Coccolithophore fluxes in the open tropical North Atlantic: Influence of thermocline depth, Amazon water, and Saharan dust

Catarina V. Guerreiro*, Karl Heinz Baumann, Geert Jan A. Brummer, Gerhard Fischer, Laura F. Korte, Ute Merkel, Carolina Sá, Henko De Stigter, Jan Berend W. Stuut

*Corresponding author for this work

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

Coccolithophores are calcifying phytoplankton and major contributors to both the organic and inorganic oceanic carbon pumps. Their export fluxes, species composition, and seasonal patterns were determined in two sediment trap moorings (M4 at 12° N, 49°W and M2 at 14° N, 37° W) collecting settling particles synchronously from October 2012 to November 2013 at 1200m of water depth in the open equatorial North Atlantic. The two trap locations showed a similar seasonal pattern in total coccolith export fluxes and a predominantly tropical coccolithophore settling assemblage. Species fluxes were dominated throughout the year by lower photic zone (LPZ) taxa (Florisphaera profunda, Gladiolithus flabellatus) but also included upper photic zone (UPZ) taxa (Umbellosphaera spp., Rhabdosphaera spp., Umbilicosphaera spp., Helicosphaera spp.). The LPZ flora was most abundant during fall 2012, whereas the UPZ flora was more important during summer. In spite of these similarities, the western part of the study area produced persistently higher fluxes, averaging 241×107 ±76×107 coccolithsm-2 d-1 at station M4 compared to only 66×107 ±31×107 coccolithsm2 d1 at station M2. Higher fluxes at M4 were mainly produced by the LPZ species, favoured by the westward deepening of the thermocline and nutricline. Still, most UPZ species also contributed to higher fluxes, reflecting enhanced productivity in the western equatorial North Atlantic. Such was the case of two marked flux peaks of the more opportunistic species Gephyrocapsa muellerae and Emiliania huxleyi in January and April 2013 at M4, indicating a fast response to the nutrient enrichment of the UPZ, probably by wind-forced mixing. Later, increased fluxes of G. oceanica and E. huxleyi in October-November 2013 coincided with the occurrence of Amazon-River-Affected surface waters. Since the spring and fall events of 2013 were also accompanied by two dust flux peaks, we propose a scenario in which atmospheric dust also provided fertilizing nutrients to this area. Enhanced surface buoyancy associated with the river plume indicates that the Amazon acted not only as a nutrient source, but also as a surface density retainer for nutrients supplied from the atmosphere. Nevertheless, lower total coccolith fluxes during these events compared to the maxima recorded in November 2012 and July 2013 indicate that transient productivity by opportunistic species was less important than "background" tropical productivity in the equatorial North Atlantic. This study illustrates how two apparently similar sites in the tropical open ocean actually differ greatly in ecological and oceanographic terms. The results presented here provide valuable insights into the processes governing the ecological dynamics and the downward export of coccolithophores in the tropical North Atlantic.

Original languageEnglish
Pages (from-to)4577-4599
Number of pages23
JournalBiogeosciences
Volume14
Issue number20
DOIs
Publication statusPublished - 17 Oct 2017

Funding

Acknowledgements. Moorings were deployed during RV Meteor cruise M89 and recovered after 1 year during RV Pelagia cruise 64PE378 by the Royal Netherlands Institute for Sea Research (NIOZ) in the framework of the ongoing multidisciplinary projects TRAFFIC, funded by the Netherlands Organization for Scientific Research (NWO; project no. 822.01.008), and DUSTTRAF-FIC, funded by the European Research Council (ERC; project no. 311152). Lab preparation of the 1/5 split of the original sediment trap sample was conducted at the NIOZ, whereas the splitting, filtering, and SEM taxonomical analysis were performed at the Geosciences Department of the University of Bremen, Germany. The first author benefited from a Marie Curie postdoctoral fellowship supported by the University of Bremen and the European Union FP7 COFUND under grant agreement no. 600411. Regarding the satellite data used in this study, the authors would like to acknowledge the following: the MODIS Atmosphere Science Team, the Aerosol Retrieval Group, and the MODIS Adaptive Processing System (MODAPS); the NASA EOSDIS Physical Oceanography Distributed Active Archive Centre (PO.DAAC) (http://podaac.jpl.nasa.gov/SeaSurfaceSalinity/Aquarius); and the Ocean Biology Processing Group (OBPG) and the Atmosphere Archive and Distribution System (LAADS) at the NASA Goddard Space Flight Center. The CCMP version 2.0 vector wind analyses were produced by Remote Sensing Systems (www.remss.com) and the CMAP precipitation data were provided by NOAA/OAR/ESRL PSD, Boulder, Colorado, USA (http://www.esrl.noaa.gov/psd/). The authors are thankful to Leandro Ponsoni, Lluisa Cros, Oliver Knebel, and Friederike Ebersbach for their contributions during the discussion of the data and to Alex Poulton and two anonymous referees for their constructive reviews.

FundersFunder number
DUSTTRAF-FIC
European Union FP7
Netherlands Organization for Scientific Research
Seventh Framework Programme311152, 600411
European Research Council
Nederlandse Organisatie voor Wetenschappelijk Onderzoek822.01.008
Koninklijk Nederlands Instituut voor Onderzoek der Zee
Universität Bremen

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