https://essopenarchive.org/users/523044/articles/741323-evolution-of-the-climate-forcing-during-the-two-years-after-the-hunga-tonga-hunga-ha-apai-eruption

*Authors*
Mark Robin Schoeberl,Yi Wang,Ghassan Taha,Daniel J Zawada,Rei Ueyama,
Andrew E. Dessler

*12 April 2024*

*Cite as*: Mark Robin Schoeberl, Yi Wang, Ghassan Taha, et al. Evolution of
the Climate Forcing During the Two Years after the Hunga Tonga-Hunga
Ha'apai Eruption. ESS Open Archive . April 12, 2024.
DOI:10.22541/essoar.171288896.63010190/v1

*Abstract*
We calculate the climate forcing for the two years after the January 15,
2022, Hunga Tonga-Hunga Ha’apai (Hunga) eruption. We use satellite
observations of stratospheric aerosols, trace gases and temperatures to
compute the tropopause radiative flux changes relative to climatology.
Overall, the net downward radiative flux decreased compared to climatology.
Although the Hunga stratospheric water vapor anomaly increases the downward
infrared radiative flux, the solar flux reduction due to Hunga aerosol
shroud dominates the net flux over most of the two-year period. Decreases
in temperature produced by the Hunga stratospheric circulation changes
contributes to the decrease in downward flux; however, the Hunga induced
decrease in ozone increases the net short-wave downward flux creating small
sub-tropical net flux increase in late 2022. Coincident with the aerosols
settling out, the water vapor anomaly disperses, and circulation changes
disappear so that the contrasting forcings all decrease together. By the
end of 2023, most of the Hunga induced radiative forcing changes have
disappeared. There is some disagreement in the satellite stratospheric
aerosol optical depth (SAOD) which we view as a measure of the uncertainty;
however, SAOD uncertainty does not alter our conclusion that, overall,
aerosols dominate the radiative flux changes followed by temperature and
ozone.


*Source: ESS OPEN ARCHIVE *

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