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Sound Speed Structure Long-term Monitoring in Antarctica by the Deep-sea Automatic Observation Float

机译:深海自动观测浮标在南极的声速结构长期监测

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摘要

Indirect observation to convert the sound speed has been carried out as a method of observing the ocean acoustic environment from water temperature and salinity observed in the mooring buoy and ship observations. However, there is a problem in that these have both high initial cost and running cost. Therefore, to address these issues, a study of the wide area ocean sound observation system using the observation data from a marine automatic observation float was performed. To capture in detail the changes in the ocean acoustic environment due to recent climate change, however, it is necessary to observe areas of the deep sea that can not be detected by Argo floats. Also, during the season when the Antarctic Ocean is frozen, continuous observation data of the deep sea cannot be acquired, and water temperature, salinity, and sound speed structure are not clear. As a result, JAMSTEC developed a new profiling float, called the “Deep NINJA” for deep-sea observations. The float was subjected to a yearlong monitoring of the Antarctic Ocean off the Adelie Coast in 2012. For the first time, it succeeded in monitoring long-term the sound speed profile to a depth of 4000 m in the Antarctic Ocean, and was able to capture a seasonal change in the surface area in the freezing and thawing seasons. In addition, by calculating sound speed from these data, simulations were performed assuming low-frequency sonar. The results obtained the ingredient that propagates while repeating a reflection in the extremely small layer of the sea surface neighborhood, and the ingredient that propagates while being reflected near a water depth of 100 m, which changes the sound speed gradient. From this, propagation loss was found to be smaller in winter than summer, and the possibility that a sound wave would propagate to a more distant place was demonstrated. This may affect the long-distance sound wave propagation of the echolocations of passive sonar and marine mammals.
机译:作为从在系泊浮标和船舶观测中观测到的水温和盐度观测海洋声环境的方法,已经进行了间接观测以转换声速。然而,存在一个问题,即它们具有较高的初始成本和运行成本。因此,为了解决这些问题,使用来自海洋自动观测浮标的观测数据进行了广域海洋声音观测系统的研究。为了详细捕获由于最近的气候变化而导致的海洋声学环境的变化,但是,有必要观察Argo浮标无法检测到的深海区域。另外,在南极冻结的季节中,无法获取深海的连续观测数据,水温,盐度和声速结构也不清楚。结果,JAMSTEC开发了一种新的剖面浮标,称为“深NINJA”,用于深海观测。 2012年,对浮标进行了为期一年的对阿德利海岸外南极海洋的监测。它首次成功地对南极洋中4000 m深度的长期声速剖面进行了监测,并能够在冷冻和解冻季节捕获表面积的季节性变化。另外,通过从这些数据计算声速,在假定低频声纳的情况下进行了模拟。结果获得了在海面附近的极小层中重复反射时传播的成分,以及在100 m的水深附近反射时传播的成分,这改变了声速梯度。据此,发现冬天的传播损失比夏天小,并且证明了声波传播到更远的地方的可能性。这可能会影响被动声纳和海洋哺乳动物回声位置的长距离声波传播。

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