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Volume 11, issue 16
Biogeosciences, 11, 4541–4557, 2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
Biogeosciences, 11, 4541–4557, 2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 28 Aug 2014

Research article | 28 Aug 2014

Particle size distribution and estimated carbon flux across the Arabian Sea oxygen minimum zone

F. Roullier1,2, L. Berline1,2, L. Guidi1,2, X. Durrieu De Madron3, M. Picheral1,2, A. Sciandra1,2, S. Pesant4, and L. Stemmann1,2 F. Roullier et al.
  • 1CNRS-INSU, Laboratoire d'Océanographie de Villefranche-sur-Mer, BP 28, 06234 Villefranche-sur-Mer CEDEX, France
  • 2Université Pierre et Marie Curie-Paris 6, Observatoire Océanologique de Villefranche-sur-Mer, 06230 Villefranche-sur-Mer, France
  • 3CEFREM, CNRS-Université de Perpignan, Via Domitia, 52 avenue Paul Alduy, 66860 Perpignan, France
  • 4PANGAEA, Data Publisher for Earth and Environmental Science, University of Bremen, 28359 Bremen, Germany

Abstract. The goal of the Arabian Sea section of the TARA oceans expedition was to study large particulate matter (LPM > 100 μm) distributions and possible impact of associated midwater biological processes on vertical carbon export through the oxygen minimum zone (OMZ) of this region. We propose that observed spatial patterns in LPM distribution resulted from the timing and location of surface phytoplankton bloom, lateral transport, microbial processes in the core of the OMZ, and enhanced biological processes mediated by bacteria and zooplankton at the lower oxycline. Indeed, satellite-derived net primary production maps showed that the northern stations of the transect were under the influence of a previous major bloom event while the most southern stations were in a more oligotrophic situation. Lagrangian simulations of particle transport showed that deep particles of the northern stations could originate from the surface bloom while the southern stations could be considered as driven by 1-D vertical processes. In the first 200 m of the OMZ core, minima in nitrate concentrations and the intermediate nepheloid layer (INL) coincided with high concentrations of 100 μm < LPM < 200 μm. These particles could correspond to colonies of bacteria or detritus produced by anaerobic microbial activity. However, the calculated carbon flux through this layer was not affected. Vertical profiles of carbon flux indicate low flux attenuation in the OMZ, with a Martin model b exponent value of 0.22. At three stations, the lower oxycline was associated to a deep nepheloid layer, an increase of calculated carbon flux and an increase in mesozooplankton abundance. Enhanced bacterial activity and zooplankton feeding in the deep OMZ is proposed as a mechanism for the observed deep particle aggregation. Estimated lower flux attenuation in the upper OMZ and re-aggregation at the lower oxycline suggest that OMZ may be regions of enhanced carbon flux to the deep sea relative to non OMZ regions.

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