天线特性对低分辨率和高分辨率卫星测高估算的海面参数的影响

IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Christopher Buchhaupt , Alejandro Egido , Salvatore Dinardo , Claire Maraldi , Thomas Moreau , Luciana Fenoglio
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引用次数: 0

摘要

在这项研究中,我们对现有的合成孔径雷达(SAR)测高信号的数值跟踪器进行了扩展,考虑了非高斯天线的特性。据我们所知,在撰写本文时,与低分辨率模式(LRM)回溯结果相比,本文提供了最一致的地球物理参数检索。该新方法是一种理论天线方向图的近似值,用三个高斯函数的和来减轻Sentinel-3A和Sentinel-6A在SAR模式下的海面高度估计误差。此外,我们解释了推导出的封闭形式方程中的偏移量,并描述了沿航迹平均水速ux(后来的平均视线速度)作为东风和北风的函数。这使我们能够减轻ux在SAR叠加中的影响,并生成了一个查找表来校正SAR模式下的海面高度估计。进一步,我们通过处理全球范围内5个月(周期72至76)的Sentinel-3A和6个月(周期17至42)的Sentinel-6A level 1A数据,讨论了这种新方法在不同天线方向图实现方面的表现。我们观察到,相对于LRM,新的重跟踪方法平均更准确。为了确保新的回调器的结果没有偏差,我们使用新的和当前最先进的方法对蒙特卡罗模拟中产生的Sentinel-3A和Sentinel-6A数据进行回调。以LRM海平面异常为参考,对模拟结果的海平面异常作为有效波高(SWH)函数的精度进行了分析。我们表明,与单一高斯近似相比,新天线表征的精度更高。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Impact of the antenna characteristics on sea surface parameters estimated from low- and high-resolution satellite altimetry
In this study, we present an extension to existing numerical retrackers of synthetic-aperture radar (SAR) altimetry signals considering a non Gaussian antenna characteristic. To our knowledge at the time of writing, this manuscript presents the most consistent retrieval of geophysical parameters compared to Low Resolution Mode (LRM) retracking results. The novelty is an approximation of the theoretical antenna pattern with a sum of three Gaussian functions to mitigate the sea surface height estimation errors for Sentinel-3A and Sentinel-6A in SAR mode. Additionally, we explain offsets in the derived closed-form equation and describe the mean along-track water velocity ux (later mean line of sight velocity) as function of eastward and northward wind This allows us to mitigate the effects of ux in a SAR stack and a lookup table is generated to correct the sea surface height estimates in SAR mode. Further on, we discuss how this new approach performs with respect to different antenna pattern implementations by processing five months (cycles 72 to 76) of Sentinel-3A and six months (cycles 17 to 42) of Sentinel-6A level 1A data on a global scale. We observe that the new retracking method is, on average, more accurate with respect to LRM. To ensure that the results of the new retracker are not biased, we retrack using the new and the current state-of-the-art method on Sentinel-3A and Sentinel-6A data produced in a Monte Carlo simulation. We analyze the simulation results with respect to the accuracy of sea level anomalies as function of the significant wave height (SWH), considering as reference the LRM sea level anomalies. We show that the accuracy of the new antenna characterization is higher compared to a single Gaussian approximation.
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来源期刊
Advances in Space Research
Advances in Space Research 地学天文-地球科学综合
CiteScore
5.20
自引率
11.50%
发文量
800
审稿时长
5.8 months
期刊介绍: The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc. NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR). All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.
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