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Glider transects in the Levantine Sea: Characteristics of the warm core Cyprus eddy

机译:黎凡特海滑翔带横断面:塞浦路斯暖涡核心特征

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Beginning in March 2009, two gliders of the Oceanography Center of the University of Cyprus (OC-UCY) began occupying a hydrographic endurance line for measurements of temperature, salinity, dissolved oxygen, optical backscatter, and fluorescence in the Levantine Sea. The transects follow a butterfly pattern near the Eratosthenes Seamount, extending to a maximum depth of 1000 m. These operational transects represent the first in a time series of transects carried out by OC-UCY. In November 2009, a joint project, “Eye of the Levantine,” was carried out and in which 6 gliders were deployed to investigate the Cyprus warm core eddy observed earlier in the year by both glider and shipboard CTD. In December 2009, the TARA Oceans vessel was involved as well with CTD and water samples and the deployment of 4 surface drifters and 2 profiling floats in and around the eddy. Near the end of the experiment, the eddy was sampled again with shipboard CTD and ADCP by the Maria S. Merian in January 2010. At this time, only the OC-UCY glider continued its endurance line, which also passed through the eddy. It completed its mission in May 2010. About 2000 profiles down to 1000 m and 1000 profiles down to 200 m have been collected by the fleet of gliders including measurements of not only temperature and salinity, but also fluorescence (Chl a, CDOM) and backscatter (at 470 nm, 532 nm, 660 nm, 700 nm and 880 nm). The most recent mission (October 2010 to February 2011) revealed the same eddy approximately 80 km to the east. The Cyprus eddy is a permanent feature (since observations began), with radius of typically 45 km and tangential current speeds of approximately 0.30 m s−1. It consists of an anticyclonic core of Levantine Intermediate Water to a depth of about 400 m. The surface signature is very weak, particularly in summer, however, it is visible in maps of absolute dynamic topography. Further analysis and modeling as well as continued observations-- of the eddy are required in order to determine how it is generated and what governs its evolution and decay.
机译:从2009年3月开始,塞浦路斯大学海洋学中心(OC-UCY)的两个滑翔机开始占据水文耐力线,用于测量黎凡特海的温度,盐度,溶解氧,光学反向散射和荧光。横断面遵循Eratosthenes海山附近的蝴蝶图案,最大延伸到1000 m。这些操作样线代表了OC-UCY执行的一系列时间样中的第一个。 2009年11月,开展了一个“黎凡特之眼”联合项目,其中部署了6架滑翔机,以研究今年早些时候滑翔机和舰载CTD观测到的塞浦路斯暖芯涡。 2009年12月,TARA Oceans船也参与了CTD和水样的研究,并在涡流内部和周围部署了4个表面浮标和2个轮廓浮标。在实验即将结束时,Maria S. Merian于2010年1月再次使用船载CTD和ADCP对涡流进行了采样。这时,只有OC-UCY滑翔机延续了其耐力线,该滑行线也通过了涡流。它于2010年5月完成了任务。滑翔机队已收集了约2000个剖面(低至1000 m)和1000个剖面(低至200 m),不仅测量了温度和盐度,还测量了荧光(Chl a,CDOM)和反向散射(在470 nm,532 nm,660 nm,700 nm和880 nm处)。最近一次飞行任务(2010年10月至2011年2月)向东约80公里处露出了同一涡流。塞浦路斯涡是一个永久性特征(自观测开始以来),半径通常为45 km,切向电流速度约为0.30 m s s -1 。它由黎凡特中级水的抗气旋核心组成,深度约为400 m。表面签名非常薄弱,尤其是在夏天,但是在绝对动态地形图中可见。进一步的分析和建模以及持续的观察- -- 为了确定涡旋的产生方式以及控制涡旋的演化和衰减的过程,需要涡旋的大小。

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