Stratospheric Climate Anomalies and Ozone Loss Caused by the Hunga Tonga‐Hunga Ha'apai Volcanic Eruption

Author:

Wang Xinyue12ORCID,Randel William2ORCID,Zhu Yunqian345,Tilmes Simone2ORCID,Starr Jon2,Yu Wandi67ORCID,Garcia Rolando2ORCID,Toon Owen B.14ORCID,Park Mijeong2ORCID,Kinnison Douglas2ORCID,Zhang Jun2ORCID,Bourassa Adam8ORCID,Rieger Landon8ORCID,Warnock Taran8ORCID,Li Jianghanyang39

Affiliation:

1. Department of Atmospheric and Oceanic Sciences University of Colorado Boulder Boulder CO USA

2. Atmospheric Chemistry Observations & Modeling Laboratory National Center for Atmospheric Research Boulder CO USA

3. Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder Boulder CO USA

4. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

5. Chemical Sciences Laboratory National Oceanic and Atmospheric Administration Boulder CO USA

6. Department of Atmospheric and Planetary Sciences Hampton University Hampton VA USA

7. Lawrence Livermore National Laboratory Livermore CA USA

8. Institute of Space and Atmospheric Studies University of Saskatchewan Saskatoon SK Canada

9. Institute of Arctic and Alpine Research University of Colorado Boulder Boulder CO USA

Abstract

AbstractThe Hunga Tonga‐Hunga Ha'apai (HTHH) volcanic eruption in January 2022 injected unprecedented amounts of water vapor (H2O) and a moderate amount of the aerosol precursor sulfur dioxide (SO2) into the Southern Hemisphere (SH) tropical stratosphere. The H2O and aerosol perturbations have persisted during 2022 and early 2023 and dispersed throughout the atmosphere. Observations show large‐scale SH stratospheric cooling, equatorward shift of the Antarctic polar vortex and slowing of the Brewer‐Dobson circulation. Satellite observations show substantial ozone reductions over SH winter midlatitudes that coincide with the largest circulation anomalies. Chemistry‐climate model simulations forced by realistic HTHH inputs of H2O and SO2 qualitatively reproduce the observed evolution of the H2O and aerosol plumes over the first year, and the model exhibits stratospheric cooling, circulation changes and ozone effects similar to observed behavior. The agreement demonstrates that the observed stratospheric changes are caused by the HTHH volcanic influences.

Funder

Climate Program Office

National Oceanic and Atmospheric Administration

National Aeronautics and Space Administration

Otto Bremer Trust

National Science Foundation

National Center for Atmospheric Research

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geophysics

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