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The Cross Equatorial Transport of the Hunga Tonga-Hunga Ha'apai Eruption Plume
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  • Mark Schoeberl,
  • Yi Wang,
  • Rei Ueyama,
  • Ghassan Taha,
  • Wandi Yu
Mark Schoeberl
Science and Technology Corporation

Corresponding Author:[email protected]

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Yi Wang
Science and Technology Corporation
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Rei Ueyama
NASA Ames Research Center
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Ghassan Taha
Morgan State University
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Wandi Yu
Hampton University
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Abstract

On Jan. 15, 2022, the Hunga Tonga-Hunga Ha’apai (HT) eruption injected SO2 and water into the middle stratosphere. Shortly after the eruption, the water vapor anomaly moved northward toward and across the equator. This northward movement appears to be due to a Rossby wave forced by the excessive IR water vapor cooling. Following the early eruption stage, persistent mid-stratospheric water vapor and aerosol layers were mostly confined to Southern Hemisphere (SH) tropics (Eq. to 30°S). However, during the spring of 2022, the westerly phase of the tropical quasi-biennial oscillation (QBO) descended through the tropics. The HT water vapor and aerosol anomalies were observed to again split across the equator coincident with the descent of the QBO shear zone. This split occurred because of the enhanced meridional transport circulation associated with the QBO. Neither transport event can be reproduced using MERRA2 assimilated winds.