Observing System Simulation Experiments (OSSEs) in Support of Next-Generation NOAA Satellite Constellation

IF 6.9 1区 地球科学 Q1 METEOROLOGY & ATMOSPHERIC SCIENCES
Lidia Cucurull, Richard A. Anthes, Sean P. F. Casey, Michael J. Mueller, Andres Vidal
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Abstract

Abstract Between 2014 and 2018 the National Oceanic and Atmospheric Administration conducted the NOAA Satellite Observing System Architecture (NSOSA) study to plan for the next generation of operational environmental satellites. The study generated some important questions that could be addressed by Observing System Simulation Experiments (OSSEs). This paper describes a series of OSSEs in which benefits to numerical weather prediction from existing observing systems are combined with enhancements from potential future capabilities. Assessments include the relative value of the quantity of different types of thermodynamic soundings for global numerical weather applications. We compare the relative impact of several sounding configuration scenarios for infrared (IR), microwave (MW), and radio occultation (RO) observing capabilities. The main results are: (1) increasing the revisit rate for satellite radiance soundings produces the largest benefits, but at a significant cost by requiring an increase of the number of polar orbiting satellites from two to twelve; (2) a large positive impact is found when the number of RO soundings/day is increased well beyond current values and other observations are held at current levels of performance; (3) RO can be used as a mitigation strategy for lower MW/IR sounding revisit rates, particularly in the tropics; and (4) smaller benefits result from increasing the horizontal resolution along the track of the satellites of MW/IR satellite radiances. Furthermore, disaggregating IR and MW instruments into six evenly distributed sun-synchronous orbits is slightly more beneficial than when the same instruments are combined and collocated on three separate orbits.
支持下一代 NOAA 卫星星座的观测系统模拟实验 (OSSE)
摘要 2014 年至 2018 年期间,美国国家海洋和大气管理局开展了诺阿卫星观测系统架构(NOSA)研究,以规划下一代业务环境卫星。该研究提出了一些重要问题,可以通过观测系统仿真实验(OSSE)来解决。本文介绍了一系列 OSSE,在这些 OSSE 中,现有观测系统对数值天气预报的益处与未来潜在能力的增强相结合。评估包括不同类型的热力学探测数量对全球数值天气应用的相对价值。我们比较了几种探测配置方案对红外(IR)、微波(MW)和射电掩星(RO)观测能力的相对影响。主要结果如下(1) 提高卫星辐射探测的重访率产生的效益最大,但需要将极轨道卫星的数量从 2 颗增加到 12 颗,因此成本很高;(2) 当 RO 探测次数/天的增加远远超过目前的值,而其他观测数据保持在目前的性能水平上时,会产生很大的积极影响;(3) RO 可用作降低 MW/IR 探空重访率的缓解策略,特别是在热带地区;以及 (4) 沿卫星轨道提高 MW/IR 卫星辐射的水平分辨率所产生的效益较小。此外,将红外和兆瓦仪器分解到六个均匀分布的太阳同步轨道上比将相同的仪器合并到三个不同的轨道上更有利。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
9.80
自引率
6.20%
发文量
231
审稿时长
6-12 weeks
期刊介绍: The Bulletin of the American Meteorological Society (BAMS) is the flagship magazine of AMS and publishes articles of interest and significance for the weather, water, and climate community as well as news, editorials, and reviews for AMS members.
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