatrick B. E. McArthur 《Celestial Mechanics and Dynamical Astronomy》1987,41(1-4):39-49
GaussFit is a new computer program for solving least squares and robust estimation problems. It has a number of unique features, including a complete programming language designed especially to formulate estimation problems, a built-in compiler and interpreter to support the programming language, and a built-in algebraic manipulator for calculating the required partial derivatives analytically. These features make GaussFit very easy to use, so that even complex problems can be set up and solved with minimal effort. GaussFit can correctly handle many cases of practical interest: nonlinear models, exact constraints, correlated observations, and models where the equations of condition contain more than one observed quantity. An experimental robust estimation capability is built into GaussFit so that data sets contaminated by outliers can be handled simply and efficiently.Invited Talk at the 18th meeting of the Division on Dynamical Astronomy of the American Astronomical Society held in Braintree, Massachussetts, May 7–9, 1987. 相似文献