Long‐Term Temperature Impacts of the Hunga Volcanic Eruption in the Stratosphere and Above

Abstract Global average upper atmosphere temperature changes linked with the Hunga volcanic eruption (January 2022) are analyzed based on satellite measurements and compared with chemistry‐climate model simulations. Results show stratospheric cooling of −0.5 to −1.0 K in the middle and upper stratosphere during 2022 through middle 2023, followed by stronger cooling (−1.0 to −2.0 K) in the mesosphere after middle 2023. The cooling patterns follow the upward propagating water vapor (H 2 O) anomalies from Hunga, and similar behavior is found between observations and model simulations. While the stratospheric cooling is mainly due to radiative cooling from enhanced H 2 O, the mesospheric temperature changes result from ozone losses in the mesosphere, which are in‐turn driven by HO x radicals from Hunga H 2 O. Comparisons with the multi‐decade climate record show that Hunga impacts on stratospheric temperatures have similar magnitude, but opposite sign, to temperature effects from the large El Chichón (1982) and Pinatubo (1991) volcanic eruptions.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-11-04
DOI
https://doi.org/10.1029/2024gl111500
Citations
7
Primary Topic
Atmospheric Ozone and Climate
Type
article
Field-Weighted Citation Impact
2.63

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Long‐Term Temperature Impacts of the Hunga Volcanic Eruption in the Stratosphere and Above

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Atmospheric Ozone and Climate
2.63
article

Long‐Term Temperature Impacts of the Hunga Volcanic Eruption in the Stratosphere and Above

Xinyue Wang, Jon Starr, William J. Randel, Douglas Edward Kinnison, Rolando R. García
article en
7 citations

Abstract

Abstract Global average upper atmosphere temperature changes linked with the Hunga volcanic eruption (January 2022) are analyzed based on satellite measurements and compared with chemistry‐climate model simulations. Results show stratospheric cooling of −0.5 to −1.0 K in the middle and upper stratosphere during 2022 through middle 2023, followed by stronger cooling (−1.0 to −2.0 K) in the mesosphere after middle 2023. The cooling patterns follow the upward propagating water vapor (H 2 O) anomalies from Hunga, and similar behavior is found between observations and model simulations. While the stratospheric cooling is mainly due to radiative cooling from enhanced H 2 O, the mesospheric temperature changes result from ozone losses in the mesosphere, which are in‐turn driven by HO x radicals from Hunga H 2 O. Comparisons with the multi‐decade climate record show that Hunga impacts on stratospheric temperatures have similar magnitude, but opposite sign, to temperature effects from the large El Chichón (1982) and Pinatubo (1991) volcanic eruptions.

Geophysical Research LettersVol. 51(21)
NSF National Center for Atmospheric Research (US), University of Colorado Boulder (US)
National Science Foundation, National Aeronautics and Space Administration, Nuclear Safety and Security Commission, NASA Headquarters
Climate action
Openalex Percentile: Top 10%
Atmospheric Ozone and Climate
2.63
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Long‐Term Temperature Impacts of the Hunga Volcanic Eruption in the Stratosphere and Above — Xinyue Wang, Jon Starr, et al. · Geophysical Research Letters (2024) | TGRS Research Map | TGRS