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dc.contributor.authorMorganti, T.es_ES
dc.contributor.authorRibes, Martaes_ES
dc.contributor.authorMoskovich, Razes_ES
dc.contributor.authorWeisz, Jeremyes_ES
dc.contributor.authorYahel, G.es_ES
dc.contributor.authorComa, Rafaeles_ES
dc.date.accessioned2021-01-25T13:26:22Z-
dc.date.available2021-01-25T13:26:22Z-
dc.date.issued2021-03-
dc.identifier.citationFrontiers in Marine Science 8: 583188 (2021)es_ES
dc.identifier.otherCEX2019-000928-S-
dc.identifier.urihttp://hdl.handle.net/10261/227486-
dc.descriptionCorrigendum: In situ Pumping Rate of 20 Marine Demosponges Is a Function of Osculum Area by Morganti, T. M., Ribes, M., Moskovich, R., Weisz, J. B., Yahel, G., and Coma, R. (2021). Frontiers in Marine Science 8: 712856. doi: 10.3389/fmars.2021.712856-
dc.description.abstractSponges play a key role in the transfer of energy and nutrients into many benthic ecosystems, and the volume of water they process is an important regulator of these fluxes. Theoretical scaling relationships between sponge volume, osculum cross-sectional area, and pumping rates were recently proposed and confirmed for small sponge specimens in the lab. To examine how these relationships apply to field populations we measured, in situ, the pumping rate (PR) of 20 species representative of different morphologies and host types (high-and low-microbial abundance, HMA and LMA) from temperate and tropical regions. The total oscula area (∑OSA) increased allometrically with sponge volume (V) exhibiting similar exponents (∑OSA=aVb, b ranging 0.6-0.7) for all species, except for tropical HMAs (b= 0.99). Osculum flow rate (OFR) also increased allometrically with OSA and oscula of the same size pumped at the same rate irrespective of sponge volume. As a result, and in contrast to former reports, the PR of most of the sponges increased allometrically (PR=a∑OSAb) with scaling exponent b≈0.75, whereas PR of tropical HMAs increased isometrically. Osculum jet speed declined with the increase in the OSA for most species. The number of oscula and their OSA were the best predictors of the PR in sponges, explaining 75-94% of the in situ variation in PR throughout the natural range of sponge size. The pumping rate of a sponge population can be estimated by measuring the osculum density and cross-sectional area distribution once the relationships between the OSA and OFR are established for each species.es_ES
dc.description.sponsorshipFinancial support was provided by the Spanish Government through the Grant (RTI2018-094187-B-100) and the ‘Severo Ochoa Centre of Excellence' accreditation (CEX2019-000928-S), and by the Pure Oceans Foundation Grant 2019-Spoplastics to RC and MR; and by a FPU fellowship from Ministerio de Educación, Cultura y Deporte (MECD) and Max Planck Society to TM. Additional financial support was provided by ISF grant 1280/13 and BSF grants 2012089 and 2017622 to GY. This is a contribution from the Marine Biogeochemistry and Global Change research group from the Generalitat de Catalunya (2017SGR1011).-
dc.language.isoenges_ES
dc.publisherFrontiers Mediaes_ES
dc.relationMICIU/ICTI2017-2020/RTI2018-094187-B-100-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccesses_ES
dc.subjectSponge (Porifera)es_ES
dc.subjectPumping ratees_ES
dc.subjectSizees_ES
dc.subjectAllometric scalinges_ES
dc.subjectOsculumes_ES
dc.subjectHMA-LMA spongeses_ES
dc.titleIn situ Pumping Rate of 20 Marine Demosponges is a Function of Osculum Areaes_ES
dc.typeartículoes_ES
dc.identifier.doihttp://dx.doi.org/10.3389/fmars.2021.583188-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttps://doi.org/10.3389/fmars.2021.583188es_ES
dc.identifier.e-issn2296-7745-
dc.rights.licensehttp://creativecommons.org/licenses/by/4.0/-
dc.contributor.funderGeneralitat de Catalunya-
dc.contributor.funderAgencia Estatal de Investigación (España)-
dc.contributor.funderMinisterio de Ciencia, Innovación y Universidades (España)-
dc.contributor.funderMinisterio de Educación, Cultura y Deporte (España)-
dc.contributor.funderMax Planck Society-
dc.relation.csices_ES
oprm.item.hasRevisionno ko 0 false*
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002809es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004189es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003176es_ES
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