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首页> 外文期刊>Geophysical Research Letters >Synergistic surface current mapping by spaceborne stereo imaging and coastal HF radar
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Synergistic surface current mapping by spaceborne stereo imaging and coastal HF radar

机译:星载立体成像和沿海高频雷达的协同表面电流测绘

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[1] Well validated optical and radar methods of surface current measurement at high spatial resolution (nominally <100 m) from space can greatly advance our ability to monitor earth's oceans, coastal zones, lakes and rivers. With interest growing in optical along-track stereo techniques for surface current and wave motion determinations, questions of how to interpret such data and how to relate them to measurements made by better validated techniques arise. Here we make the first systematic appraisal of surface currents derived from along-track stereo Sun glitter (ATSSG) imagery through comparisons with simultaneous synoptic flows observed by coastal HF radars working at frequencies of 13.9 and 24.5 MHz, which return averaged currents within surface layers of roughly 1 m and 2 m depth respectively. At our Tsushima Strait (Japan) test site, we found that these two techniques provided largely compatible surface current patterns, with the main difference apparent in current strength. Within the northwest (southern) comparison region, the magnitudes of the ATSSG current vectors derived for 13 August 2006 were on average 22% (40%) higher than the corresponding vectors for the 1-m (2-m) depth radar. These results reflect near-surface vertical current structure, differences in the flow components sensed by the two techniques and disparities in instrumental performance. The vertical profile constructed here from ATSSG, HF radar and ADCP data is the first to resolve downwind drift in the upper 2 m of the open ocean. The profile e-folding depth suggests Stokes drift from waves of 10-m wavelength visible in the images.
机译:[1]经过验证的光学和雷达方法能够以很高的空间分辨率(标称<100 m)从地面测量电流,可以大大提高我们监测地球的海洋,沿海地区,湖泊和河流的能力。随着对沿表面电流和波动确定的光学沿航迹立体声技术的兴趣日益浓厚,出现了有关如何解释此类数据以及如何将其与通过更好验证的技术进行的测量相关的问题。在这里,我们通过沿海岸立体雷达在13.9和24.5 MHz频率下观测到的同步天气流进行比较,对沿轨道立体声太阳闪光(ATSSG)图像得出的地表电流进行了首次系统化评估,这些流向返回的是表层的平均电流。深度分别约为1 m和2 m。在我们的对马海峡(日本)测试现场,我们发现这两种技术提供了大致兼容的表面电流模式,主要区别在于电流强度。在西北(南部)比较区域内,2006年8月13日导出的ATSSG当前矢量的幅度平均比1米(2米)深度雷达的相应矢量高22%(40%)。这些结果反映了近地表垂直电流结构,两种技术检测到的流量分量的差异以及仪器性能的差异。由ATSSG,HF雷达和ADCP数据构建的垂直剖面是第一个解决公海2 m处顺风漂移的问题。轮廓的电子折叠深度表明斯托克斯偏离了图像中可见的10米波长的波。

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