2022 年 3 月南极洲东部极端气温上升的卫星微波辐射测量结果

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Cosmic Research Pub Date : 2024-02-27 DOI:10.1134/s0010952523700612
L. M. Mitnik, V. P. Kuleshov, M. L. Mitnik, A. V. Baranyuk
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引用次数: 0

摘要

摘要 介绍了在 2022 年 3 月暖湿气流(大气河(AR))从塔斯马尼亚地区入侵的条件下,频率为 ν = 10-190 GHz 的 MTVZA-GYа 微波卫星辐射计和频率为 ν = 6-89 GHz 的 AMSR2 对南极洲东部和南大洋邻近地区的探测结果。南极洲东部海岸的自动气象站以及沃斯托克站、康科迪亚站和穹顶 CII 站都记录了 AR 导致的地表空气变暖。利用从海岸的凯西站和位于 3230 米高空的协和站发射的无线电探空仪读数,以及以距离协和站约 200 公里处为中心、直径为 200 公里的圆形区域平均亮度温度时间序列,研究了南极洲上空大气特征的变化。根据大气-杉树系统微波辐射传输模型的结果,利用协和站的无线电探空剖面估算了空气和地表温度以及大气水汽含量变化对亮度温度 Tb(ν) 变化的影响。结果表明,南极洲东部大部分地区在 89-92 千兆赫频率下 Tb(ν) 的增加主要是由枞树温度的增加引起的。在水蒸气吸收线区域,频率为 ∼176-190 GHz 的 Tb(ν) 增加是由杉杉温度和空气温湿度的增加引起的。根据在 6-48 和 88-92 GHz 大气透明度窗口频率上测量的公海亮度温度 Tb(ν),确定了风速 W、云液态水含量 Q 和大气水汽含量 V,并研究了 AR 区域参数的时变性。
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Satellite Microwave Radiometric Measurements of Extreme Temperature Rise in East Antarctica in March 2022

Abstract

The results of sensing of East Antarctica and the adjoining areas of the Southern Ocean by MTVZA-GYа microwave satellite radiometers at frequency ν = 10–190 GHz and AMSR2 at ν = 6–89 GHz in conditions of warm and humid air (an atmospheric river (AR)) invasion from the area of Tasmania area in March 2022 are presented. The surface air warming caused by AR was recorded by the Automatic Weather Station at the coast and at the Vostok, Concordia, and Dome CII stations in East Antarctica. The variability of atmospheric characteristics above Antarctica was studied using readings of radiosondes launched from the Casey station at the coast and Concordia station at a height of 3230 m and time series of brightness temperatures averaged over a circular area 200 km in diameter with the center at a distance of ~200 km from the Concordia station. The influence of air and surface temperature and atmospheric water-vapor content variations on brightness temperature Tb(ν) variations was estimated from the results of modeling of microwave radiation transfer in the atmosphere–firn system using radiosonde profiles from the Concordia station. It was shown that the increase in Tb(ν) at frequencies of 89–92 GHz of a large part of East Antarctica was caused mainly by an increase in the firn temperature. The increase at frequencies of ∼176–190 GHz in the area of the water vapor absorption line was caused by an increase of both the firn temperature and air temperature and humidity. Based on measurements of brightness temperature Tb(ν) over the open ocean at frequencies in the atmospheric-transparency windows of ∼6–48 and 88–92 GHz, wind speed W, cloud liquid-water content Q, and atmospheric water-vapor content V were determined and the temporal variability of parameters in the AR area was studied.

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来源期刊
Cosmic Research
Cosmic Research 地学天文-工程:宇航
CiteScore
1.10
自引率
33.30%
发文量
41
审稿时长
6-12 weeks
期刊介绍: Cosmic Research publishes scientific papers covering all subjects of space science and technology, including the following: ballistics, flight dynamics of the Earth’s artificial satellites and automatic interplanetary stations; problems of transatmospheric descent; design and structure of spacecraft and scientific research instrumentation; life support systems and radiation safety of manned spacecrafts; exploration of the Earth from Space; exploration of near space; exploration of the Sun, planets, secondary planets, and interplanetary medium; exploration of stars, nebulae, interstellar medium, galaxies, and quasars from spacecraft; and various astrophysical problems related to space exploration. A chronicle of scientific events and other notices concerning the main topics of the journal are also presented.
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