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dc.contributor.authorTaylor, John R.
dc.contributor.authorFerrari, Raffaele
dc.date.accessioned2012-10-04T12:37:13Z
dc.date.available2012-10-04T12:37:13Z
dc.date.issued2011-12
dc.date.submitted2011-08
dc.identifier.issn0094-8276
dc.identifier.urihttp://hdl.handle.net/1721.1/73581
dc.description.abstractDensity fronts are ubiquitous features of the upper ocean. Here, numerical simulations show that restratification at fronts inhibits vertical mixing, triggering phytoplankton blooms in low-light conditions. The stability of the water column at fronts is set by a competition between frontal instabilities, which restratify the upper ocean, and turbulent mixing, which acts to destroy this stratification. Recent studies have found that frontal instabilities can restratify the upper ocean, even in the presence of strong surface cooling and destabilizing winds. During winter at high latitudes, primary production by phytoplankton is generally limited by low ambient light levels and deep turbulent mixing. When the turbulent mixing, inhibited by frontal restratification, becomes smaller than a ‘critical turbulence’ threshold, a phytoplankton bloom can develop. The finding that fronts can trigger phytoplankton blooms by reducing mixing, provides an explanation for satellite observations of high chlorophyll concentrations at high latitude fronts.en_US
dc.description.sponsorshipUnited States. Office of Naval Research (Award N00014-08-1-1060)en_US
dc.language.isoen_US
dc.publisherAmerican Geophysical Union (AGU)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1029/2011gl049312en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceOther University Web Domainen_US
dc.titleOcean fronts trigger high latitude phytoplankton bloomsen_US
dc.typeArticleen_US
dc.identifier.citationTaylor, J. R., and R. Ferrari. “Ocean Fronts Trigger High Latitude Phytoplankton Blooms.” Geophysical Research Letters 38.23 (2011). ©2011. American Geophysical Union.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorFerrari, Raffaele
dc.relation.journalGeophysical Research Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsTaylor, J. R.; Ferrari, R.en
dc.identifier.orcidhttps://orcid.org/0000-0002-3736-1956
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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