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Characteristics of internal waves in the South China Sea Observed by a shipboard coherent radar

机译:舰载相干雷达观测南海内部波的特征

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In 2005 and 2007, a coherent, X-band radar was deployed in the South China Sea on two different ships. In both cases, the two parabolic antennas of the radar were fixed at grazing angles of approximately 2° looking toward the bow of the ship. The radar transmitted and received through a single antenna but alternated between the two antennas approximately every half second. One antenna was horizontally polarized and the other was vertically polarized. The data were analyzed by computing normalized radar cross sections and scatterer velocities as a function of ground range and time. Surface signatures of the internal waves were obvious in both types of image and at both polarizations as regions of enhanced cross sections or scatterer velocities. The collected imagery showed that at least two different types of internal waves exist in the South China Sea: small, nearly sinusoidal trains of waves and large soliton-like waves. These different types travel at very different speeds and interact with each other. The small nearly sinusoidal waves travelled at phase speeds near 1 m/s that increased as the small wave trains were overtaken by the faster solitons. Combined with other shipboard measurements, the radar measurements yielded the widths, maximum velocities, and strain rates of the solitons as well as the dependence of phase speed on amplitude. When the speeds of both the ship and the solitons were removed, the measurements showed that soliton full-widths at half-maximum ranged from about 0.5 to 4.5 km. These widths showed a dependence on the amplitude of the soliton. The phase speeds of the solitons also depended on their amplitude, reaching 3 m/s in deep water but only about 1.2 m/s in shallow water. CTD profiles were used to estimate an interface depth for a two-layer fluid model of the propagation of the solitons. The phase speeds predicted by this model agreed well with the observed dependence of the soliton phase speed on amplitude in both shallow and de--ep water.
机译:2005年和2007年,相干的X波段雷达在南中国海部署在两艘不同的船只上。在这两种情况下,雷达的两个抛物面天线都固定在朝向船首的大约2°的掠射角处。雷达通过单个天线发送和接收,但大约每半秒在两个天线之间交替。一个天线是水平极化的,另一个是垂直极化的。通过计算归一化雷达横截面和散射速度作为地面范围和时间的函数来分析数据。内波的表面特征在两种类型的图像中和在两种极化情况下均表现为明显的横截面或散射速度增强区域。收集到的图像显示,南中国海中至少存在两种​​不同类型的内波:小的,接近正弦波的海浪和类似孤子的大波。这些不同的类型以非常不同的速度行进并且彼此交互。几乎为正弦的小波以接近1 m / s的相速度行进,随着小波列被更快的孤子所取代,该相速度增加。结合其他舰载测量,雷达测量得出孤子的宽度,最大速度和应变率,以及相速度对振幅的依赖性。当船舶和孤子的速度都消除时,测量结果表明,半最大孤子的全宽范围约为0.5至4.5 km。这些宽度显示出对孤子振幅的依赖性。孤子的相速度还取决于它们的振幅,在深水中达到3 m / s,而在浅水中达到约1.2 m / s。 CTD轮廓用于估计孤子传播的两层流体模型的界面深度。由该模型预测的相速度与所观察到的孤子相速度对浅波和去磁波幅值的依赖关系很好。 -- ep水。

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    《OCEANS 2010》|2010年|P.1-7|共7页
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