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Accumulation of nutrients during the formation of star fruit cultivars under different irrigation regimes

dc.contributor.authorRozane, Danilo Eduardo [UNESP]
dc.contributor.authorPrado, Renato de Mello [UNESP]
dc.contributor.authorDe Paula, Betania Vahl
dc.contributor.authorDos Santos, Eduardo Maciel Haitzmann [UNESP]
dc.contributor.authorNatale, William
dc.contributor.authorDe Amorim, Daniel Angelucci
dc.contributor.authorHernandes, Amanda
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionUniversidade Federal de Sergipe (UFS)
dc.contributor.institutionFederal University of Ceara (UFC)
dc.contributor.institutionExperimental Farm of Caldas
dc.contributor.institutionBatatais Agriculture House
dc.date.accessioned2023-07-29T12:41:24Z
dc.date.available2023-07-29T12:41:24Z
dc.date.issued2022-01-01
dc.description.abstractNutrient accumulation during the formation of star fruit (Averrhoa carambola) trees can be affected by the water regime and by the cultivar, but the details are not yet known for this species. The aim of this study was to evaluate the nutrient uptake of two star fruit cultivars in the formation phase under two irrigation regimes. The experiment was developed with a completely randomized design, with subdivided plots, with two irrigation levels (with and without irrigation) as plots, and two star fruit cultivars as subplots (‘B-10’ and ‘Golden Star’) and seven collection times from 0 to 720 days after transplanting (DAT) into the field as sub-subplots with six replicates. Nutrient uptake was evaluated in stem and leaves, and it was possible to observe that nutrient uptake and the average accumulation rate followed the dry matter mass accumulation of star fruit trees in formation. Nutrient uptake by shoots at 720 DAT differed for the Golden Star cultivar in the rainfed regime and for the B-10 cultivar in both irrigation regimes. There was no difference and followed the sequence Ca > K > N > Mg > S > P > Mn > Fe > Zn > B > Cu, and for Golden Star cultivar in the irrigated regime, the accumulation sequence was Ca> K> N> Mg> Mn> P> S> Fe> Zn > B> Cu. The highest accumulation occurred in the irrigated regime regardless of cultivar. Golden Star cultivar accumulated, on average, larger amounts of N, P, K, Mg, S, Fe and Mn.en
dc.description.affiliationSão Paulo State University (UNESP) Department of Agronomy
dc.description.affiliationFederal University of Santa Maria (UFSM) Department of Soil Science
dc.description.affiliationFederal University of Ceara (UFC) Department of Fitotecnia
dc.description.affiliationAgricultural Research Company of Minas Gerais (EPAMIG) Experimental Farm of Caldas
dc.description.affiliationCoordination of Integral Technical Assistance (CATI) Batatais Agriculture House
dc.description.affiliationUnespSão Paulo State University (UNESP) Department of Agronomy
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipIdFAPESP: 2006 / 55569-4
dc.description.sponsorshipIdFAPESP: 2006 / 55570-2
dc.identifierhttp://dx.doi.org/10.17584/rcch.2022v16i2.13832
dc.identifier.citationRevista Colombiana de Ciencias Horticolas, v. 16, n. 2, 2022.
dc.identifier.doi10.17584/rcch.2022v16i2.13832
dc.identifier.issn2422-3719
dc.identifier.scopus2-s2.0-85143761386
dc.identifier.urihttp://hdl.handle.net/11449/246456
dc.language.isoeng
dc.relation.ispartofRevista Colombiana de Ciencias Horticolas
dc.sourceScopus
dc.subjectAverrhoa carambola
dc.subjectnutrient uptake
dc.subjectnutritional requirement
dc.subjectwater deficit
dc.titleAccumulation of nutrients during the formation of star fruit cultivars under different irrigation regimesen
dc.titleAcumulación de nutrientes durante la formación de cultivares de carambola en formación bajo regímenes de irrigaciónes
dc.typeArtigo
dspace.entity.typePublication
unesp.author.orcid0000-0003-0518-3689[1]
unesp.author.orcid0000-0003-1998-6343[2]
unesp.author.orcid0000-0002-2348-1527[3]
unesp.author.orcid0000-0003-1585-3500[4]
unesp.author.orcid0000-0001-9572-4463[5]
unesp.author.orcid0000-0003-4921-5080[6]
unesp.author.orcid0000-0002-8545-7581[7]

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