首页> 外文会议>MTS/IEEE Conference and Exhibition on OCEANS >NEPTUNE regional observatory system design
【24h】

NEPTUNE regional observatory system design

机译:海王星区域天文台系统设计

获取原文

摘要

A team from the University of Washington (UW), the Woods Hole Oceanographic Institute (WHOI), the Monterey Bay Aquarium Research Institute (MBARI), the Jet Propulsion Laboratory (JPL), and the Institute for Pacific Ocean Science and Technology (IPOST) of Canada is jointly developing the North East Pacific Time-series Underwater Networked Experiment (NEPTUNE). NEPTUNE is being designed as a long-lived, highly reliable underwater observatory. Its basic intent is to instrument the Juan de Fuca tectonic plate, which lies just off the coasts of Washington, Oregon, and British Columbia. NEPTUNE will use standard telecommunication fiber optic cable to provide a communication and power infrastructure. A high-speed data link (up to 1 Gb/second) and high power (at least 5 kW/node) will be available at 30 nodes spaced at approximately 100-km intervals over the tectonic plate. Each node will act as a local relay point for scientific instruments and experiments that will be deployed on the sea floor and in the water column above it. The installation of such instruments will be on a "plug and play" basis, which will allow for expansion of capability as new instruments are developed and instruments that need repair or have completed their experiments are removed. The scientific investigations enabled by the NEPTUNE observatory are very diverse. This paper presents the current design of the observatory, including descriptions of the key subsystems. Innovative approaches are being developed to provide high power, broadband communications, data archiving, and accurate timing and control. The methodology for ensuring the reliability and affordability of the observatory is discussed.
机译:来自华盛顿大学(UW)的一个小组,伍兹霍尔海洋研究所(WHOI),蒙特利湾水族馆研究所(MBARI),喷气推进实验室(JPL),以及研究所太平洋科技(IPOST)加拿大共同发展东北太平洋时间系列水下网络实验(海王星)。海王星被设计为长期寿命,高度可靠的水下天文台。其基本意图是介绍Juan de Fuca构造板,它位于华盛顿,俄勒冈州和不列颠哥伦比亚省的海岸。海王星将使用标准电信光纤电缆提供通信和电力基础设施。一个高速数据链路(高至1 Gb /秒)和高功率(至少5千瓦/节点)将可在在约100公里的间隔在板块隔开30个节点。每个节点将充当本地中继点,用于科学仪器和实验,将在海底和水柱上部署。这些仪器的安装将在“即插即用”的基础上,这将允许扩展能力,因为开发了新的仪器,并删除了需要修理或已完成其实验的仪器。海王星观测所支持的科学调查非常多样化。本文介绍了天文台的当前设计,包括关键子系统的描述。正在开发创新的方法来提供高功率,宽带通信,数据归档和准确的时机控制。讨论了确保天文台可靠性和可负担性的方法。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号