Please use this identifier to cite or link to this item: https://accedacris.ulpgc.es/jspui/handle/10553/159702
Title: Long-term changes in air-sea heat fluxes in the North Atlantic: toward a latitudinal reorganization of the ocean heat budget
Authors: Portalés-Julià, Pedro
Machín, Francisco 
UNESCO Clasification: 251007 Oceanografía física
Keywords: Air-sea heat fluxes
Ocean heat budget
North Atlantic
Climate variability
ERA5, et al
Issue Date: 2026
Journal: Journal of Sea Research 
Abstract: This study analyzes the ocean heat budget (OHB) in the eastern North Atlantic (0°–60° N, 20° W) using monthly ERA5 data from 1980 to 2024. The four main surface fluxes—short-wave and long-wave radiation, latent and sensible heat—were examined to characterize meridional and seasonal variability, detect long-term trends, and identify their physical drivers. The OHB shows a three-zone structure: a tropical heat sink (0–20° N) dominated by short-wave input up to +250 ± 35 W m−2; a subtropical transition zone (20–40° N) where latent heat loss peaks near 30° N (∼ − 130 ± 23 W m−2); and a subpolar heat source (40–60° N) driven by wintertime turbulent fluxes exceeding −150 ± 48 W m−2. Between 1980 and 2024, sea-surface temperature rose by ∼ 0.27 ± 0.05 °C dec−1 and specific humidity by ∼ 0.20 ± 0.04 g kg−1 dec−1. Latent-heat flux trends reached +2.5 ± 1.1 W m−2 dec−1 in the subtropics, while sensible-heat flux decreased by ∼ 1 ± 0.22 W m−2 dec−1 north of 50° N. These contrasting tendencies indicate a latitudinal reorganization of air–sea heat exchange: enhanced evaporative cooling near 30° N and reduced winter heat loss at subpolar latitudes. Net short-wave radiation remains the main contributor to the OHB (32 ± 7–62 ± 5%), while latent heat flux drives most of the variability. Together, the results point to a progressive redistribution of ocean heat under ongoing climate change.
URI: https://accedacris.ulpgc.es/jspui/handle/10553/159702
ISSN: 1385-1101
DOI: https://doi.org/10.1016/j.seares.2026.102688
Source: Journal of Sea Research [ISSN 1385-1101], v. 210 (Marzo 2026)
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