Stratospheric Circulation in the Southern Hemisphere: links to tropical winds, ozone and the Hunga Eruption -Part 2: Evidence from a Global Chemistry-Climate Model
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This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
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Abstract
The Southern Hemisphere (SH) stratospheric circulation can be categorized based upon the development of a low-latitude jet (LLJ) in the upper stratosphere during winter months. We analyze the dynamics of the LLJ based on a large ensemble of chemistry-climate model simulations, supported by reanalysis data. The LLJ is associated with westerly wind anomalies in the middle and upper stratosphere during mid-winter, together with weak planetary wave activity and a slower Brewer-Dobson circulation. Circulation effects extend into the tropical upper stratosphere, where the LLJ impacts the tropical semi-annual oscillation (SAO). Additionally, the LLJ is linked to a persistent, strong polar vortex in the lower stratosphere during October–December. This cold, strong vortex is associated with decreased ozone amounts in winter and spring; ozone radiative feedbacks reinforce the cold vortex after sunlight returns in October. The 2022 Hunga eruption coincided with an anomalously strong LLJ year, and ensemble simulations of Hunga impacts show that the eruption pushed the SH winter circulation towards LLJ behavior, although the ensemble-mean forced Hunga signal is small and embedded within a large amount of stochastic variability. These results advance our understanding of how LLJ dynamics connect to the large-scale stratospheric circulation and ozone depletion, with implications for predicting polar climate and composition.