EGU25-4603, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-4603
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 08:30–10:15 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X4, X4.136
Polar ozone anomalies, radiative effects, and their connection to mesospheric tidal dynamics during extreme events
Guochun Shi1, Hanli Liu2, Alexander Kozlovsky3, Njål Gulbrandsen4, Dimitry Pokhotelov5, Mark Lester6, Masaki Tsutsumi7,8, Kun Wu9, and Gunter Stober1
Guochun Shi et al.
  • 1University of Bern, Institute of Applied Physics, Microwave Physics, Switzerland (guochun.shi@unibe.ch)
  • 2High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA
  • 3Sodankylä Geophysical Observatory, University of Oulu, Finland
  • 4Tromsø Geophysical Observatory UiT - The Arctic University of Norway, Tromsø, Norway
  • 5Potsdam Institute for Climate Impact Research, Member of the Leibniz Association, Potsdam, Germany
  • 6Department of Physics and Astronomy, University of Leicester, Leicester, UK
  • 7National Institute of Polar Research, Tachikawa, Japan
  • 8The Graduate University for Advanced Studies (SOKENDAI), Tokyo, Japan
  • 9School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha, China

Continuous ozone measurements above Ny-Ålesund, Svalbard (79°N, 12°E), using the ground-based microwave radiometer GROMOS-C, effectively capture the daily, seasonal, and interannual variability of polar ozone in the middle atmosphere. In this study, we analyze observed ozone changes during sudden stratospheric warming (SSW) events and compare the measurements with Aura/MLS satellite data and WACCM-X simulations. Results reveal the formation of a double-ozone layer in the stratosphere and lower mesosphere following the onset of SSW events, with ozone levels increasing by approximately 50% relative to the background value. Ozone absorbs solar UV radiation, contributing to radiative heating in the stratosphere and mesosphere. To further explore the impact of radiative ozone processes on mesospheric tide variability during SSWs, we extract diurnal (DT), semidiurnal (SDT), and terdiurnal (TDT) tidal components from zonal and meridional wind measurements recorded by meteor radars at three high-latitude stations: Sodankylä (67.37°N, 26.63°E), Tromsø (69.58°N, 19.22°E), and Svalbard (78.99°N, 15.99°E). The analysis reveals connections between tidal amplitude anomalies and radiative effects of ozone in the polar regions during SSW events. Additionally, we investigate the response of polar ozone to the May 2024 superstorm using Aura/MLS measurements and MERRA-2 reanalysis data. The results highlight a rapid and significant stratospheric ozone response following the superstorm and provide quantitative insights into the impact of such extreme events on ozone variability and UV radiation. This study underscores the critical role of ozone radiative processes in polar atmospheric dynamics and their modulation by extreme events, including SSWs and solar storms.

How to cite: Shi, G., Liu, H., Kozlovsky, A., Gulbrandsen, N., Pokhotelov, D., Lester, M., Tsutsumi, M., Wu, K., and Stober, G.: Polar ozone anomalies, radiative effects, and their connection to mesospheric tidal dynamics during extreme events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4603, https://doi.org/10.5194/egusphere-egu25-4603, 2025.