Facies of slurry-flow deposits, Britannia Formation (Lower Cretaceous), North Sea: implications for flow evolution and deposit geometry   总被引：4，自引：0，他引：4  

Donald R. Lowe  Martin Guy†  Andrew Palfrey† 《Sedimentology》2003,50(1):45-80

ABSTRACT Mud‐rich sandstone beds in the Lower Cretaceous Britannia Formation, UK North Sea, were deposited by sediment flows transitional between debris flows and turbidity currents, termed slurry flows. Much of the mud in these flows was transported as sand‐ and silt‐sized grains that were approximately hydraulically equivalent to suspended quartz and feldspar. In the eastern Britannia Field, individual slurry beds are continuous over long distances, and abundant core makes it possible to document facies changes across the field. Most beds display regular areal grain‐size changes. In this study, fining trends, especially in the size of the largest grains, are used to estimate palaeoflow and palaeoslope directions. In the middle part of the Britannia Formation, stratigraphic zones 40 and 45, slurry flows moved from south‐west and south towards the north‐east and north. Most zone 45 beds lens out before reaching the northern edge of the field, apparently by wedging out against the northern basin slope. Zone 40 and 45 beds show downflow facies transitions from low‐mud‐content, dish‐structured and wispy‐laminated sandstone to high‐mud‐content banded units. In zone 50, at the top of the formation, flows moved from north to south or north‐west to south‐east, and their deposits show transitions from proximal mud‐rich banded and mixed slurried beds to more distal lower‐mud‐content banded and wispy‐laminated units. The contrasting facies trends in zones 40 and 45 and zone 50 may reflect differing grain‐size relationships between quartz and feldspar grains and mud particles in the depositing flows. In zones 40 and 45, quartz grains average 0·30–0·32 mm in diameter, ≈ 0·10 mm coarser than in zone 50. The medium‐grained quartz in zones 40 and 45 flows may have been slightly coarser than the associated mud grains, resulting in the preferential deposition of quartz in proximal areas and downslope enrichment of the flows in mud. In zone 50 flows, mud was probably slightly coarser than the associated fine‐grained quartz, resulting in early mud sedimentation and enrichment of the distal flows in fine‐grained quartz and feldspar. Mud particles in all flows may have had an effective grain size of ≈ 0·25 mm. Both mud content and suspended‐load fallout rate played key roles in the sedimentation of Britannia slurry flows and structuring of the resulting deposits. During deposition of zones 40 and 45, the area of the eastern Britannia Field in block 16/26 may have been a locally enclosed subbasin within which the depositing slurry flows were locally ponded. Slurry beds in the eastern Britannia Field are ‘lumpy’ sheet‐like bodies that show facies changes but little additional complexity. There is no thin‐bedded facies that might represent waning flows analogous to low‐density turbidity currents. The dominance of laminar, cohesion‐dominated shear layers during sedimentation prevented most bed erosion, and the deposystem lacked channel, levee and overbank facies that commonly make up turbidity current‐dominated systems. Britannia slurry flows, although turbulent and capable of size‐fractionating even fine‐grained sediments, left sand bodies with geometries and facies more like those deposited by poorly differentiated laminar debris flows.  相似文献   

南海各月月平均海流场的数值模拟   总被引：3，自引：0，他引：3       下载免费PDF全文

李东辉  游小宝  张铭 《气象科学》2003,23(1):31-38

本文用一个区域三维、自由表面、斜压海洋模式对南海全年各月的三维平均流场进行了数值模拟，模拟得到的环境特征与己有的实测资料十分相近，这表明该模拟结果是可信的，该数值模拟也是成功的。  相似文献   

一个有限区变网格模式的设计   总被引：1，自引：0，他引：1       下载免费PDF全文

钱滔滔  郭肖容  廖洞贤 《大气科学》1997,21(6):687-697

在国家气象中心业务运行的有限区球面均匀网格模式的基础上设计了一个有限区变网格模式。使预报的窗口区设计为均匀细网格0.5°，而窗口区以外则以0.1°经纬度均匀向外递增。采用廖洞贤1995年提出的坐标变换方法，变网格中的模式方程可以在相应的均匀网格上进行计算。利用实际资料对绝热模式进行了变网格与全场均匀细网格0.5°的对比试验。3个个例的试验结果表明:对窗口区变网格模式预报几乎与全场均匀细网格模式预报水平相当。但由于窗口区外网格点数减少而所用计算机时（CPU）节省了一半以上。  相似文献   

基岩水的壁间运动及基本特征   总被引：5，自引：0，他引：5  

罗绍河  王心义 《水文地质工程地质》1997,24(3):15-17

本文通过对基岩水与孔隙水的比较分析，介绍了基岩水的分布、水动力学和水化学特征，指出了基岩水运动具有均位趋势、选择流动及汇流特性，得出了渗流理论不宜用于基岩水的结论。  相似文献   

Time-dependent, coupled, Ekman boundary layer solutions incorporating Stokes drift   总被引：2，自引：0，他引：2  

D. M. Lewis  S. E. Belcher 《Dynamics of Atmospheres and Oceans》2004,37(4):313-351

Recent technological advances in current measuring devices has resulted in a large observational database related to wind-driven motions in the upper ocean mixed layer. This has served to highlight the fact that transient motions make up a substantial contribution of the resulting Ekman currents. At the same time, certain discrepancies have emerged between the observed angular deflections of the steady-state currents from the surface wind stress, both at the surface and at sub-surface depths, which cannot be reconciled using the classical Ekman model. This paper seeks to tackle these two issues.First a general analytical method is presented for solving the time dependent horizontal momentum Ekman equations. Analysis of the unsteady terms that arise from simple special cases shows how the evolution proceeds through three stages. At early times, the Coriolis acceleration is insignificant, and the current is unidirectional and deepens through downward diffusion of momentum. Later Coriolis acceleration deflects the current vectors in the upper layers, whilst downward diffusion of momentum continues to deepen the layer. Finally, once diffusion has penetrated down to the depth of the steady-state current, then the transients decay on the inertial or diffusive timescale, depending upon the boundary conditions of the particular problem.In the second half of the paper, a new steady-state model is developed that includes the effects of wind-generated waves, through the action of their Stokes drift on the planetary vorticity. Comparisons between observations and the theoretical predictions, demonstrate that inclusion of the Stokes drift is the key to reconciling the discrepancies in the angular deflections of the steady-state currents. This leads to the conclusion that Ekman layer currents are significantly influenced by the surface waves.  相似文献   

圆形截面灌注桩正截面均匀配筋计算可视化     

杨超  罗运军  张英才 《岩土工程技术》2004,18(6):299-302

在圆形截面均匀配筋偏心受压混凝土构件的正截面承载力基本计算公式的基础之上 ,结合基坑工程中圆截面灌注桩的受力特点 ,推导了灌注桩均匀配筋计算的有关公式 ,并以此为基础 ,利用可视化编程软件Delphi 6 .0编写了相应的配筋计算程序。通过实际例证 ,表明该程序计算快捷且结果准确。  相似文献   

山区三维地震勘探大时差静校正及时深转换     

何黄生  陈光明刘威周峰岩  陈国忠 《中国煤田地质》2004,16(2):34-36

山地煤矿采区地形条件复杂，正确进行大时差静校正是处理好二维地震勘探资料的重要一环。大时差静校正会改变煤层反射波时间(t0)及双曲线特征，为减小校正误差，需设立一个CMP面，将校正量分为高频分量和CMP校正量。在地形高差变化剧烈的山地，不能用高于地表面的统一基准面为零线进行时深转换，须进行充填层时差(△t)校正，将统一基准面校正到地表面，再以地表面为零线进行时深转换成图。以便准确无误的展示煤层赋存形态，提高构造图精度。  相似文献   

A Numerical Study on Coastal Defence at Chennai and Related Management Strategies     

J. S. Mani 《Natural Hazards》2004,31(2):523-536

Chennai coast, right from the inception of Madras harbourin the year 1876, has been experiencinghostile conditions such as (i) coastal erosion, (ii) sandbar formation at the entrance to inlets, (iii) sea water ingression and (iv) change insea bed elevation, etc. In addition, construction of a new satellite harbour, about18 km north of Madras harbour has produced a negative impact on the delicatecoastal features such as (i) Pulicat lake, (ii) Ennore shoals, etc. Construction ofthis satellite harbour has led to the accumulation of sand south of the southbreakwater of the harbour and its accelerated growth is of concern to an inletlocated 2.6~km south of the harbour. `Coastal erosion', a perennial problemassociated with north Chennai sea front for the past 100 years has been addressedin this paper. The paper discusses on a long term solution and details of themethodologies to be adopted for effective management of the coast. Thesolution presented in this paper is based on numerical model study consideringthe nearshore currents and wave induced sediment transports.  相似文献   

The geoid EDIN2000 and mean sea surface topography around the British Isles   总被引：2，自引：0，他引：2  

Roger Hipkin  Keith Haines  Ciaran Beggan  Richard Bingley  Fabrice Hernandez  Jason Holt  Trevor Baker 《Geophysical Journal International》2004,157(2):565-577

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Inviscid behaviour of fines-rich pyroclastic flows inferred from experiments on gas-particle mixtures     

O. Roche  M.A. Gilbertson  R.S.J. Sparks 《Earth and Planetary Science Letters》2005,240(2):401-414

Experiments were carried out on granular flows generated by instantaneous release of gas-fluidised, bidisperse mixtures and propagating into a horizontal channel. The mixture consists of fine (< 100 μm) and coarse (> 100 μm) particles of same density, with corresponding grain size ratios of ∼ 2 to 9. Initial fluidisation of the mixture destroys the interparticle frictional contacts, and the flow behaviour then depends on the initial bed packing and on the timescale required to re-establish strong frictional contacts. At a fines mass fraction (α) below that of optimal packing (∼ 40%), the initial mixtures consist of a continuous network of coarse particles with fines in interstitial voids. Strong frictional contacts between the coarse particles are probably rapidly re-established and the flows steadily decelerate. Some internal friction reduction appears to occur as α and the grain size ratio increases, possibly due to particle rolling and the lower roughness of internal shear surfaces. Segregation only occurs at large grain size ratio due to dynamical sieving with fines concentrated at the flow base. In contrast, at α above that for optimal packing, the initial mixtures consist of coarse particles embedded in a matrix of fines. Flow velocities and run-outs are similar to that of the monodisperse fine end-member, thus showing that the coarse particles are transported passively within the matrix whatever their amount and grain size are. These flows propagate at constant height and velocity as inviscid fluid gravity currents, thus suggesting negligible interparticle friction. We have determined a Froude number of 2.61 ± 0.08 consistent with the dam-break model for fluid flows, and with no significant variation as a function of α, the grain size ratio, and the initial bed expansion. Very little segregation occurs, which suggests low intensity particle interactions during flow propagation and that active fluidisation is not taking place. Strong frictional contacts are only re-established in the final stages of emplacement and stop the flow motion. We infer that fines-rich (i.e. matrix-supported) pyroclastic flows propagate as inviscid fluid gravity currents for most of their emplacement, and this is consistent with some field data.  相似文献