Cooling the coldest continent: The 4 December 2021 Total Solar Eclipse over Antarctica

IF 6.9 1区 地球科学 Q1 METEOROLOGY & ATMOSPHERIC SCIENCES
René Garreaud, Deniz Bozkurt, Carl Spangrude, Tomas Carrasco-Escaff, Roberto Rondanelli, Ricardo Muñoz, Xavier M. Jubier, Matthew Lazzara, Linda Keller, Patricio Rojo
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Abstract

Abstract Total solar eclipses (TSEs) are impressive astronomical events which have attracted people’s curiosity since ancient times. Their abrupt alterations to the radiation balance have stimulated studies on “Eclipse Meteorology,” most of them documenting events in the Northern Hemisphere while only one TSE (23 November 2003) has been described over Antarctica. On 4 December 2021− just a few days before the austral summer solstice− the moon blocked the sun over the austral high latitudes, with the path of totality arching from the Weddell Sea to the Amundsen Sea, thus producing a ∼2-minute central TSE. In this work we present high resolution meteorological observations from Union Glacier Camp (80°S, 83°W), the only location with a working station under totality, and South Pole station. These observations were complemented with meteorological records from 37 surface stations across Antarctica. Notably, the largest cooling (∼5°C) was observed over the East Antarctic dome, where obscurity was ∼85% while many sectors experienced insignificant temperature changes. This heterogenous cooling distribution, at odds with the seemingly homogeneous land-surface of Antarctica, is partially captured by a simple radiative model. To further diagnose the effect of the eclipse on the surface meteorology we ran multiple pairs of simulations (eclipse-enabled and -disabled) using the Weather Research and Forecasting model (WRF). The overall pattern and magnitude of the simulated cooling agree well with the observations and reveals that, in addition to the solar radiation deficit and cloud cover, low-level winds and the height of the planetary boundary layer are key determinants of the temperature changes and their spatial variability.
冷却最冷的大陆:2021年12月4日南极洲的日全食
摘要日全食是令人印象深刻的天文现象,自古以来就吸引着人们的好奇心。它们对辐射平衡的突然改变刺激了对“日食气象学”的研究,其中大多数记录了北半球的事件,而只有一次TSE(2003年11月23日)被描述在南极洲。在2021年12月4日,也就是在南方夏至的前几天,月亮在南方高纬度地区挡住了太阳,全食的路径从威德尔海到阿蒙森海呈弧形,从而产生了大约2分钟的中央TSE。在这项工作中,我们提供了来自联合冰川营地(80°S, 83°W)的高分辨率气象观测,这是唯一一个在全食下设有工作站的地点,以及南极站。这些观测得到了南极各地37个地面站的气象记录的补充。值得注意的是,最大的降温(~ 5°C)是在南极东部穹窿观测到的,那里的暗度为~ 85%,而许多扇区经历了微不足道的温度变化。这种不均匀的冷却分布,与南极洲表面均匀的陆地表面不一致,被一个简单的辐射模型部分捕捉到。为了进一步诊断日食对地面气象的影响,我们使用天气研究与预报模型(WRF)进行了多对模拟(启用和禁用日食)。模拟变冷的总体模式和幅度与观测结果吻合良好,表明除了太阳辐射亏缺和云量外,低层风和行星边界层高度是温度变化及其空间变异的关键决定因素。
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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