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中国海洋潮汐40年来研究进展 总被引：1，自引：0，他引：1
近４０年来我国海洋潮汐的研究获得显著进展。本文分别对潮汐的分析、推算，潮汐谱估计，平均海面，潮波理论和数值研究等方面进行阐述。潮汐分析、推算已有１００多个分潮的模型可供应用，交点订正系统除利用ｆ、ｕ的１１个公式外，还根据Ｗ．Ｈｏｒｎ的ｊ．ｖ模型，利用Ｄ．Ｅ．Ｃａｒｔｗｒｉｇｈｔ新的引潮势展开推出５９个ｊ、ｖ公式，后者理论上更为精确，它反映了近代天文学研究进展的成就。平均海面提出一种随机动态分析、预测模型，能比较可靠地求出平均海面长期变化趋势，并能对未来几年内作出月平均海面的预报。潮波理论结合中国海实际，研究潮汐摩擦规律及其效应，已能说明中国海主要分潮波系统的形成及其分布变化，潮波数值计算和模拟取得很大的发展，有些在建港和海洋开发利用中已经得到应用，是一种很有前途的研究方法。潮汐表的编算水平高、范围遍及各国主要海港，受到用户的欢迎。总起来说，我国海洋潮汐的研究工作，经４０年来的努力，从总体上说达到了国际水平，某些方面居领先地位。但整个潮汐的观测站网、仪器装备、监测水平和精度，仍有待改进提高。 相似文献
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建立潮汐汊道P-A关系的沉积动力学方法 总被引：6，自引：0，他引：6
在均衡状态下，潮汐汉道系统的纳潮量(P)与口门面积(A)之间存在着较稳定的关系，通常用幂函数形式来表达。计算P-A关系的传统O’Brien方法因其统计性质无法给出单一潮汐汉道的P-A关系。根据沉积动力学原理，每个潮汐汉道的P-A关系都受涨落潮历时、断面平均流速、口门形态、纳潮量、淡水径流量、沿岸毛输沙量和沉积物粒度等因素的控制，对上述因素的每一种组合，都有对应的均衡态P-A关系。作者在前人工作的基础上，尝试着建立了计算单一潮汐汊道P-A关系的沉积动力学方法，并以山东半岛月湖为算例对该方法的应用进行了讨论。结果表明，均衡态潮汐汉道的P-A关系的指数n稳定在1．15左右，而系统C的变化较大。 相似文献
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采用POM海洋模式模拟了渤海潮汐的主要特征。4个主要天文分潮的计算结果与实测吻合较好,在此基础上进一步探讨了渤海3个主要浅水分潮的基本特征。根据模式计算结果发现:渤海M_4和MS_4潮波传播特征类似,均存在5个潮波系统,其中4个为逆时针旋转,1个为顺时针旋转,与前人的研究成果比较一致。此外,根据浅水分潮和产生浅水分潮的源分潮的关系式推算得到MS_4分潮的振幅和迟角,与直接通过调和分析得到MS_4分潮的振幅和迟角进行对比,结果也是比较符合。针对M_6分潮在渤海传播特征进行分析,发现:本海域存在7个M_6分潮无潮点,其中4个为逆时针旋转,3个为顺时针旋转。计算结果还发现:3个浅水分潮都是在近岸浅水海域振幅相对较大,这显然与浅水分潮的产生机制密切相关。 相似文献
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海面水位各种高度的出现频率在海洋工程和航运中具有重要意义。为了得出其分布，最直接和可靠的方法当然是利用长期实测资料进行统计。但是在需要获得水位分布的地点往往没有足够长期的资料，这时就必须采用其他的方法来推算。
我国近海引起水位升降的主要因素是天文潮，故利用潮汐调和常数推算天文潮并考虑到到非天文因素的水位变化是一个比较可靠的办法。这个方法比较准确，但需要进行潮汐预报，计算量比较大。本文提出的方法所涉及的计算量很小，但仍能获得较好的效果。这个方法的基本出发点是：由于不同地点海面水位分布有一定的共性，水位分布和它的数字特征之间有密切的关系，而数字特征又决定于潮汐调和常数及非天文水位标准差，因而可利用潮汐调和常数及非天文水位标准差求得数字特征，然后进一步得出水位分布。这个方法所用到的数字特征为标准差、偏度和峰度，它们汉语拼音的第一个字母分别为B,P和F，故这个方法被称为BPF 法。
1977年我们提出 BPF 法时，主要应用于海图深度基准面，应用中的有关问题将另文讨论。 相似文献
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潮汐“波面”分析法 总被引：2，自引：0，他引：2
黄祖珂 《山东海洋学院学报》1980,10(4):1-12
本文提出的潮汐分析方法是在半图解法基本原理的基础上发展起来的一种方法。它利用34天的潮汐资料，依据坐标公式在“潮汐波面”上计算出720个非整点的潮高值，对这些潮高值分族后再按照严格的最小二乘法求得75个分潮的调和常数，得到了比较好的结果。 相似文献
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本文根据闽江下游有潮区的潮汐特性,应用1957—1981年的年平均潮差资料,建立了其年平均潮差与天文因素M_2分潮节点因子f_(M2)的线性回归方程,井用统计方法计算出年最大潮差,且分析了该潮差沿程变化的影响因素。 相似文献
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在渤海选用了82个强天气过程,利用三维模式模拟了海区的天文-风暴潮,模式经实测资料检验,获得了较满意的模拟结果。根据渤海沿岸主要验潮站观测年极值高(低)水位和年极值风增(减)水所得到的多年一遇高(低)水位和多年一遇风增(减)水,以及天文最高(最低)潮位,建立了由多年一遇风增(减)水和天文最高(最低)潮位的线性组合计算多年一遇高(低)水位的计算公式,并以此公式推算了渤海海区5个典型地区的多年一遇高(低)水位,供海洋工程设计时使用。 相似文献
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In this paper, tidal data of 19 years were analysed to obtain the harmonic constants of 472 constituents; yearly variations of the harmonic constants of some constituents for 19 years were also examined.We have also derived the formulae of response analysis by using another approach, and calculated 161 response weights of astronomical tides, solar radiational tides and nonlinear tides for 10 stations. Some significant results were obtained. 相似文献
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The sea level variations along Visakhapatnam coast are governed by astronomical tides and nontidal oscillations including atmospheric pressure, winds, coastal currents, Ekman Pumping, and river influx. Tidal and nontidal sea level oscillations are usually studied separately because of the vastly different ways in which they are forced. In this study the tidal oscillations along Visakhapatnam are analyzed using GOTIC2 tidal model. The correlation between monthly mean sea level and monthly mean tides is 47% (r = 0.68) and increases to 54% (r = 0.74) when applied for inverse-barometric effect. The major six partial tides are computed and presented. The tidal variations from Neap tide to Spring tide are studied. 相似文献
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深圳海域潮汐海啸波耦合数值研究 总被引：3，自引：0，他引：3
以COMCOT海啸模式和TPXO7.1全球潮汐模式为基础,采用三层嵌套网格,建立了南海海啸与潮汐耦合计算模型,分析深圳海域海啸和潮汐相互作用。潮汐计算结果与实测数据吻合较好,高、低潮位平均误差小于15 cm,20 cm;在潮汐验证的基础上,以马尼拉海沟潜在地震海啸源为案例,进行8.0,9.0级地震海啸与潮汐耦合情景模拟计算,计算结果表明,9级地震海啸在深圳海域外海波高为140~150 cm,如先行波为正波发生在高潮时将产生异常高潮位,负波发生在低潮时将产生异常低潮位,线性叠加计算结果偏大,在25.0 cm之内,到达时间差异小于6 min。 相似文献
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基于潮汐表数据同化的天文潮数值预报模型及其模拟预报效果 总被引：1，自引：0，他引：1
潮汐表是利用长期潮汐观测结果经调和分析实现的主要港湾潮汐预报结果,具有较高的预报精度,而通常的天文潮数值预报目前还难以达到潮汐表的预报精度.本研究在建立常规天文潮数值预报模型的基础上,建立了基于潮汐表数据同化的天文潮数值预报模型,并分别采用这2种模型预报福建沿岸海域的天文潮.其结果表明同化模型的预报结果无论是在潮时还是在潮高均明显优于常规模型;同化模型能显著地改善所研究的沿岸海域90个水位点中至少45个水位点的潮汐预报结果,而其他水位点的预报结果也有不同程度地改善. 相似文献
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The coast of Zhejiang Province is a zone of maximum tidal ranges in China. One of the causes is the influence of the adjacent continental shelf. A model is presented in this paper, whose theory suggests that the amplitudes of semidiurnal tides should be amplified on the southern continental shelf of the East China Sea, while those of diurnal tides should not. The values computed from the equations are basically in agreement with observations. 相似文献
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Open coast storm surge water levels consist of wind setup due to wind shear at the water surface; a wave setup component caused by wind induced waves transferring momentum to the water column; an atmospheric pressure head component due to the atmospheric pressure deficit over the spatial extent of the storm system; a Coriolis forced setup or setdown component due to the effects of the rotation of the earth acting on the wind driven alongshore current at the coast; a possible seiche component due to resonance effects initiated by moving wind system, and, if astronomical tides are present, an astronomical tide component (although the tide is typically considered to be a forced astronomical event and not really a direct part of the external wind-driven meteorological component of storm surge). Typically the most important component of a storm surge is the wind setup component, especially on the U.S. East Coast and the Gulf of Mexico shorelines. In many approaches to storm surge modeling, a constant depth approximation is invoked over a limited step size in the computational domain. The use of a constant depth approximation has received little attention in the literature although can be very important to the resulting magnitude of the computed storm surge. The importance of discrete step size to the wind setup storm surge component is considered herein with a simple case computation of the wind setup component on a linear slope offshore profile. The present study findings show that the constant depth approximation to wind setup storm surge estimation is biased on the low side (except in extremely shallow water depths) and can provide large errors if discrete step size is not sufficiently resolved. Guidance has been provided on the error that one might encounter for various step sizes on different slopes. 相似文献
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J.M. Knight P.E.R. Dale R.J.K. Dunn G.J. Broadbent C.J. Lemckert 《Estuarine, Coastal and Shelf Science》2008
Tidal flooding and surface drainage patterns have often been used to describe mangrove species zonation. However, in mangrove forests exhibiting little topography, ambiguous species distributions and/or few species, such approaches are ineffective. We identified four physiognomic mangrove forest types (Riverine, Fringing, Overwash and Basin) at Coombabah Lake, a tidal lake in southeast Queensland, Australia and investigated tidal flooding patterns using synoptic surveys of tidal observations at the local Standard Port combined with local water depth observation. Subsequently three sub-types of the basin forest type were identified: (1) Deep Basin Forest with mature trees, ∼50 cm standing water and ∼3 tides per year; (2) Medium Depth Basin Forest with intermediate tree development, ∼15–30 cm standing water and 20–40 tides per year; and (3) Shallow Basin Forest with relatively recent mangrove establishment, 5–15 cm standing water and ∼80 tides per year. These three basin sub-types were found to flood at different tide heights with the Shallow Basin flooding for tides above mean high water springs and the Deep Basin flooding only for tide heights approaching the highest astronomical tide. We propose that these basin types represent a succession in mangrove forest development that corresponds with increasing water depth and tree maturation over time. The succession not only represents increasing age but also change in basin substrate composition. This is manifest as increasing pneumatophore density and an increasing area of basin surface occupied by contiguous pneumatophore cover. As a result, it seems that mangrove development is able to modify tidal flooding into the basin by increasingly impeding water movement. 相似文献
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长江口受台风影响严重,台风风暴潮、上游洪峰及天文大潮相遇将致使长江下游至长江口水位暴涨,对沿岸至河口的防汛安全构成严重威胁。基于ADCIRC模型构建东中国海至长江口风暴潮数学模型,模拟9711号台风和0012号台风两场典型台风水位过程。以典型台风为基础构成多种台风路径,分析不同登陆位置和走向对长江沿线风暴增水影响。研究大洪水、不同路径台风、天文大潮共同影响下长江下游沿线风暴增水分布规律。结果表明:登陆位置处于长江口南侧情况下长江河道沿线增水大于正面登陆长江口和北侧登陆型台风;平行于长江河道方向移动的台风造成沿线增水大于斜向穿越长江口的台风,不同台风走向对于风暴增水影响程度小于登陆位置;台风风暴潮、上游洪峰及天文大潮“三碰头”情形下长江沿线增水分布呈单峰型,从大通至江阴不断增大,江阴至中浚维持高位,中浚至口外迅速减小。 相似文献
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《Deep Sea Research Part I: Oceanographic Research Papers》2001,48(6):1375-1399
Semidiurnal tides, and especially the lunar tide M2, are dominant dynamics in the Bay of Biscay. Strong tidal currents are associated with the presence of a significant continental slope. By combining Newton's gravitation laws and Euler's equations, Laplace's equations contain the astronomical forcing responsible for the observed semidiurnal tides. In shallow waters, this direct forcing is often neglected. We study here its influence on the tidal dynamics over the continental slope through the development of a simple model describing the barotropic semidiurnal dynamics on a transect perpendicular to the slope. This new model results from the combination of two different models, i.e. the one developed by Rosenfeld and Beardsley (1987), which takes into account the tide-generating force, and that of Battisti and Clarke (1982), which neglects it. A first model is developed by neglecting the direct astronomical forcing in equations: it consists in solving a second-order homogeneous propagation equation for the barotropic semidiurnal tide and needs only coastal conditions as well as the knowledge of the along-slope wave number of the solution. For a mean slope typical of the South Brittany area, this non-forced model provides results in accordance with those of Battisti and Clarke and Le Cann (1990): in particular, in the upper part of the slope, it shows a polarization inversion of tidal ellipses characteristic of the tidal dynamics observed in this area. Then, the direct astronomical forcing is kept in equations. The simple model developed without this forcing is fitted in order to solve the resulting forced propagation equation for the barotropic tide. The solution of this second model is the sum of a forced wave responding to the direct astronomical forcing and of a free wave generated at the coastal boundary. Under the same boundary conditions, the results obtained with the influence of the tide-generating force are then compared with those obtained without it. This comparison allows one to apprehend the importance of the direct astronomical forcing on tidal dynamics across the slope: in particular, the main difference appears in deep waters where this forcing induces a phase-lag between the plain and the shelf for the sea-surface slope. 相似文献