English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Conference Paper

Temperature perturbation of the summer middle atmosphere after a strong volcanic eruption in UA-ICON simulations

Authors

Wallis,  Sandra
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Schmidt,  Hauke
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

von Savigny,  Christian
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

External Ressource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in GFZpublic
Supplementary Material (public)
There is no public supplementary material available
Citation

Wallis, S., Schmidt, H., von Savigny, C. (2023): Temperature perturbation of the summer middle atmosphere after a strong volcanic eruption in UA-ICON simulations, XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) (Berlin 2023).
https://doi.org/10.57757/IUGG23-0667


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5016815
Abstract
Sulfur dioxide can be injected directly into the stratosphere during and after explosive tropical volcanic eruptions. There, it mostly converts to sulfate aerosol leading to a warming of the lower stratosphere that can alter the stratospheric circulation. The impact of such events on the stratosphere is well known, but the response of the mesosphere is less understood. Few observations after the 1991 Pinatubo eruption indicate a post-volcanic mesospheric warming. The underlying dynamical mechanism behind such a phenomenon was investigated by us using the UA-ICON model. We simulated the response of the middle atmosphere to a tropical eruption that emitted twice as much sulfur dioxide as was released by the 1991 Pinatubo event. Our study found a significant warming of the polar summer mesopause of up to 15-21 K in the first austral summer after the simulated eruption. We argue that this mesospheric temperature perturbation is mainly due to vertical coupling in the summer hemisphere and potentially enhanced by interhemispheric coupling.