Seasonal constraints on inferred planetary heat content

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Seasonal constraints on inferred planetary heat content

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Title: Seasonal constraints on inferred planetary heat content
Author: McKinnon, Karen Aline ORCID  0000-0003-3314-8442 ; Huybers, Peter John

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Citation: McKinnon, Karen A., and Peter Huybers. 2016. “Seasonal Constraints on Inferred Planetary Heat Content.” Geophysical Research Letters 43 (20) (October 28): 10,955–10,964. doi:10.1002/2016gl071055.
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Abstract: Planetary heating can be quantified using top of the atmosphere energy fluxes or through monitoring the heat content of the Earth system. It has been difficult, however, to compare the two methods with each other because of biases in satellite measurements and incomplete spatial coverage of ocean observations. Here we focus on the the seasonal cycle whose amplitude is large relative to satellite biases and observational errors. The seasonal budget can be closed through inferring contributions from high-latitude oceans and marginal seas using the covariance structure of National Center for Atmospheric Research (NCAR) Community Earth System Model (CESM1). In contrast, if these regions are approximated as the average across well-observed regions, the amplitude of the seasonal cycle is overestimated relative to satellite constraints. Analysis of the same CESM1 simulation indicates that complete measurement of the upper ocean would increase the magnitude and precision of interannual trend estimates in ocean heating more than fully measuring the deep ocean.
Published Version: doi:10.1002/2016GL071055
Terms of Use: This article is made available under the terms and conditions applicable to Other Posted Material, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#LAA
Citable link to this page: http://nrs.harvard.edu/urn-3:HUL.InstRepos:33973836
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