共查询到16条相似文献，搜索用时 109 毫秒
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高分一号(GF-1)光学遥感卫星的发射为海洋内波的研究提供了精细的观测资料,利用其图像高空间分辨率的优势,结合高时间分辨率的中分辨率成像光谱仪(MODIS)的匹配数据,能够对南中国海东沙岛附近的内波开展特征参量的反演。本文处理了GF-1和MODIS的准同步图像,选取东沙岛附近的相邻时刻的同一条内波进行分析,提取其空间位移,计算出内孤立波传播的群速度。分析GF-1和MODIS图像上同一条内波的灰度剖面,计算了明暗条纹间距,结合当地水深和温盐数据,应用非线性薛定谔方程反演内孤立波的振幅,探究大陆架附近内孤立波的振幅演变。研究结果表明:内孤立波的群速度在东沙岛附近向西传播过程中逐渐变小;在相似的温盐条件下,遥感图像中内波的明暗条纹间距和振幅呈现负相关,在深海区水深和振幅呈现正相关关系,在浅海区由于非线性作用增强会出现振幅随水深变小反而增大的现象。 相似文献
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基于光学遥感的安达曼海内孤立波传播速度特性研究 总被引：2，自引：1，他引：1
安达曼海内孤立波非常活跃且错综复杂，传播速度是内孤立波的重要特征参量，本文采用光学遥感手段建立了内孤立波传播速度的计算方法。收集并处理大量Terra/Aqua-MODIS遥感图像，利用两景图像追踪同一内孤立波与同一激发源产生的内孤立波波群两种方法定量研究安达曼海内孤立波传播速度。研究结果表明:安达曼海内孤立波传播速度在0.5～2.7 m/s之间，内孤立波传播方向主要受海底地形的影响，传播速度大小在传播过程中随水深变浅而呈减小的趋势，在深水区传播速度大小还呈现出季节性差异。 相似文献
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卫星遥感技术是探测海洋内孤立波的重要手段,目前提取内孤立波特征参数的工作均使用SAR图像。本文首次探讨了基于MODIS可见光图像的内孤立波信息反演方法,并对位于南海北部水深3 000m左右的内孤立波个例进行了研究,发现其振幅为124m,传播速度为3.14m/s,半波宽度为3 258m。根据潜标现场观测结果对反演得到的内孤立波信息进行了检验,结果表明,此方法具有较高的准确度,为研究南海北部深水区内孤立波提供了一条新的可行路径。 相似文献
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为研究内孤立波的地形和背景流共振机制,用地形和背景流共振机制计算了3个潜标观测的内孤立波(不同模态、不同波长)的流速和传播速度,并与观测到的内孤立波进行比较。潜标观测的第一模态内孤立波(波长分别为6.4和3.3km)都是下凹型内孤立波,2个内孤立波的传播速度约为1.4m/s、最大振幅约为48m,水平流向结构都是上层西北向、下层东南向,波长3.3km 的内孤立波波峰前后有更明显的下降流和上升流。用共振机制计算出的第一模态和第二模态纬向流速的垂向结构与观测相同,最大纬向流速出现的深度与观测一致,分别相差5和12m。用共振机制计算出的内孤立波传播速度与用 KdV 方程计算的传播速度相当,共振机制计算波速为0.66~1.21m/s,KdV 方程计算波速为0.79~1.40m/s。 相似文献
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由于大振幅非线性内波对东沙群岛附近的海上石油平台具有很大的破坏性,已有多名学者对该海域的非线性内波的
传播波速进行了研究。主要根据2009 年6 月24 日15 时40 分至25 日16 时40 分“科学一号”考察船在东沙岛东北部陆架
上K106 站进行的长达25 h的X波段雷达、温度链、ADCP 同步观测数据,在该海域利用Radon 变换技术获取了本次观测到
的内孤立波的传播速度。利用孤立波到达前30 min的ADCP流速值,计算得到内波传播方向上的背景流大小为0.04 m/s。最终
得出6月24 日22时30 分时的内孤立波传播速度为3.04 m/s,传播方向约为297毅;6 月25 日8 时30 分的内孤立波传播速度
为2.73 m/s,传播方向约为289毅;6 月25 日12 时内孤立波的传播速度为2.59 m/s,传播方向约为283毅。第一个孤立波与后
两个孤立波,在振幅和速度大小上存在明显不同,其生成机制也可能不同。 相似文献
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通过分析欧洲空间局的地球资源卫星(ERS-1/2)从1995—2010年的合成孔径雷达(SAR)图像,研究了东海内孤立波的时间分布特征,绘制了东海内孤立波的空间分布图,并且反演了个别海区内孤立波的传播速度。研究结果表明:东海内孤立波主要分布在两个海域,台湾东北部海域和长江口、杭州湾以及外舟山群岛附近海域。在这两个海域,大潮期间的强潮流有利于内孤立波的出现。在长江口及附近海域,跃层强时,内孤立波出现的概率相对较高。台湾东北部内孤立波波速约为0.6—0.8 m/s,长江口及附近海域内孤立波波速约为0.6 m/s左右。 相似文献
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基于布放在南海东北部陆坡海域的5套潜标观测到的内孤立波波列数据和孤立波扰动KdV(PKdV)理论,研究内孤立波在趋浅陆架上的传播特征。得出如下结果:1)观测到的内孤立波属于C型内孤立波,即平均重现周期为(23.41±0.31)h。2)内孤立波在西传爬坡过程中,其振幅表现为先增大后减小再增大,与该海域温跃层深度的变化趋势一致;由观测数据和理论计算得到的孤立波振幅增长率(SAGR)数值接近,表明该海域的内孤立波的振幅变化可以采用由孤立波PKdV方程导出的趋浅温跃层理论来描述。3)随着水深变浅,内孤立波传播方向向北偏移,传播速度减小,即在A,B和D站位,传播方向分别为279°,296°和301°,偏转角度达22°;传播速度分别为2.36,2.23和1.47 m/s,减小38%。 相似文献
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内孤立波是发生在密度稳定层化海水中的一种特殊的海洋内波。预测内孤立波传播难度较大。本文提出了一种方法,利用美国麻省理工学院大气环流模型（MITgcm）的内孤立波模型计算了大量模拟数据,建立数据库。采用机器学习的方法,建立一个基于支持向量机（support vector machine,SVM）的安达曼海南部内孤立波传播预测模型。最后运用安达曼海南部的Sentinel-1A合成孔径雷达（SAR）图像对内孤立波传播预测模型结果进行检验。结果表明：基于SVM的内孤立波传播时间预测模型预测的时间平均绝对百分比误差为8.43%,平均绝对误差为1.00 h。基于SVM的内孤立波到达位置预测模型预测的位置平均绝对百分比误差为0.071%,平均绝对误差为0.069°。基于SVM的内孤立波振幅预测模型预测的振幅范围为23.80~84.98 m。 相似文献
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本文利用TerraSAR-X(TSX)卫星于2010年4月22日在南海东沙岛附近海域获取的数据进行海洋内孤立波动力要素和海表流速信息的提取研究。基于TSX数据的后向散射强度信息,利用经验模态分解法得到内孤立波半波宽度,再利用两层模型法和参数化法计算得到内孤立波振幅和相速度。反演结果显示,利用参数化方法得到的振幅(约21~39 m)和两层模型法得到的相速度(约1.07 m/s)与历史实测资料较为一致。进而利用TSX的顺轨干涉数据获取研究海域内的多普勒速度,再分别采用M4S模型法和直接分离法处理,进而提取海表流速。结果显示,两种方法得到的海表流速的全场平均值较为一致,均为1.10 m/s左右。M4S模型法对流速最大值的改变量较大而直接分离法对流速最小值的改变量较大。M4S模型对内孤立波波峰线区域海表流速的修正大于无内孤立波的海域。最后,基于KdV方程计算得到内孤立波引起的表面流的流速约为0.28 m/s,对反演出的海表流速贡献占比23%。 相似文献
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基于遥感与现场观测数据的南海北部内波传播速度 总被引：2，自引：0，他引：2
南海北部是全球海洋中内波最为活跃、生成和演变机制较为复杂的海域,本文利用多源卫星遥感数据(MODIS、GF-1、ENVISAT ASAR、RADARSAT-2)和现场观测数据开展了南海北部内波传播速度的研究。通过匹配捕获同一条内波的相邻两幅遥感图像,由内波的空间位移和时间间隔反演传播速度,并以0.5°×0.5°网格给出了南海北部内波传播速度的分布图。研究结果表明,内波传播速度受背景流场、水体层结和底地形变化等多因素影响,特别是水深。在南海北部由东至西、由南至北方向,内波传播速度逐渐递减。深海区内波传播速度最大,可达3m/s以上;内波在向西大陆架传播过程中,随着水深变浅速度逐渐减慢,传播速度为1—2m/s;大陆架浅海的内波传播速度较小,仅为零点几米每秒。同时,利用Kd V方程反演了内波传播速度理论值,对遥感数据提取的内波传播速度进行了精度验证,结果较为一致。 相似文献
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The South China Sea (SCS) is a hot spot for oceanic internal solitary waves due to many factors, such as the complexity of the terrain environment. The internal solitary waves in the northern SCS mainl... 相似文献
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Oceanic pycnocline depth retrieval from SAR imagery in the existence of solitary internal waves 总被引：2，自引：1，他引：1
Oceanic pycnocline depth is usually inferred from in situ measurements. It is attempted to estimate the depth remotely. As solitary internal waves occur on oceanic pycnocline and propagate along it, it is possible to retrieve the depth indirectly in virtue of the solitary internal waves. A numerical model is presented for retrieving the pycnocline depth from synthetic aperture radar （SAR） images where the solitary internal waves are visible and when ocean waters are fully stratified. This numerical model is constructed by combining the solitary internal wave model and a two-layer ocean model. It is also assumed that the observed groups of solitary internal wave packets on the SAR imagery are generated by local semidiurnal tides. A case study in the East China Sea shows a good agreement with in situ CTD （conductivity-temperature-depth） data. 相似文献
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南海文昌地区内波振幅反演研究 总被引：3，自引：2，他引：1
The field experiment is conducted from April 16,2005 to July 20,2005 at Wenchang area east of Hainan Island(19°35'N,112°E) of China.Internal wave packets are observed frequently with thermistor chains during the experiment.Meanwhile,internal waves are also detected from a synthetic aperture radar(SAR) image on June 19,2005 and several other moderate-resolution imaging spectroradiometer(MODIS) images near a mooring position.The distance between the positive and negative peaks induced by the internal wave can be obtained from satellite images.Combined with remote sensing images and in situ data,a new method to inverse the amplitude of the internal wave is proposed based on a corrected nonlinear Schr?dinger(NLS) equation.Two relationships are given between the peak-to-peak distance and the characteristic wavelength of the internal wave for different nonlinear and dispersion coefficients.Based on the satellite images,the amplitude inversion of the internal waves are carried out with the NLS equation as well as the Kd V equation.The calculated amplitudes of the NLS equation are close to the observation amplitude which promise the NLS equation a reliable method. 相似文献
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Nonlinear internal waves(NIWs) are ubiquitous around the Kara Sea, a part of the Arctic Ocean that is north of Siberia. Three hot spot sources for internal waves, one of which is the Kara Strait, have been identified based on Envisat ASAR. The generation and evolution of the NIWs through the interactions of the tide and topography across the strait is studied based on a nonhydrostatic numerical model. The model captures most wave characteristics shown by satellite data. A typical inter-packets distance on the Barents Sea side is about 25 km in summer, with a phase speed about 0.65 m/s. A northward background current may intensify the accumulation of energy during generation, but it has little influence on the other properties of the generated waves. The single internal solitary wave(ISW) structure is a special phenomenon that follows major wave trains, with a distance about 5–8 km. This wave is generated with the leading wave packets during the same tidal period. When a steady current toward the Kara Sea is included, the basic generation process is similar, but the waves toward the Kara Sea weaken and display an internal bore-like structure with smaller amplitude than in the control experiment. In winter, due to the growth of sea ice, stratification across the Kara Strait is mainly determined by the salinity, with an almost uniform temperature close to freezing. A pycnocline deepens near the middle of the water depth(Barents Sea side), and the NIWs process is not as important as the NIWs process in summer. There is no fission process during the simulation. 相似文献
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J.C.B. da Silva A.L. NewJ.M. Magalhaes 《Deep Sea Research Part I: Oceanographic Research Papers》2011,58(3):229-240
Analysis of a comprehensive dataset of Synthetic Aperture Radar (SAR) images acquired over the sea area around the Mascarene Plateau in the western Indian Ocean reveals, for the first time, the full two-dimensional spatial structure of internal solitary waves in this region of the ocean. The satellite SAR images show that powerful internal waves radiate both to the west and east from a central sill near 12.5°S, 61°E between the Saya de Malha and Nazareth Banks. To first order, the waves appear in tidally generated packets on both sides of the sill, and those on the western side have crest lengths in excess of 350 km, amongst the longest yet recorded anywhere in the world's oceans. The propagation characteristics of these internal waves are well described by first mode linear waves interacting with background shear taken from the westward-flowing South Equatorial Current (SEC), a large part of which flows through the sill in question. Analysis of the timings and locations of the packets indicates that both the westward- and eastward-traveling waves are generated from the western side of the sill at the predicted time of maximum tidal flow to the west. The linear generation mechanism is therefore proposed as the splitting of a large lee wave that forms on the western side of the sill, in a similar manner to that already identified for the shelf break generation of internal waves in the northern Bay of Biscay. While lee waves should form on either side of the sill in an oscillatory tidal flow, that on the western side would be expected to be much larger than that on the eastern side because of a superposition of the tidal flow and the steady westward flow of SEC. The existence of a large lee wave at the right time in the tidal cycle is then finally confirmed by direct observations. Our study also confirms the existence of second mode internal waves that form on the western side of the sill and travel across the sill towards the east. 相似文献