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Hadley Circulation Response to Orbital Precession. Part I: Aquaplanets

Merlis, Timothy M. and Schneider, Tapio and Bordoni, Simona and Eisenman, Ian (2013) Hadley Circulation Response to Orbital Precession. Part I: Aquaplanets. Journal of Climate, 26 (3). pp. 740-753. ISSN 0894-8755. doi:10.1175/JCLI-D-11-00716.1. https://resolver.caltech.edu/CaltechAUTHORS:20130308-075759181

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Abstract

The response of the monsoonal and annual-mean Hadley circulation to orbital precession is examined in an idealized atmospheric general circulation model with an aquaplanet slab-ocean lower boundary. Contrary to expectations, the simulated monsoonal Hadley circulation is weaker when perihelion occurs at the summer solstice than when aphelion occurs at the summer solstice. The angular momentum balance and energy balance are examined to understand the mechanisms that produce this result. That the summer with stronger insolation has a weaker circulation is the result of an increase in the atmosphere’s energetic stratification, the gross moist stability, which increases more than the amount required to balance the change in atmospheric energy flux divergence necessitated by the change in top-of-atmosphere net radiation. The solstice-season changes result in annual-mean Hadley circulation changes (e.g., changes in circulation strength).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1175/JCLI-D-11-00716.1DOIUNSPECIFIED
http://journals.ametsoc.org/doi/abs/10.1175/JCLI-D-11-00716.1PublisherUNSPECIFIED
ORCID:
AuthorORCID
Schneider, Tapio0000-0001-5687-2287
Bordoni, Simona0000-0003-4771-3350
Additional Information:© 2013 American Meteorological Society. Manuscript received 6 December 2011, in final form 24 July 2012. A careful reading of Tim Merlis’s Ph.D. thesis by Andy Thompson is greatly appreciated. We thank Rob Korty and Damianos Mantsis for helpful comments on the manuscript. This work was supported by a National Science Foundation Graduate Research Fellowship, a Princeton Center for Theoretical Science Fellowship, and National Science Foundation Grant AGS-1049201. The program codes for the simulations, based on the Flexible Modeling System of the Geophysical Fluid Dynamics Laboratory, as well as the simulation results themselves, are available from the authors upon request.
Funders:
Funding AgencyGrant Number
NSF Graduate Research FellowshipUNSPECIFIED
Princeton Center for Theoretical Science FellowshipUNSPECIFIED
NSFAGS-1049201
Subject Keywords:Atmospheric circulation; Hadley circulation; Paleoclimate
Issue or Number:3
DOI:10.1175/JCLI-D-11-00716.1
Record Number:CaltechAUTHORS:20130308-075759181
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130308-075759181
Official Citation:Merlis, Timothy M., Tapio Schneider, Simona Bordoni, Ian Eisenman, 2013: Hadley Circulation Response to Orbital Precession. Part I: Aquaplanets. J. Climate, 26, 740–753. doi: http://dx.doi.org/10.1175/JCLI-D-11-00716.1
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37401
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:15 Apr 2013 19:54
Last Modified:09 Nov 2021 23:28

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