Storm Track Shifts under Climate Change: What Can Be Learned from Large-Scale Dry Dynamics
- Creators
- Mbengue, Cheikh
- Schneider, Tapio
Abstract
Earth's storm tracks are instrumental for transporting heat, momentum, and moisture and thus strongly influence the surface climate. Climate models, supported by a growing body of observational data, have demonstrated that storm tracks shift poleward as the climate warms. But the dynamical mechanisms responsible for this shift remain unclear. To isolate what portion of the storm track shift may be accounted for by large-scale dry dynamics alone, disregarding the latent heat released in phase changes of water, this study investigates the storm track shift under various kinds of climate change in an idealized dry general circulation model (GCM) with an adjustable but constant convective stability. It is found that increasing the mean surface temperature or the convective stability leads to poleward shifts of storm tracks, even if the convective stability is increased only in a narrow band around the equator. Under warming and convective stability changes roughly corresponding to a doubling of CO_2 concentrations from a present-day Earthlike climate, storm tracks shift about 0.8° poleward, somewhat less than but in qualitative agreement with studies using moist GCMs. About 63% (0.5°) of the poleward shift is shown to be caused by tropical convective stability variations. This demonstrates that tropical processes alone (the increased dry static stability of a warmer moist adiabat) can account for part of the poleward shift of storm tracks under global warming. This poleward shift generally occurs in tandem with a poleward expansion of the Hadley circulation; however, the Hadley circulation expansion does not always parallel the storm track shift.
Additional Information
© 2013 American Meteorological Society. Manuscript received 10 July 2013, in final form 2 October 2013. We are grateful for the financial support provided by the National Science Foundation (Grant AGS-1019211) and for helpful discussions with Xavier Levine.Attached Files
Published - jcli-d-13-00404.1.pdf
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Additional details
- Eprint ID
- 43227
- Resolver ID
- CaltechAUTHORS:20140106-112443566
- NSF
- AGS-1019211
- Created
-
2014-01-09Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences