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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Formation of black carbon rich `sombric' horizons in the subsoil - A case study from subtropical Brazil

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Autor(es):
Chiapini, Mariane [1] ; Schellekens, Judith [1] ; Calegari, Marcia Regina [2] ; de Almeida, Jaime Antonio [3] ; Buurman, Peter [4] ; de Camargo, Plinio Barbosa [5] ; Vidal-Torrado, Pablo [1]
Número total de Autores: 7
Afiliação do(s) autor(es):
[1] Univ Sao Paulo, Escola Super Agr Luis de Queiroz ESALQ, Dept Ciencia Solo, Av Padua Dias 11, Piracicaba, SP - Brazil
[2] Univ Estadual Oeste Parana UNIOESTE, Dept Geog, Campus Marechal Candido Rondon, Rua Pernambuco 177, BR-85970000 Marechal Candido Rodondo, Parana - Brazil
[3] UDESC, Dept Solos, Ctr Ciencias Agrovet, Av Luis de Camoes 2090, BR-88520000 Loges, SC - Brazil
[4] Wageningen Univ, Earth Syst Sci Grp, POB 47, NL-6700 AA Wageningen - Netherlands
[5] Univ Sao Paulo, Ctr Isotop Energy Agr, Piracicaba - Brazil
Número total de Afiliações: 5
Tipo de documento: Artigo Científico
Fonte: Geoderma; v. 314, p. 232-244, MAR 15 2018.
Citações Web of Science: 3
Resumo

The formation of sombric horizons (dark horizons in the subsoil) is still not understood. In order to improve our understanding of the formation of sombric horizons we studied these soils in southern Brazil from various perspectives. The lateral configuration and grain size distribution excluded the possibility that the sombric horizon is a paleosol covered by an eolian deposit or colluvium. Micromorphology showed intense biological activity, indicating strong bioturbation. The absence of clay and OM coatings indicates that the sombric horizon in the study area was not formed by illuviation. Considering changes with depth, phytoliths and delta C-13 isotopes clearly showed that the OM from the sombric horizon had a larger contribution from grasses, while a larger contribution from black carbon (BC) was evidenced by the molecular composition. A larger contribution from grasses and BC both correspond to drier climatic conditions. However, similar depth trends for delta C-13 and PAHs were found in the reference profile (without sombric horizon), in agreement with climatic change but not explaining the different morphology. The molecular composition and C/N ratio showed that the profiles differed in degree of decomposition, with the OM in the soils that contained a sombric horizon being more decomposed than that in the reference profile. The sombric horizon is thus a remnant of an earlier phase of soil formation under a drier climate, which is made visible by differences in decomposition of OM related to subsequent more humid conditions. Stronger decomposition in the profiles with a sombric horizon may be related to better drainage, explaining their occurrence in the highest positions within the landscape and suggesting a topographic control. (AU)

Processo FAPESP: 14/23969-0 - Dinâmica da matéria orgânica do solo e sua relação com o ambiente e com processos pedogenéticos: química molecular (pirólise-CG/EM) de solos tropicais
Beneficiário:Pablo Vidal Torrado
Linha de fomento: Auxílio à Pesquisa - Regular
Processo FAPESP: 13/03953-9 - Dinâmica da matéria orgânica em organossolos de turfeiras tropicais (Diamantina-MG, Brasil) - desenvolvimento de proxies moleculares para a reconstrução de mudanças paleoambientais
Beneficiário:Judith Schellekens
Linha de fomento: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 15/03577-2 - Pedogênese e caracterização molecular de horizontes sômbricos em solos da região de tijucas do sul-pr.
Beneficiário:Mariane Chiapini
Linha de fomento: Bolsas no Brasil - Mestrado