High-resolution variability of dissolved and suspended organic matter in the Cape Verde Frontal Zone
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Frontiers
Materia
Particulate organic matter (POM) Dissolved organic matter (DOM) Colored dissolved organic matter Submesoscale Mesoscale Cape Verde Frontal Zone Carbon cycling Fluorescent dissolved organic matter (FDOM)
Fecha
2022-11-24Referencia bibliográfica
Campanero R... [et al.]. (2022) High-resolution variability of dissolved and suspended organic matter in the Cape Verde Frontal Zone. Front. Mar. Sci. 9:1006432. doi: [10.3389/fmars.2022.1006432]
Patrocinador
Spanish National Science Plan research grant FERMIO CTM2014-57334-JIN; Spanish National Science Plan research grant FLUXES CTM2015-69392-C3; European Commission eIMPACT PID2019-109084RB-C21 PID2019-109084RB-C22; Ministry of Science and Innovation, Spain (MICINN); Spanish Government BES-2016-076462 BES2016-079216 BES-2016-077949; Juan de la Cierva Formacion fellowship FJCI-641-2015-25712; European Union's Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant 834330; project SUMMER from the European Union's Horizon 2020 research and innovation program AMD-817806-5Resumen
Distributions of dissolved (DOM) and suspended (POM) organic matter, and
their chromophoric (CDOM) and fluorescent (FDOM) fractions, are investigated
at high resolution (< 10 km) in the Cape Verde Frontal Zone (CVFZ) during fall
2017. In the epipelagic layer (< 200 m), meso- and submesoscale structures
(meanders, eddies) captured by the high resolution sampling dictate the tight
coupling between physical and biogeochemical parameters at the front.
Remarkably, fluorescent humic-like substances show relatively high
fluorescence intensities between 50 and 150 m, apparently not related to
local mineralization processes. We hypothesize that it is due to the input of
Sahara dust, which transports highly re-worked DOM with distinctive optical
properties. In the mesopelagic layer (200-1500 m), our results suggest that
DOM and POM mineralization occurs mainly during the transit of the water
masses from the formation sites to the CVFZ. Therefore, most of the local
mineralization seems to be due to fast-sinking POM produced in situ or
imported from the Mauritanian upwelling. These local mineralization
processes lead to the production of refractory CDOM, an empirical evidence
of the microbial carbon pump mechanism. DOM released from these fastsinking
POM is the likely reason behind the observed columns of relatively high
DOC surrounded by areas of lower concentration. DOM and POM dynamics in the CVFZ has turned out to be very complex, in parallel to the complexity of
meso- and submesoscale structures present in the area. On top of this high
resolution variability, the input of Sahara dust or the release of DOM from
sinking particles have been hypothesized to explain the observed distributions.
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