https://www.nature.com/articles/s43247-025-02181-9

*Authors*
Ashok Kumar Gupta, Tushar Mittal, Kristen E. Fauria, Ralf Bennartz & Jasper
F. Kok

*27 March 2025*

*Abstract*
The 2022 Hunga volcanic eruption injected a significant quantity of water
vapor into the stratosphere while releasing only limited sulfur dioxide. It
has been proposed that this excess water vapor could have contributed to
global warming, potentially pushing temperatures beyond the 1.5 °C
threshold of the Paris Climate Accord. However, given the cooling effects
of sulfate aerosols and the contrasting impacts of ozone loss (cooling)
versus gain (warming), assessing the eruption’s net radiative effect is
essential. Here, we quantify the Hunga-induced perturbations in
stratospheric water vapor, sulfate aerosols, and ozone using satellite
observations and radiative transfer simulations. Our analysis shows that
these components induce clear-sky instantaneous net radiative energy losses
at both the top of the atmosphere and near the tropopause. In 2022, the
Southern Hemisphere experienced a radiative forcing of −0.55 ± 0.05 W m⁻²
at the top of the atmosphere and −0.52 ± 0.05 W m⁻² near the tropopause. By
2023, these values decreased to −0.26 ± 0.04 W m⁻² and −0.25 ± 0.04 W m⁻²,
respectively. Employing a two-layer energy balance model, we estimate that
these losses resulted in cooling of about −0.10 ± 0.02 K in the Southern
Hemisphere by the end of 2022 and 2023. Thus, we conclude that the Hunga
eruption cooled rather than warmed the Southern Hemisphere during this
period.

*Source: Communications earth & environment*

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