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dc.contributor.authorKeil, P.
dc.contributor.authorSchmidt, H.
dc.contributor.authorStevens, B.
dc.contributor.authorByrne, M. P.
dc.contributor.authorSegura, H.
dc.contributor.authorPutrasahan, D.
dc.date.accessioned2023-08-10T11:30:17Z
dc.date.available2023-08-10T11:30:17Z
dc.date.issued2023-10-01
dc.identifier290664655
dc.identifier43b82cb6-165b-4534-b219-f314406dc883
dc.identifier85166958358
dc.identifier.citationKeil , P , Schmidt , H , Stevens , B , Byrne , M P , Segura , H & Putrasahan , D 2023 , ' Tropical tropospheric warming pattern explained by shifts in convective heating in the Matsuno-Gill model ' , Quarterly Journal of the Royal Meteorological Society , vol. 149 , no. 756 , pp. 2678-2695 . https://doi.org/10.1002/qj.4526en
dc.identifier.issn0035-9009
dc.identifier.otherRIS: urn:89A3AEEBD504109D9C8CFF7F47A77633
dc.identifier.otherORCID: /0000-0001-9019-3915/work/140362569
dc.identifier.urihttps://hdl.handle.net/10023/28139
dc.descriptionFunding: The research is supported by public funding to the Max Planck Society. H. Schmidt acknowledges support from the German Federal Ministry of Education and Research within the SOCTOC project of the ROMIC2 programme.en
dc.description.abstractHorizontal temperature gradients in the tropical free troposphere are fairly weak, and tropical tropospheric warming is usually treated as uniform. However, here we show that projected tropospheric warming is spatially inhomogeneous in CMIP6 models, as well as in a storm-resolving climate model. We relate the upper tropospheric warming pattern to sea surface temperature changes that reorganise convection and thereby cause spatial shifts in convective heating. Using the classical Gill model for tropical circulation and forcing it with precipitation changes that arise due to greenhouse gas warming we can understand and reproduce the different warming patterns simulated by a range of global climate models. Forcing the Gill model with precipitation changes from a certain region demonstrates how local tropospheric temperature changes depend on local changes in convective heating. Close to the equator anomalous geopotential gradients are balanced by the dissipation term in the Gill model. The optimal dissipation timescale to reproduce the warming pattern varies depending on the CMIP6 model, and is between 1 and 10 days. We demonstrate that horizontal advection and eddy momentum fluxes have large enough equivalent dissipation timescales to balance the gradients in geopotential and thereby shape the warming pattern. While climate models show a large spread in projections of tropical sea surface temperature and precipitation changes, our results imply that once these predictions improve, our confidence in the predicted upper tropospheric warming pattern should also increase.
dc.format.extent18
dc.format.extent11749083
dc.language.isoeng
dc.relation.ispartofQuarterly Journal of the Royal Meteorological Societyen
dc.subjectTropical circulationen
dc.subjectClimate changeen
dc.subjectTropospheric warmingen
dc.subjectConvectionen
dc.subjectSimple modelsen
dc.subjectDASen
dc.subjectSDG 13 - Climate Actionen
dc.subjectMCCen
dc.titleTropical tropospheric warming pattern explained by shifts in convective heating in the Matsuno-Gill modelen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. Centre for Energy Ethicsen
dc.identifier.doi10.1002/qj.4526
dc.description.statusPeer revieweden


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