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Estimating Arctic sea ice thickness and volume using CryoSat-2 radar altimeter data

机译:使用CryoSat-2雷达高度计数据估算北极海冰的厚度和体积

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摘要

Arctic sea ice is a major element of the Earth's climate system. It acts to regulate regional heat and freshwater budgets and subsequent atmospheric and oceanic circulation across the Arctic and at lower latitudes. Satellites have observed a decline in Arctic sea ice extent for all months since 1979. However, to fully understand how changes in the Arctic sea ice cover impact on our global weather and climate, long-term and accurate observations of its thickness distribution are also required. Such observations were made possible with the launch of the European Space Agency's (ESA's) CryoSat-2 satellite in April 2010, which provides unparalleled coverage of the Arctic Ocean up to 88 degrees N. Here we provide an end-to-end, comprehensive description of the data processing steps employed to estimate Northern Hemisphere sea ice thickness and subsequent volume using CryoSat-2 radar altimeter data and complementary observations. This is a sea ice processor that has been under constant development at the Centre for Polar Observation and Modelling (CPOM) since the early 1990s. We show that there is no significant bias in our satellite sea ice thickness retrievals when compared with independent measurements. We also provide a detailed analysis of the uncertainties associated with our sea ice thickness and volume estimates by considering the independent sources of error in the retrieval. Each month, the main contributors to the uncertainty are snow depth and snow density, which suggests that a crucial next step in Arctic sea ice research is to develop improved estimates of snow loading. In this paper we apply our theory and methods solely to CryoSat-2 data in the Northern Hemisphere. However, they may act as a guide to developing a sea ice processing system for satellite radar altimeter data over the Southern Hemisphere, and from other Polar orbiting missions. (C) 2017 COSPAR. Published by Elsevier Ltd.
机译:北极海冰是地球气候系统的主要元素。它的作用是调节区域的热量和淡水预算,以及随后整个北极和低纬度地区的大气和海洋循环。自1979年以来,卫星一直观测到北极海冰面积下降。但是,要充分了解北极海冰覆盖量的变化如何影响我们的全球天气和气候,还需要对其厚度分布进行长期而准确的观测。 2010年4月,欧洲航天局(ESA)的CryoSat-2卫星发射,使这种观测成为可能。该卫星提供了无与伦比的北冰洋至88度的覆盖。在这里,我们提供端到端的全面描述CryoSat-2雷达高度计数据和补充观测资料用于估算北半球海冰厚度和后续体积的数据处理步骤的概述。自1990年代初以来,这是一种海冰处理器,一直在极地观测与建模中心(CPOM)进行开发。我们表明,与独立测量相比,我们的卫星海冰厚度反演中没有显着偏差。我们还通过考虑取回过程中的独立误差源,对与我们的海冰厚度和体积估计有关的不确定性进行了详细分析。每个月,不确定性的主要起因是雪深和雪密度,这表明北极海冰研究的关键下一步是发展对雪量的估计。在本文中,我们仅将理论和方法应用于北半球的CryoSat-2数据。但是,它们可以作为开发海冰处理系统的指南,以用于南半球以及其他极地轨道飞行任务的卫星雷达高度计数据。 (C)2017 COSPAR。由Elsevier Ltd.发布

著录项

  • 来源
    《Advances in space research》 |2018年第6期|1203-1225|共23页
  • 作者单位

    Univ Leeds, Sch Earth & Environm, Ctr Polar Observat & Modelling, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England;

    UCL, Dept Earth Sci, Ctr Polar Observat & Modelling, Gower St, London WC1E 6BT, England;

    Univ Leeds, Sch Earth & Environm, Ctr Polar Observat & Modelling, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Cryosphere; Sea ice; Remote sensing; Arctic;

    机译:冰冻圈;海冰;遥感;北极;

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