4.5 Article

Anthropogenic Influence on the Antarctic Mesospheric Cooling Observed during the Southern Hemisphere Minor Sudden Stratospheric Warming

期刊

ATMOSPHERE
卷 13, 期 9, 页码 -

出版社

MDPI
DOI: 10.3390/atmos13091475

关键词

sudden stratospheric warming; mesospheric cooling; meteor radar; planetary waves; chemical species transport; residual mean meridional circulation

资金

  1. Korean Meteorological Administration (KMA) Research and Development Program, South Korea [KMI2020-01114]
  2. Korea Meteorological Institute (KMI) [KMI2020-01114] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

向作者/读者索取更多资源

The physical processes and impacts of sudden stratospheric warming (SSW) in the northern hemisphere have been well studied, but little is known about SSW in the southern hemisphere. By analyzing observations from various instruments, researchers found cooling in the Antarctic mesopause during a minor SSW in 2019. The cooling was attributed to the interactions between planetary waves, CO2 infrared cooling, and ozone depletion, rather than adiabatic cooling from gravity waves alone. This study highlights the importance of lower atmosphere chemistry in influencing the thermal structure of the polar mesosphere during SSW.
Processes behind Sudden Stratospheric Warming (SSW), which occurs more frequently in the northern hemispheric polar latitudes and its influence from the stratosphere to the upper atmosphere are well documented. However, physical processes associated with SSW, although it ensues rarely in the southern hemisphere (SH), have a strong influence on the background atmosphere from the stratosphere to the mesosphere and are poorly understood. Using a ground-based meteor radar, satellite-borne Microwave-Limb sounder, and Modern-Era Retrospective Analysis for Research and Applications observations, we identified cooling of Antarctic mesopause by 26 K in response to a 66 K warming in the polar stratosphere during the 2019 minor SSW in the SH. The observed cooling is attributed to the interplay between planetary waves, CO2 infrared cooling, and O-3 depletion, rather than adiabatic cooling due to gravity waves alone during SSW. It is proposed that anthropogenic and other sources generating chemical tracers in the lower atmosphere have caused mesospheric cooling and could be transported from the lower atmosphere both vertically and meridionally through residual mean meridional circulation from the tropics. Therefore, our study for the first time demonstrates the effect of lower atmosphere chemistry on the polar mesosphere thermal structure during the 2019 SSW.

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