小型单拖网渔船V 型网板水动力性能研究   总被引：1，自引：0，他引：1  

李崇聪  梁振林  黄六一  周为峰  孙鹏  王磊 《海洋科学》2013,37(11):69-73

网板是拖网的重要属具之一, 广泛应用于近岸小型单拖渔船的生产作业中, 其水动力性能的优劣直接关系到拖网的生产效果和经济效益。作者以网板面积1 m²、展弦比0.55的 V 型网板为例进行小型单拖渔船的水动力性能研究。 基于田内相似准则, 相似比为2制作网板模型, 进行循环水槽模型试验, 实验冲角在10～60°范围内, 来流速度在0.2～0.7 m/s, 得出网板升阻力系数等流体动力特性曲线、临界冲角、最大升阻比。结果表明, 该型网板的最大升阻比约为1.86, 达到最大升阻比的临界冲角在15～25°附近, 该结果可为渔业生产操作中网板冲角的设置提供依据。实验结果同时显示, 该型网板的水动力效率略低于其他类型网板, 说明其板型仍有较大的改进空间。  相似文献   

Preliminary Study on the Water Drag of Schlegel＇s Black Rockfish Sebastes schlegeli     

LIWentao ZHANGXiumei GAOTianxiang JINGAiguo 《中国海洋大学学报(英文版)》2004,3(1):70-74

Drag forces acting on Schlegel‘s black rockfish Sebastes schlegeli were studied. A new drag force transducer was designed and used to measure the water drag on Schlegel‘s black rockfish in a vertical recirculating flume tank. Fourteen individuals were investigated, yielding two mean drag coefficients referred to the cross-sectional area and volume^2/3 respectively at water velocities ranging from 0.3 to 1.0 ms^-1 The drag coefficients can be used for estimating the drag forces acting on Sebastes schlegeli in water.  相似文献   

东海深部致密储层主要钻井技术及其应用          下载免费PDF全文

张海山  宫吉泽 《探矿工程》2019,46(1):39-44

随着东海对深部致密储层油气资源的勘探开发,深井、超深井钻井面临的地层埋藏深、压力体系复杂、地层可钻性差、裸眼段长、井斜大等难题,需要研究可行的技术方案加以解决。为此,2012年以来,在东海实施的深井、超深井中,通过应用深井井身结构优化、高效抗摩减阻剂、动力导向和复合冲击提速技术、井口回注固井技术和随钻声波固井质量评价技术,实现了安全、快速的钻井效果。上述技术的应用对致密地层钻进、提高钻井速度、缩短钻井周期、降低作业成本、获得更好的经济效益,具有重要的保障作用。  相似文献   

偏心系数和锚腚角对固定锚腚拖曳锚运动的影响     

张春会  张海霞  赵全胜  田英辉  郑晓明 《岩土力学》2018,39(2):515-522

为观测和分析安装中拖曳锚在土中的运动特性,自制了由玻璃水槽、拖曳系统和拉力传感器组成的板锚拖曳试验装置。将硅凝胶与水混合制备成了透明土,依据有效重度强度比确定模型锚材料,按照1:50缩尺比例,在自制板锚拖曳试验装置上开展固定锚腚拖曳锚拖曳试验,研究了偏心系数和锚腚角对固定锚腚拖曳锚运动特性的影响规律。结果表明：该试验装置可以直接观测拖曳板锚嵌入土中运动的全过程;锚眼法向偏心距和切向偏心距不是独立参数,偏心系数能综合描述锚眼偏心对板锚在土中运动的影响;锚腚角是影响板锚在土中运动的重要参数,随着锚腚角增加,板锚最终嵌土深度先增加后减小;随着锚眼偏心系数增加,板锚最终嵌土深度先增加后减小;固定锚腚拖曳锚在土中的运动轨迹近似服从负指数函数曲线。  相似文献   

Two-dimensional Dynamics Simulation of Two-phase Debris Flow     

LIU Wei  HE Siming  OUYANG Chaojun 《《地质学报》英文版》2017,91(5):1873-1883

To investigate the movement mechanism of debris flow, a two‐dimensional, two‐phase, depth‐integrated model is introduced. The model uses Mohr‐Coulomb plasticity for the solid rheology, and the fluid stress is modeled as a Newtonian fluid. The interaction between solid and liquid phases, which plays a major role in debris flow movement, is assumed to consist of drag and buoyancy forces. The applicability of drag force formulas is discussed. Considering the complex interaction between debris flow and the bed surface, a combined friction boundary condition is imposed on the bottom, and this is also discussed. To solve the complex model equations, a numerical method with second‐order accuracy based on the finite volume method is proposed. Several numerical experiments are performed to verify the feasibilities of model and numerical schemes. Numerical results demonstrate that different solid volume fractions substantially affect debris flow movement.  相似文献   

板翼动力锚水中自由下落过程数值模拟     

刘君  张雪琪 《海洋工程》2017,35(3):29-36

板翼动力锚是依靠自重完成安装并靠自重和海床土的抗力来锚固的新型动力锚。板翼动力锚在水中自由下落的阻力决定了锚到达海床表面时的速度,进而直接决定了锚贯入海床中的深度以及它能提供的承载力。板翼动力锚的形状比较复杂,采用计算流体动力学的方法研究板翼动力锚的下落速度、水平位移和转角与下落位移的关系。计算结果表明:板翼动力锚的拖曳阻力系数约为0.93~1.12之间;在沉贯过程中应使加载臂与翼板共面以减少阻力;板翼动力锚的终端速度约为28 m/s。  相似文献   

Effect of Peak Perforation on Flow Past A Conic Cylinder at Re=100: Drag, Lift and Strouhal Number     

LIN Li-ming  ZHONG Xing-fu  WU Ying-xiang 《海洋工程》2017,31(3):330-340

A flow past a circular-section cylinder with a perforated conic shroud, in which the perforation is located at the peak of the conic disturbance as the shroud installed on the cylinder and uniformly distributed with several circular holes, is numerically simulated at a Reynolds number of 100. Two factors in the perforation are taken into account, i.e. the attack angle relative to the direction of incoming flow and diameter of holes. The effect of such perforation on the drag, lift and vortex-shedding frequency is mainly investigated. Results have shown that variation of the attack angle has a little effect, especially on the drag and vortex-shedding frequency, except in certain cases due to the varied vortex-shedding patterns in the near wake. The increasing hole diameter still exhibits a little effect on the drag and frequency of vortex shedding, but really reduces the lift, in particular at larger wavelength, such as the lift reduction reaching almost 66%–68% after introducing the perforation.  相似文献   

一个重力滑动构造的范例——介绍河南芦店滑动构造     

孙锦屏  ;李万程 《中国煤炭地质》2009,(4):9-15

芦店滑动构造是河南省西部嵩（山）箕（山）地区滑动构造群中的一个典型实例。其主要表现为双期相向滑动的叠加、两类滑动构造模型的拚合及两种动力因素的作用。通过对其综合研究得出滑动构造是正断层演化的结果,属于正断层的一种类型的新认识。认知滑动构造的意义在于：可在较新地层下寻找、预测埋藏较浅的煤层,如芦店滑动构造区。若按传统构造解释,芦店地区地表出露为中生界三叠系红层,其下伏主采二1煤埋深一般在1 400m左右,超过现行勘查规范资源储量估算垂深1 200m以浅的要求,但利用滑动构造观点客观、合理解释后,煤层埋藏深度最浅处只有几十m。芦店滑动构造的解释成为利用新理论找煤的一个典型范例。  相似文献   

Effect of radiation on the stability of equilibrium points in the binary stellar systems: RW-Monocerotis,Krüger 60     

M. K. Das  Pankaj Narang  S. Mahajan  M. Yuasa 《Astrophysics and Space Science》2008,314(4):261-274

We have studied the stability of location of various equilibrium points of a passive micron size particle in the field of radiating binary stellar system within the framework of circular restricted three body problem. Influence of radial radiation pressure and Poynting-Robertson drag (PR-drag) on the equilibrium points and their stability in the binary stellar systems RW-Monocerotis and Krüger-60 has been studied. It is shown that both collinear and off axis equilibrium points are linearly unstable for increasing value of β ₁ (ratio of radiation to gravitational force of the massive component) in presence of PR-drag for the binary systems. Further we find that out of plane equilibrium points (L _i , i=6,7) may exists for range of values of β ₁>1 for these binary systems in the presence of PR-drag. Our linear stability analysis shows that the motion near the equilibrium points L _6,7 of the binary systems is unstable both in the absence and presence of PR-drag.  相似文献   

On particle trajectories in restricted 3-body problem including the effect of radiation: Sun-Jupiter system     

M. K. Das  Pankaj Narang  M. Yuasa  L. M. Saha 《Astrophysics and Space Science》2008,314(1-3):59-71

In this work, we have simulated orbits of a particle moving in gravitational field of the Sun-Jupiter system. The effect of solar radiation pressure, including Poynting Robertson drag, on the evolution of particle orbits in phase space have been studied for different values of the parameter β ₁ (the ratio of radiation to gravitational force) and initial conditions. Characteristics of various computed trajectories have been studied using wavelet transform (WT), Fourier transform (FT) and Poincare surface of section method. We use wavelet analysis to identify transitions of a trajectory in time-frequency plane and further apply it to classify it as regular or chaotic in phase space. Unlike the Fourier transform method (FT), we observe that the wavelet transform (WT) also provides a basis to identify ‘sticky’ trajectories in the present dynamical system.  相似文献