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Vortex structures in the Southeastern Baltic Sea: satellite observations and concurrent measurements

机译:东南波罗的海的涡旋结构:卫星观测和并发测量

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Vortex structures of different types are common in the Southeastern Baltic Sea. Intensive western winds, a complex coastline and an absence of steady currents make this region very appealing for studying the nature of vortex processes. These processes are clearly identified from Space. We present results of a multi-year satellite monitoring of mesoscale and submesoscale vortex structures in the Southeastern part of the Baltic Sea and of supporting field studies. An important part of our work was accumulation of remote sensing data as the first step in evaluation of circulation patterns and vortex structures presented on the sea surface. An analyzed remote sensing data include color composite images from MSI Sentinel-2, OLI Landsat-8 and ETM+ Landsat-7 as well as radar images from Sentinel-1 and Radardsat-2 that also provide a powerful tool for an identification of circulation processes on the sea surface. Continuous monitoring of the Southeastern Baltic Sea with an analysis of satellite visual and radar images show that the Gulf of Gdansk is the most frequent area with mesoscale and submesoscale eddies. They appear in this area mostly in summer and mainly under the atmospheric influence. Some eddies remain stable for at least of 8 days and could be easily tracked on color composite images. The other area of the vortex structure was determined to the north of the Cape Taran. In summer months from 2014 to 2018, we performed oceanographic concurrent experiments in the southeastern part of the Baltic Sea. Field studies of spatial and temporal characteristics of vortex structures proved results found by an analysis of satellite images.
机译:不同类型的涡旋结构在东南波罗的海海域常见。密集的西风,复杂的海岸线和缺乏稳定的电流使这个区域非常有吸引力,用于研究涡流过程的性质。这些过程清楚地从空间中识别出来。我们展示了波罗的海东南部的Mesoscale和CumseScale涡旋结构的多年卫星监测的结果,并支持实地研究。我们作品的一个重要部分是遥感数据的积累作为评估海面上呈现的循环模式和涡旋结构的第一步。被分析的遥感数据包括从彩色合成图像MSI哨兵-2,OLI陆地卫星-8和ETM +陆地卫星-7以及从哨兵-1和Radardsat-2雷达的图像,也可用于循环过程对的识别提供了有力的工具海面。持续监测东南波罗的海,分析卫星视觉和雷达图像显示,格但斯克的海湾是Mesoscale和亚源镜头最常见的区域。它们主要在夏季出现在这个区域,主要是在大气影响下。一些漩涡至少在8天内保持稳定,并且可以在彩色复合图像上轻松跟踪。涡旋结构的另一个区域被确定为塔兰披港的北部。在2014年至2018年的夏季,我们在波罗的海的东南部进行了海洋同时的实验。涡旋结构的空间和时间特征的现场研究证明了卫星图像分析的结果。

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