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dc.contributor.authorCalleja, Maria L.
dc.contributor.authorAnsari, I, Mohd
dc.contributor.authorRostad, Anders
dc.contributor.authorSilva, Luis and Kaartvedt, Stein
dc.contributor.authorIrigoien, Xabier
dc.contributor.authorMoran, Xose Anxelu G.
dc.date.accessioned2019-06-18T11:49:13Z-
dc.date.available2019-06-18T11:49:13Z-
dc.date.issued2018
dc.identifierISI:000457360200001
dc.identifier.urihttp://dspace.azti.es/handle/24689/796-
dc.description.abstractThe vast majority of marine dissolved organic carbon (DOC), the largest reservoir of reduced carbon on Earth, is believed to accumulate in the abyssal layers of the ocean over timescales of decades to millennia. However, evidence is growing that small animals that migrate vertically every day from the surface to mesopelagic layers are significantly contributing to the active vertical flux of organic matter. Whether that represents an important source of carbon available for microbial production and respiration at the mesopelagic realm, and its contribution to oceanic carbon budgets and energy flows, is yet to be explored. Here we present data suggesting that Red Sea migrating animals may produce an overlooked source of labile DOC (used at a mean rate of 2.1 mu mol C L-1 d(-1)) that does not accumulate but fuels the metabolism in the twilight zone, generating a disregarded hotspot for heterotrophic prokaryotes.
dc.language.isoeng
dc.publisherFRONTIERS MEDIA SA
dc.subjectRed Sea
dc.subjectmesopelagic layer
dc.subjectdiet vertical migration
dc.subjectheterotrophic prokaryotes
dc.subjectdissolved organic carbon
dc.subjectVERTICAL-DISTRIBUTION
dc.subjectCARBON EXPORT
dc.subjectZOOPLANKTON
dc.subjectMIGRATION
dc.subjectBACTERIA
dc.subjectPICOPLANKTON
dc.subjectTRANSPORT
dc.subjectDYNAMICS
dc.subjectWATERS
dc.subjectMESO
dc.titleThe Mesopelagic Scattering Layer: A Hotspot for Heterotrophic Prokaryotes in the Red Sea Twilight Zone
dc.typeArticle
dc.identifier.journalFRONTIERS IN MARINE SCIENCE
dc.format.volume5
dc.contributor.funderKing Abdullah University for Science and Technology
dc.identifier.e-issn2296-7745
dc.identifier.doi10.3389/fmars.2018.00259
Aparece en las tipos de publicación: Artículos científicos



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