Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 49, Issue 16, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2022GL099796
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Funding
- National Oceanic and Atmospheric Administration (NOAA), U.S. Department of Commerce [NA18OAR4320123, NA19OAR0220146, NA19OAR0220147]
- Allen Institute for Artificial Intelligence
- Weather Program Office
- Office of Oceanic and Atmospheric Research, NOAA
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This study used a global storm resolving model to simulate the changes in the frequency of intense convection under different sea surface temperature conditions. The results showed that increased sea surface temperature globally enhanced the frequency of intense convection, but with significant spatial and seasonal variations. Changes in the spatial pattern of intense convection were associated with changes in planetary circulation.
Intense convection (updrafts exceeding 10 m s(-1)) plays an essential role in severe weather and Earth's energy balance. Despite its importance, how the global pattern of intense convection changes in response to warmed climates remains unclear, as simulations from traditional climate models are too coarse to simulate intense convection. Here we use a kilometer-scale global storm resolving model (GSRM) and conduct year-long simulations of a control run, forced by analyzed sea surface temperature (SST), and one with a 4 K increase in SST. Comparisons show that the increased SST enhances the frequency of intense convection globally with large spatial and seasonal variations. Changes in the spatial pattern of intense convection are associated with changes in planetary circulation. Increases in the intense convection frequency do not necessarily reflect increases in convective available potential energy. The GSRM results are also compared with previously published traditional climate model projections.
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