Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean

Studied oceanographic transect across the Equatorial Atlantic is considered as a “screenshot” of suspended particulate matter distribution against a hydrographical background. The area of abnormal high suspended matter volume concentrations was found above the Sierra Leone Rise from top to bottom (e...

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Main Authors: Sivkov, Vadim, Bubnova, Ekaterina
Format: Text
Language:English
Published: 2021
Subjects:
Online Access:https://doi.org/10.5194/os-2021-45
https://os.copernicus.org/preprints/os-2021-45/
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spelling ftcopernicus:oai:publications.copernicus.org:osd94715 2023-05-15T14:02:17+02:00 Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean Sivkov, Vadim Bubnova, Ekaterina 2021-06-09 application/pdf https://doi.org/10.5194/os-2021-45 https://os.copernicus.org/preprints/os-2021-45/ eng eng doi:10.5194/os-2021-45 https://os.copernicus.org/preprints/os-2021-45/ eISSN: 1812-0792 Text 2021 ftcopernicus https://doi.org/10.5194/os-2021-45 2021-06-14T16:22:13Z Studied oceanographic transect across the Equatorial Atlantic is considered as a “screenshot” of suspended particulate matter distribution against a hydrographical background. The area of abnormal high suspended matter volume concentrations was found above the Sierra Leone Rise from top to bottom (eastern part of the transect). The suggested explanation for the anomaly is based on the ballast hypothesis whereby solid particles are incorporated as ballast into suspended biogenic aggregates, leading to increased velocities of sinking. This process is located within the Northwest African upwelling area since the plankton exposed to the Saharan dust abundance form a significant number of aggregates lately transported equatorward via Canary Current. The intermediate nepheloid layer associated with the Deep Western Boundary Current was recorded from the American Slope at the 3200–3700 m to the depth of 4300 m above the Para Abyssal Plain. Antarctic Bottom Water enriched in the suspended matter was found mostly in the troughs at 40–41° W. It was detached from the bottom, coinciding with the core of the flow due to the bottom rise (“dam”) located up-stream. The grain size of particles was in accordance with polymodal distribution – the 2–4 μm and the 8–13 μm modes. The registered rise in the percentage of the 7–21 μm-sized particles suggests the presence of the well-known coarse mode (20–60 μm) formed by aggregation of transparent exopolymer particles (mucus). Text Antarc* Antarctic Copernicus Publications: E-Journals Antarctic
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Studied oceanographic transect across the Equatorial Atlantic is considered as a “screenshot” of suspended particulate matter distribution against a hydrographical background. The area of abnormal high suspended matter volume concentrations was found above the Sierra Leone Rise from top to bottom (eastern part of the transect). The suggested explanation for the anomaly is based on the ballast hypothesis whereby solid particles are incorporated as ballast into suspended biogenic aggregates, leading to increased velocities of sinking. This process is located within the Northwest African upwelling area since the plankton exposed to the Saharan dust abundance form a significant number of aggregates lately transported equatorward via Canary Current. The intermediate nepheloid layer associated with the Deep Western Boundary Current was recorded from the American Slope at the 3200–3700 m to the depth of 4300 m above the Para Abyssal Plain. Antarctic Bottom Water enriched in the suspended matter was found mostly in the troughs at 40–41° W. It was detached from the bottom, coinciding with the core of the flow due to the bottom rise (“dam”) located up-stream. The grain size of particles was in accordance with polymodal distribution – the 2–4 μm and the 8–13 μm modes. The registered rise in the percentage of the 7–21 μm-sized particles suggests the presence of the well-known coarse mode (20–60 μm) formed by aggregation of transparent exopolymer particles (mucus).
format Text
author Sivkov, Vadim
Bubnova, Ekaterina
spellingShingle Sivkov, Vadim
Bubnova, Ekaterina
Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
author_facet Sivkov, Vadim
Bubnova, Ekaterina
author_sort Sivkov, Vadim
title Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
title_short Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
title_full Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
title_fullStr Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
title_full_unstemmed Distribution of suspended particulate matter at the equatorial transect in the Atlantic Ocean
title_sort distribution of suspended particulate matter at the equatorial transect in the atlantic ocean
publishDate 2021
url https://doi.org/10.5194/os-2021-45
https://os.copernicus.org/preprints/os-2021-45/
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source eISSN: 1812-0792
op_relation doi:10.5194/os-2021-45
https://os.copernicus.org/preprints/os-2021-45/
op_doi https://doi.org/10.5194/os-2021-45
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