EGU24-5458, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-5458
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The radiative impact of the 2022 Hunga Tonga-Hunga Ha’apai stratospheric eruption: a 2-year perspective

Pasquale Sellitto1,2, Redha Belhadji1, Clair Duchamp3, Aurélien Podglajen3, Elisa Carboni4, Richard Siddans4, Corinna Kloss5, and Bernard Legras3
Pasquale Sellitto et al.
  • 1Univ. Paris Est Créteil and Université de Paris, CNRS, Laboratoire Interuniversitaire des Systèmes Atmosphériques, Institut Pierre Simon Laplace, Créteil, France
  • 2Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Etneo, Catania, Italy
  • 3Laboratoire de Météorologie Dynamique, UMR CNRS 8539, École Normale Supérieure, PSL Research University, École Polytechnique, Sorbonne Universités, École des Ponts PARISTECH, Institut Pierre Simon Laplace, Paris, France
  • 4UK Research and Innovation, Science and Technology Facilities Council, Rutherford Appleton Laboratory, Chilton, UK
  • 5Laboratoire de Physique de l’Environnement et de l’Espace, CNRS UMR 7328, Université d’Orléans, Orléans, France

The underwater Hunga Tonga-Hunga Ha’apai (HTHH) volcano erupted in the early hours of 15th January 2022 and injected volcanic gases and aerosols to over 50 km altitude. This eruption produced the largest global perturbation of stratospheric aerosols since the Pinatubo eruption in 1991 and the largest perturbation of stratospheric water vapour observed in the satellite era. Using offline radiative transfer modelling and observations, it was shown that the combined radiative effect of the water vapour and aerosol perturbations from the HTHH eruption produced a positive radiative forcing at TOA (top-of-atmosphere), leading to a net warming of the climate system, and a fast radiatively-driven plume descent, during the first month after the event (Sellitto et al., 2022). This was the first time a warming effect on the climate system and a plume sinking was linked to volcanic eruptions, which usually produce a transient cooling and a possible plume lofting. Building on these first analyses, we synthesise satellite, ground-based, in situ and radiosonde observations accumulated after 2 years since the eruption and we investigate the evolution of the radiative impacts at this temporal scale. As aerosols sedimented and the water vapour was entrained in the ascending branch Brewer–Dobson circulation, a  clear vertical separation of the stratospheric aerosol and the moisture anomaly were observed; the effect of this vertical separation on the TOA radiative forcing and localised atmospheric diabatic heating/cooling is analysed and discussed.

 

Reference:

Sellitto, P., Podglajen, A., Belhadji, R. et al. The unexpected radiative impact of the Hunga Tonga eruption of 15th January 2022. Commun Earth Environ 3, 288 (2022). https://doi.org/10.1038/s43247-022-00618-z

How to cite: Sellitto, P., Belhadji, R., Duchamp, C., Podglajen, A., Carboni, E., Siddans, R., Kloss, C., and Legras, B.: The radiative impact of the 2022 Hunga Tonga-Hunga Ha’apai stratospheric eruption: a 2-year perspective, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-5458, https://doi.org/10.5194/egusphere-egu24-5458, 2024.