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Eddy Influences on Hadley Circulations: Simulations with an Idealized GCM

Walker, Christopher C. and Schneider, Tapio (2006) Eddy Influences on Hadley Circulations: Simulations with an Idealized GCM. Journal of the Atmospheric Sciences, 63 (12). pp. 3333-3360. ISSN 0022-4928. https://resolver.caltech.edu/CaltechAUTHORS:WALjas06

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Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:WALjas06

Abstract

An idealized GCM is used to investigate how the strength and meridional extent of the Hadley circulation depend on the planet radius, rotation rate, and thermal driving. Over wide parameter ranges, the strength and meridional extent of the Hadley circulation display clear scaling relations with regime transitions, which are not predicted by existing theories of axisymmetric Hadley circulations. For example, the scaling of the strength as a function of the radiative-equilibrium equator-to-pole temperature contrast exhibits a regime transition corresponding to a regime transition in scaling laws of baroclinic eddy fluxes. The scaling of the strength of the cross-equatorial Hadley cell as a function of the latitude of maximum radiative-equilibrium temperature exhibits a regime transition from a regime in which eddy momentum fluxes strongly influence the strength to a regime in which the influence of eddy momentum fluxes is weak. Over a wide range of flow parameters, albeit not always, the Hadley circulation strength is directly related to the eddy momentum flux divergence at the latitude of the streamfunction extremum. Simulations with hemispherically symmetric thermal driving span circulations with local Rossby numbers in the horizontal upper branch of the Hadley circulation between 0.1 and 0.8, indicating that neither nonlinear nearly inviscid theories, valid for Ro → 1, nor linear theories, valid for Ro → 0, of axisymmetric Hadley circulations can be expected to be generally adequate. Nonlinear theories of axisymmetric Hadley circulations may account for aspects of the circulation when the maximum radiative-equilibrium temperature is displaced sufficiently far away from the equator, which results in cross-equatorial Hadley cells with nearly angular momentum-conserving upper branches. The dependence of the Hadley circulation on eddy fluxes, which are themselves dependent on extratropical circulation characteristics such as meridional temperature gradients, suggests that tropical circulations depend on the extratropical climate.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1175/JAS3821.1DOIUNSPECIFIED
ORCID:
AuthorORCID
Schneider, Tapio0000-0001-5687-2287
Additional Information:© 2006 American Meteorological Society Manuscript received 10 November 2005, in final form 19 April 2006 We thank Dorian Abbot, Richard Lindzen, Edwin Schneider, Adam Sobel, and an anonymous reviewer for very helpful comments on an earlier version of this paper. We are grateful for financial support by the Davidow Discovery Fund, by an Alfred P. Sloan Research Fellowship, and by the National Science Foundation (Grant ATM-0450059) and for computing resources provided by the National Center for Atmospheric Research (which is sponsored by the National Science Foundation). The program code for the simulations described in this paper, as well as the simulation results themselves, are available from the authors upon request.
Issue or Number:12
Record Number:CaltechAUTHORS:WALjas06
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:WALjas06
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:6974
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:04 Jan 2007
Last Modified:02 Oct 2019 23:37

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