Not exact matches
Rather than use a model - based estimate, as did Hansen (2005) and Trenberth (2009), the authors achieve this by calculating it from
observations of ocean heat content (down to 1800 metres) from the PMEL / JPL / JIMAR data sets over the period July 2005 to June 2010 - a time period dominated by the superior
ARGO - based
system.
The change of the locations of the
observations (horizontal sampling) during the past 50 years is responsible for this divergence, because Ship - based
system pre-2000 has insufficient sampling on the global ocean for instance in Southern Hemisphere, while these area begin to achieve full sampling in this century by
Argo system.
Recent ocean heat content (OHC) calculations have shown a dramatic shift during the period 2001 — 2003, which is nearly coincident with a major transition in the ocean
observation network from a ship - based
system to
Argo floats.
An observing
system serving this purpose would be one where a few critical in situ
observations, coupled with satellite
observations and the
Argo float array, provide a reliable and sustainable measure of the AMOC for decades to come.
Enhancements such as «deep
Argo», «bio-
Argo», full - depth gliders, and enhanced moored
observations should be evaluated in the context of a full - depth observing
system.
To move one step closer to understanding Earth's perturbed energy budget, we need a full depth, global ocean
observation system — a deep
Argo.