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dc.contributor.authorOLIVEIRA, J. F. dept_BR
dc.contributor.authorBROSSARD, M.pt_BR
dc.contributor.authorCORAZZA, E. J.pt_BR
dc.contributor.authorMARCHAO, R. L.pt_BR
dc.contributor.authorGUIMARÃES, M. de F.pt_BR
dc.date.accessioned2016-12-23T11:11:11Zpt_BR
dc.date.available2016-12-23T11:11:11Zpt_BR
dc.date.created2016-12-23pt_BR
dc.date.issued2016pt_BR
dc.identifier.citationJournal of Near Infrared Spectroscopy, v. 24, n. 3, p. 243-254, March 2016.pt_BR
dc.identifier.urihttp://www.alice.cnptia.embrapa.br/alice/handle/doc/1059216pt_BR
dc.descriptionABSTRACT: In soil science, structural features of soils are an important attribute; soils can be characterised by proportional size distribution of aggregates and the pore space between and within those aggregates. The objective of this study was to evaluate the relationship between the visible and near infrared (Vis?NIR) spectra and microaggregates from a collection of Ferralsols. Our dataset consists of 56 spectra from seven soil profiles of kaolinitic and oxidic-gibbsitic Ferralsols. Soils were characterised according to their morphological features: those with a typical porous massive structure and those with a cohesive massive structure. Size distribution of five classes of microaggregate was determined (1000?2000 µm, 500?1000 µm, 250?500 µm, 105?250 µm and < 105?µm). From the soil spectra, we determined the CIE (Commission Internationale de l'Éclairage) red index (RICIE) and the absorption intensities of kaolinite (IKa) and gibbsite (IGb). The predominant fraction of microaggregates exhibited sizes between 250 and 1000µm (&#934;250?1000). The proportional increase of this microaggregate class in the soils increased the scattering and variability of reflected light, particularly when soil samples showed more than 0.50 g g?1 of &#934;250?1000. The microaggregate size explained over 55% of reflectance intensity variability of wavelengths in the vis?NIR regions, principally on reflectance intensity and concavity of the spectra at 436 nm, 546 nm and 2236 nm, which decreases with increased proportion of &#934;250?1000. Thus, different structural features of Ferralsols can be directly evaluated through Vis?NIR spectroscopy, even in samples sieved through 2.00 mm. These results highlight the potential use of Vis?NIR spectroscopy in studies of soil classification, soil physical behaviour and soil physical fertility and environmental studies, principally by a new method of analysing bulk density and structure of soil directly from the soil spectra, without the need for predictive models. As well as spectra, RICIE,IKa and IGb can be used to characterise the different structural features of Ferralsols.pt_BR
dc.language.isoengeng
dc.rightsopenAccesseng
dc.subjectEspectroscopia de refletância difusapt_BR
dc.subjectMicropedpt_BR
dc.subjectSolo mineralpt_BR
dc.subjectDiffuse reflectance spectroscopypt_BR
dc.subjectLatosolpt_BR
dc.subjectSoil mineralpt_BR
dc.titleVisible and near infrared spectra of Ferralsols according to their structural features.pt_BR
dc.typeArtigo de periódicopt_BR
dc.date.updated2017-01-09T11:11:11Zpt_BR
dc.subject.thesagroEstrutura do Solopt_BR
dc.subject.thesagroLatossolopt_BR
dc.subject.nalthesaurusSoil structurept_BR
riaa.ainfo.id1059216pt_BR
riaa.ainfo.lastupdate2017-01-09pt_BR
dc.identifier.doihttps://doi.org/10.1255/jnirs.1202pt_BR
dc.contributor.institutionJosé Francirlei de Oliveira, Universidade Estadual de Londrina; Michel Brossard, IRD (Institut de recherche pour le développement); EDEMAR JOAQUIM CORAZZA, SCT; ROBELIO LEANDRO MARCHAO, CPAC; Maria de Fátima Guimarães, Universidade Estadual de Londrina.pt_BR
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