Propagation of elastic waves in a cylindrical bore in a liquidsaturated porous solid     

M. D. Sharma  M. L. Gogna 《Geophysical Journal International》1990,103(1):47-54

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Quasi-shear wave coupling in weakly anisotropic 3-D media   总被引：2，自引：0，他引：2  

R.T. Coates  C. H. Chapman 《Geophysical Journal International》1990,103(2):301-320

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近岸海浪、风暴潮及海啸灾害远程实时监测系统的现场试验及应用   总被引：1，自引：0，他引：1  

王盛安  龙小敏  黎满球  姚远  潘文亮 《热带海洋学报》2009,28(1)

利用自主研发的近岸海浪、风暴潮及海啸灾害远程实时监测系统,在广东省阳江市闸坡附近海域进行了远程实时监测试验.文章介绍了监测系统的组成,对2007年9月1日-10月3日的观测记录进行了分析,计算出台风增水、波高和波周期,采用低通滤波方法获得重力外波.实验结果表明,研发的近岸海浪、风暴潮及海啸灾害远程实时监测系统可供实际推广应用.  相似文献   

Distribution of the nonlinear random ocean wave period     

侯一筠  李明杰  宋贵霆  司广成  齐鹏  胡珀 《中国海洋湖沼学报》2009,27(4):919-923

Because of the intrinsic difficulty in determining distributions for wave periods, previous studies on wave period distribution models have not taken nonlinearity into account and have not performed well in terms of describing and statistically analyzing the probability density distribution of ocean waves. In this study, a statistical model of random waves is developed using Stokes wave theory of water wave dynamics. In addition, a new nonlinear probability distribution function for the wave period is presented with the parameters of spectral density width and nonlinear wave steepness, which is more reasonable as a physical mechanism. The magnitude of wave steepness determines the intensity of the nonlinear effect, while the spectral width only changes the energy distribution. The wave steepness is found to be an important parameter in terms of not only dynamics but also statistics. The value of wave steepness reflects the degree that the wave period distribution skews from the Cauchy distribution, and it also describes the variation in the distribution function, which resembles that of the wave surface elevation distribution and wave height distribution. We found that the distribution curves skew leftward and upward as the wave steepness increases. The wave period observations for the SZFII-1 buoy, made off the coast of Weihai (37°27.6′ N, 122°15.1′ E), China, are used to verify the new distribution. The coefficient of the correlation between the new distribution and the buoy data at different spectral widths (ν=0.3−0.5) is within the range of 0.968 6 to 0.991 7. In addition, the Longuet-Higgins (1975) and Sun (1988) distributions and the new distribution presented in this work are compared. The validations and comparisons indicate that the new nonlinear probability density distribution fits the buoy measurements better than the Longuet-Higgins and Sun distributions do. We believe that adoption of the new wave period distribution would improve traditional statistical wave theory.  相似文献   

方向分布对三维聚焦波浪波面特性影响研究     

李金宣  柳淑学  孙一艳  HONG Keyyong 《海洋工程》2008,26(2):26-33

波浪聚焦被认为是产生极限波浪的重要机理之一,近年来受到普遍重视。通过高阶谱方法,引入造波边界建立数值计算模型,模拟聚焦波浪在不同方向分布时的产生和聚焦过程,研究波浪的方向分布对聚焦波浪的波面、波峰最大值、聚焦点的偏移、波面参数及频谱的影响。研究结果表明波浪方向分布越窄,波浪的非线性影响越强、波面越陡,波峰值、聚焦点的偏移和波面特征参数都越大;同时方向分布对波浪聚焦前后的能量具有很大的影响。  相似文献   

涌浪对风浪能量影响的实验研究     

黄必桂  郑桂珍  丛培秀 《中国海洋大学学报(自然科学版)》2009,39(3)

在实验室风浪水槽中进行纯风浪和混合浪波面位移观测,研究波长较长的规则波对风浪能量的影响.本文用混合浪和纯风浪中的风浪显著波的零阶谱矩之比代表混合浪中的风浪与纯风浪能量之比,并以此表征涌浪对风浪能量的影响.研究了该能量比随涌浪波陡S、风区x、波龄倒数u/C、涌浪频率与纯风浪谱峰频率之比fs/fwp的变化规律.结果表明,涌浪对风浪能量的抑制作用随涌浪波陡的增加、波龄倒数的增大及涌浪频率与纯风浪谱峰频率之比的增大而增强.发现该能量比依赖于无因次量R=(1+80(πS)2)1.9(fs/fwp)0.9(u/C)0.27,并拟合得到2者的经验关系.此外,本文实验还发现,在某些情况下,涌浪的存在使风浪能量增加.  相似文献   

Relative velocities among accreting planetesimals in binary systems: The circumprimary case     

P. Thébault  F. Marzari 《Icarus》2006,183(1):193-206

We investigate classical planetesimal accretion in a binary star system of separation ab?50 AU by numerical simulations, with particular focus on the region at a distance of 1 AU from the primary. The planetesimals orbit the primary, are perturbed by the companion and are in addition subjected to a gas drag force. We concentrate on the problem of relative velocities Δv among planetesimals of different sizes. For various stellar mass ratios and binary orbital parameters we determine regions where Δv exceed planetesimal escape velocities vesc (thus preventing runaway accretion) or even the threshold velocity vero for which erosion dominates accretion. Gaseous friction has two crucial effects on the velocity distribution: it damps secular perturbations by forcing periastron alignment of orbits, but at the same time the size-dependence of this orbital alignment induces a significant Δv increase between bodies of different sizes. This differential phasing effect proves very efficient and almost always increases Δv to values preventing runaway accretion, except in a narrow eb?0 domain. The erosion threshold Δv>vero is reached in a wide (ab,eb) space for small <10-km planetesimals, but in a much more limited region for bigger ?50-km objects. In the intermediate vesc<Δv<vero domain, a possible growth mode would be the type II runaway growth identified by Kortenkamp et al. [Kortenkamp, S., Wetherill, G., Inaba, S., 2001. Science 293, 1127-1129].  相似文献   

Near-infrared adaptive optics imaging of the satellites and individual rings of Uranus     

S.G. Gibbard  I. de Pater 《Icarus》2005,174(1):253-262

We present the first Earth-based images of several of the individual faint rings of Uranus, as observed with the adaptive optics system on the W.M. Keck II telescope on four consecutive days in October 2003. We derive reflectivities based on multiple measurements of 8 minor moons of Uranus as well as Ariel and Miranda in filters centered at wavelengths of 1.25(J), 1.63(H), and 2.1(Kp) μm. These observations have a phase angle of 1.84°-1.96°. We find that the small satellites are somewhat less bright than in observations made by the HST at smaller phase angles, confirming an opposition surge effect. We calculate albedoes for the ring groups and for each ring separately. We find that the ε ring particles, as well as the particles in the three other ring groups, have albedoes near 0.043 at these phase angles. The equivalent depths of some of the individual rings are different than predicted based upon ring widths from occultation measurements (assuming a constant particle ring brightness); in particular the γ ring is fainter and the η ring brighter than expected. Our results indicate that q, the ratio of ε ring intensity at apoapse vs. periapse, is close to 3.2±0.16. This agrees well with a model that has a filling factor for the ε ring of 0.06 (Karkoschka, 2001, Icarus 151, 78-83). We also determine values of the north to south brightness ratio for the individual rings and find that in most cases they are close to unity.  相似文献   

极限波浪运动特性的非线性数值模拟   总被引：1，自引：0，他引：1       下载免费PDF全文

宁德志  滕斌  姜立明  臧军 《海洋学报》2008,30(3):126-132

利用时域高阶边界元方法建立了模拟极限波浪运动的完全非线性数值模型,其中自由水面满足完全非线性自由水面条件.采用半混合欧拉-拉格朗日方法追踪流体瞬时水面,运用四阶Runge-Kutta方法更新下一时间步的波面和速度势,同时应用镜像格林函数消除水槽两个侧面和底面上的积分.研究中利用波浪聚焦的方法产生极限波浪,并且在水槽中开展了物理模型实验,将测点试验数据与数值结果进行了对比,两者吻合得很好.对极限波浪运动的非线性和流域内速度分布进行了研究.  相似文献   

广东一次寒潮8级大风物理过程分析   总被引：1，自引：0，他引：1  

苏百兴  段朝霞 《海洋预报》2009,26(1)

本文利用NCEP1°×1°的网格点分析资料和常规观测资料对2006年1月4～7日广东寒潮造成的广东海面8级大风过程进行了物理机制分析.结果表明:受强冷空气南下影响,有着较深厚的强冷平流输送,加之高空动量下传的共同作用,故而造成了广东东、西部海面先后出现了8级大风过程.这为以后更准确地预报广东海面大风提供了良好的依据.  相似文献