A dynamically based method for estimating the Atlantic meridional overturning circulation at 26° N from satellite altimetry

Sanchez-Franks, Alejandra ORCID: https://orcid.org/0000-0002-4831-5461; Frajka-Williams, Eleanor ORCID: https://orcid.org/0000-0001-8773-7838; Moat, Ben I. ORCID: https://orcid.org/0000-0001-8676-7779; Smeed, David A. ORCID: https://orcid.org/0000-0003-1740-1778. 2021 A dynamically based method for estimating the Atlantic meridional overturning circulation at 26° N from satellite altimetry. Ocean Science, 17 (5). 1321-1340. 10.5194/os-17-1321-2021

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Official URL: http://dx.doi.org/10.5194/os-17-1321-2021

Abstract/Summary

The large-scale system of ocean currents that transport warm waters in the upper 1000 m northward and return deeper cooler waters southward is known as the Atlantic meridional overturning circulation (AMOC). Variations in the AMOC have significant repercussions for the climate system; hence, there is a need for long-term monitoring of AMOC fluctuations. Currently the longest record of continuous directly measured AMOC changes is from the RAPID-MOCHA-WBTS programme, initiated in 2004. The RAPID programme and other mooring programmes have revolutionised our understanding of large-scale circulation; however, by design they are constrained to measurements at a single latitude and cannot tell us anything pre-2004. Nearly global coverage of surface ocean data from satellite altimetry has been available since the launch of the TOPEX/Poseidon satellite in 1992 and has been shown to provide reliable estimates of surface ocean transports on interannual timescales including previous studies that have investigated empirical correlations between sea surface height variability and the overturning circulation. Here we show a direct calculation of ocean circulation from satellite altimetry of the upper mid-ocean transport (UMO), the Gulf Stream transport through the Florida Straits (GS), and the AMOC using a dynamically based method that combines geostrophy with a time mean of the vertical structure of the flow from the 26∘ N RAPID moorings. The satellite-based transport captures 56 %, 49 %, and 69 % of the UMO, GS, and AMOC transport variability, respectively, from the 26∘ N RAPID array on interannual (18-month) timescales. Further investigation into the vertical structure of the horizontal transport shows that the first baroclinic mode accounts for 83 % of the interior geostrophic variability, and the combined barotropic and first baroclinic mode representation of dynamic height accounts for 98 % of the variability. Finally, the methods developed here are used to reconstruct the UMO and the AMOC for the time period pre-dating RAPID, 1993 to 2003. The effective implementation of satellite-based method for monitoring the AMOC at 26∘ N lays down the starting point for monitoring large-scale circulation at all latitudes.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.5194/os-17-1321-2021
ISSN:	1812-0792
Date made live:	28 Sep 2021 15:53 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/531122

Item Type:

Publication - Article

Digital Object Identifier (DOI):

10.5194/os-17-1321-2021

ISSN:

1812-0792

Date made live:

28 Sep 2021 15:53 +0 (UTC)

URI:

https://nora.nerc.ac.uk/id/eprint/531122