A Numerical Model for Natural Backfill of Pipeline Trenches Subjected to Unidirectional／Oscillatory Flows     

LIANGDong-fang CHENGLiang KervinYEOW 《中国海洋工程》2005,19(2):269-286

A numerical model for the self-burial of a pipeline trench is developed. Morphological evolutions of a pipeline trench under steady-current or oscillatory-flow conditions are simulated with/without a pipeline inside the trench. The oscillatory flow in this study represents the action of waves. The two-dimensional Reynolds-averaged continuity and Navier-Stokes equations with the standard k-e turbulence closure, as well as the sediment transport equations, are solved with the finite difference method in a eurvilirrear coordinate system. Both bed and suspended loads of sediment transport are included in the morphological model. Because of the lack of experimental data on the backfilling of pipeline trenches, the numericalmodel is firstly verified against three closely-relevant experiments available in literature. A detailed measurement of the channel migration phenomenon under steady currents is employed for the assessment of the integral performance of themodel. The two experimental results from U-tube tests are used to validate the model‘s ability in predicting oscillatory flows. Different time-marching schemes are employed for the morphological computation under unidirectional and oscillatory conditions. It is found that vortex motions within the trench play an important role in the trench development.  相似文献   

风浪周期分布与谱宽度的关系     

文凡  高志一 《海洋湖沼通报》2006,(3):1-5

本文通过分析实验室风浪周期分布,发现风浪周期累积概率分布曲线低于Longuet-Higgins理论结果,在小概率周期区域实验结果与理论结果的差异明显。对实验结果进一步分析发现,在谱不是很窄时,在小概率处风浪周期累积概率随谱宽度的增大而降低,这与窄谱假定下的理论结果相反,Longuet-Higgins理论结果在小概率处不便于描述周期分布随谱宽度的变化。根据实验结果提出风浪周期的Weibull分布经验公式,Weibull分布中的参数依赖于谱宽度。  相似文献   

往复流中双向导向叶冲动透平模型性能试验研究     

梁贤光  孙培亚  王伟  蒋念东 《海洋工程》2001,19(4):84-93

研制了 30 0双向自调导叶透平试验机组 ,安装在 10 0 0活塞式往复流透平试验台上 ,对两种叶轮方案和 6种不同喷咀、扩压器进行了不同活塞行程、不同周期和不同恒定输出电压下性能试验。试验结果表明在喷咀出口角α1=2 1 5°、扩压器入口角α2 =6 5 5°和α1=2 4°、α2 =6 3°组合最佳 ,最高效率达 5 3 3% ,而且在宽广流量系数范围内 ,特别是大流量系数范围内都有较高效率。大大优于常用对称翼透平。将上下游导叶固定 ,变成双向固定导叶透平。用No 1叶轮和 6种导叶出口角组合进行试验。表明最佳导叶出口角为 2 4°～ 30°,最高效率仍达 38 5 % ,比对称翼透平仍高许多  相似文献   

A Study on the Spectral Form of Nearshore Water Waves     

Kuo Yiyu Chien Chungching Professor 《中国海洋工程》1993,(3)

- The spectral form of wind waves is investigated based on the ocean wave data observed at three nearshore stations of Taiwan. In this study, the generalized forms of Pierson-Moskowitz spectrum and JONSWAP spectrum are used to describe the local wave spectrum by selecting suitable spectral form parameters. It is shown that, at a specific site, the similarity of wave spectral form exists. Thus it is possible to use a representative spectral form for a given nearshore region to describe the wave spectrum at this nearshore. On the other hand, the effects of relative water depth on spectral form are examined. The feasibility of two spectral models in finite water depth is evaluated by using the same field wave data.  相似文献   

渤海湾盆地南堡凹陷原油成因类型及其分布规律   总被引：8，自引：3，他引：5  

李素梅  姜振学  董月霞  王旭东 《现代地质》2008,22(5)

南堡凹陷近年油气勘探取得了重大突破,为揭示该区滩海与陆地油气成因及分布规律,对67个原油和油砂样品进行了详细的地球化学研究。南堡凹陷原油具有低硫、中高蜡含量特征,陆相成因特点显著。共分为4种类型原油:(1)陆地沙三段深部层系原油,具有高4-甲基甾烷丰度、低奥利烷丰度与低甲基菲指数值和轻微偏高成熟度特征;(2)陆地Es1—Ed原油与Ng和Nm原油,其特征与第一类原油相反;上第三系原油普遍遭遇生物降解;(3)滩海东营组原油,以较高伽马蜡烷/C30藿烷和高甾烷/藿烷值区别于陆地原油;(4)滩海奥陶系潜山原油,具有低丰度甾萜类生物标志物、相对高丰度孕甾烷、三环萜烷与重排甾烷系列等特征,显示较高成熟度。上述4种成因类型原油指示南堡凹陷陆地、滩海均存在多层导有利烃源岩;同层位中滩海Es1-Ed存在较陆地更为优越的有利烃源岩,南堡滩海地区具有广泛的油气勘探前景。  相似文献   

渤海GNSS-R机载测风试验及其反演结果     

周兆明  符养 《武汉大学学报(信息科学版)》2008,33(3):241-244

对渤海GNSS-R机载试验进行了海面风场反演.结果表明,风速精度优于1 m/s,风向精度优于20°.  相似文献   

The origin of accretionary lapilli   总被引：1，自引：0，他引：1  

J. S. Gilbert  S. J. Lane 《Bulletin of Volcanology》1994,56(5):398-411

Experimental investigations in a recirculating wind tunnel of the mechanisms of formation of accretionary lapilli have demonstrated that growth is controlled by collision of liquid-coated particles, due to differences in fall velocities, and binding as a result of surface tension forces and secondary mineral growth. The liquids present on particle surfaces in eruption plumes are acid solutions stable at 100% relative humidity, from which secondary minerals, e.g. calcium sulphate and sodium chloride, precipitate prior to impact of accretionary lapilli with the ground. Concentric grain-size zones within accretionary lapilli build up due to differences in the supply of particular particle sizes during aggregate growth. Accretionary lapilli do not evolve by scavenging of particles by liquid drops followed by evaporation — a process which, in wind tunnel experiments, generates horizontally layered hemispherical aggregates. Size analysis of particles in the wind tunnel air stream and particles adhering to growing aggregates demonstrate that the aggregation coefficient is highly grain-size dependent. Theoretical simulation of accretionary lapilli growth in eruption plumes predicts maximum sizes in the range 0.7–20 mm for ash cloud thicknesses of 0.5–10 km respectively.  相似文献   

Structure and energy transfer of unstable hot star winds     

A. Feldmeier 《Astrophysics and Space Science》1994,221(1-2):393-408

Due to the instability of the radiation line force, the winds of hot, luminous stars should show a pronounced time-dependence resulting from the nonlinear growth of initially small perturbations. Following the method of Owocki, Castor & Rybicki (1988), we describe the time-dependent wind structure obtained with an independently developed code. Under the central assumption ofisothermality, our results are in very good agreement with the ones by Owocki et al. We find that the response of the wind to periodic base perturbations remains largely periodic, at least up tor 2...3R _* , with no clear evidence of stochastic behaviour.In order to test the foregoing assumption of isothermality and to compute the X-ray emission from models of structured winds, we have also incorporated theenergy equation into our simulations. We encountered the numerical problem that all radiative cooling zones collapse because of the oscillatory thermal instability (cf. Langer et al. 1981). We present a method to hinder this collapse by changing the cooling function at low temperatures. The resulting wind showsresolved cooling zones; but, for a supergiant wind relatively close to the star (r 10R _* ), the macroscopic wind structure is very similar to isothermal calculations. Most of the hot material is caused by shell-shell collisions.  相似文献   

新疆地区夏季平流层低层风场特征分析及数值模拟     

王晓婷  李森  史小康  黄江平  胡艳冰 《气象科技》2021,49(6):878-884

利用2017年6—8月的FNL再分析资料分析了新疆地区夏季平流层低层风场的时空演变特征，开展了平流层低层风场的高分辨率数值模拟和检验。结果表明：新疆地区夏季平流层纬向风随时间的变化存在经向差异，同时准零风层开始和结束的时间也存在经向差异，准零风层开始时间南部地区早于北部地区，而准零风层结束时间则相反。整个夏季新疆地区上空的准零风层处于70～40 hPa之间，其高度随时间呈先降低而后升高的变化趋势。准零风层数值模拟结果表明，模拟的准零风层参数与探空资料分析结果相比二者存在一致的变化趋势，准零风层起始高度的平均绝对误差为467 m，该高度对应的风速均方根误差为1.75 m/s。  相似文献   

近海核电厂核素地下水释放通量的模型计算方法     

朱君  李婷  陈超  谢添  张艾明 《吉林大学学报(地球科学版)》2021,51(1):201-211

为了定量计算陵区近海核电站排水管线泄漏情景下核素通过地下水途径向海洋环境的释放通量，以某近海核电站为例进行研究。首先，应用GOCAD软件建立三维地形地质模型，刻画地层的分布、剥蚀以及倾向等特点；然后，运用地下水数值模拟软件FEFLOW精细刻画丘陵区地下水系统的补给、径流和排泄特征；最后，以不被吸附滞留的核素³H和被吸附滞留的核素⁹⁰Sr、¹³⁷Cs为对象，通过实验测定了⁹⁰Sr、¹³⁷Cs在不同岩土介质中的分配系数，模拟计算了排水管线连续渗漏60 a后³H、⁹⁰Sr、¹³⁷Cs在地下水中的放射性分布及释放。结果表明：³H迁移速度基本与地下水流速一致，地下水中的最大放射性浓度为0.285 0 Bq/L，第20 000天时向收纳水域的释放通量达到最大值，约526 Bq/d；⁹⁰Sr吸附性能相对较弱，最大迁移距离约80 m，地下水中的最大放射性浓度为0.032 1 Bq/L；¹³⁷Cs吸附能力较强，相当长的时间内被滞留在管线附近，地下水中最大放射性浓度分别为6.840×10^-3 Bq/L，释放通量为0 Bq/d。由弥散度的不确定分析可知，弥散度越大，地下水中³H的最大放射性浓度越小，向海洋环境的释放通量越多。  相似文献