2013
DOI: 10.1175/jcli-d-12-00467.1
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The Relationship between ITCZ Location and Cross-Equatorial Atmospheric Heat Transport: From the Seasonal Cycle to the Last Glacial Maximum

Abstract: The authors quantify the relationship between the location of the intertropical convergence zone (ITCZ) and the atmospheric heat transport across the equator (AHTEQ) in climate models and in observations. The observed zonal mean ITCZ location varies from 5.3°S in the boreal winter to 7.2°N in the boreal summer with an annual mean position of 1.65°N while the AHTEQ varies from 2.1 PW northward in the boreal winter to 2.3 PW southward in the boreal summer with an annual mean of 0.1 PW southward. Seasonal variati… Show more

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Cited by 359 publications
(474 citation statements)
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“…This is sufficiently small compared to the average incoming radiation flux of 341.4 W m 22 that we can consider that the model is at equilibrium and the majority of the adjustment has taken place. We note that the TOA imbalance in the PMIP2 simulations, which have been used to study the energetics of the atmosphere in glacial times (Donohoe et al 2013), has a range from 0.2 to 1.6 W m 22 . Our simulations are therefore no further from equilibrium than other similar modeling studies.…”
Section: Model Configurationmentioning
confidence: 99%
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“…This is sufficiently small compared to the average incoming radiation flux of 341.4 W m 22 that we can consider that the model is at equilibrium and the majority of the adjustment has taken place. We note that the TOA imbalance in the PMIP2 simulations, which have been used to study the energetics of the atmosphere in glacial times (Donohoe et al 2013), has a range from 0.2 to 1.6 W m 22 . Our simulations are therefore no further from equilibrium than other similar modeling studies.…”
Section: Model Configurationmentioning
confidence: 99%
“…This has two components: one due to reflections from the surface and one due to reflections from the atmosphere. In the global mean this latter term is the largest (Donohoe and Battisti 2011). Following Donohoe and Battisti (2011) we decompose the planetary albedo into these two components.…”
Section: Model Configurationmentioning
confidence: 99%
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