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The Hunga volcanic eruption in January 2022 injected extreme amounts of water vapor (H2O) and a moderate amount of the aerosol precursor sulfur dioxide (SO2) into the Southern Hemisphere (SH) stratosphere. The H2O and aerosol perturbations have persisted and dispersed throughout the atmosphere, and observations show large-scale SH stratospheric cooling, strengthening of the Antarctic polar vortex and slowing of the Brewer-Dobson circulation during 2022. Satellite measurements show substantial reductions in ozone over the SH winter midlatitudes. Ensemble chemistry-climate model simulations forced by realistic Hunga inputs of H2O and SO2 qualitatively reproduce the observed evolution of the H2O and aerosol plumes, and the model exhibits stratospheric cooling, circulation changes and ozone reductions similar to observed behavior. These studies enable understanding of circulation and chemistry impacts of the unique Hunga eruption amid internal climate variability.

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