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Abstract The January 2022 eruption of Hunga Tonga‐Hunga Ha'apai (HTHH) injected a huge amount (∼150 Tg) of water vapor (H 2 O) into the stratosphere, along with small amount of SO 2 . An off‐line 3‐D chemical transport model (CTM) successfully reproduces the spread of the injected H 2 O through October 2023 as observed by the Microwave Limb Sounder. Dehydration in the 2023 Antarctic polar vortex caused the first substantial (∼20 Tg) removal of HTHH H 2 O from the stratosphere. The CTM indicates that this process will dominate removal of HTHH H 2 O for the coming years, giving an overall e‐folding timescale of 4 years; around 25 Tg of the injected H 2 O is predicted to still remain in the stratosphere by 2030. Following relatively low Antarctic column ozone in midwinter 2023 due to transport effects, additional springtime depletion due to H 2 O‐related chemistry was small and maximized at the vortex edge (10 DU in column).
Zhou et al. (Sat,) studied this question.