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Storm deposits in a carbonate ramp: implications in the origin of the carbonate mud accumulated in distal ramp (Kimmendgian, Iberian basin)

dc.contributor.authorBádenas, Beatriz
dc.date.accessioned2015-04-06T09:38:47Z
dc.date.available2015-04-06T09:38:47Z
dc.date.issued1997
dc.identifier.urihttp://hdl.handle.net/10272/10230
dc.description.abstractFacies distribution and sedimentary procceses in a storm dominated carbonate ramp (Kimmeridgian, northern Iberian basin) is studied in detail. Shallow ramp areas are dominated by coral reef facies. They grade basinsward into muddy facies, that have different storm deposits (storm lobes and bars, proximal tempestites and distal tempestites). The analysis of the relationship between these deposits along to the study of the composition of the carbonate grains, al/ow us to conclude that most of the coarse grain were produced in the reefal dominated areas. Downslope sediment transport was due to storm induced density currents. A significant part of the mud accumulated Offshore may be also resedimented in origin. Downslope transport in the studied ramp was favoured by its windward orientationen_US
dc.language.isospaen_US
dc.publisherSociedad Geológica de Españaen_US
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subject.otherStorm depositsen_US
dc.subject.otherCarbonate muden_US
dc.subject.otherKimmeridgian rampen_US
dc.subject.otherIberian basinen_US
dc.titleDepósitos de tormenta en una rampa carbonatada: implicaciones sobre el origen del fango carbonatado acumulado en su zona distal (Kimmeridgiense, Cuenca Ibérica)en_US
dc.titleStorm deposits in a carbonate ramp: implications in the origin of the carbonate mud accumulated in distal ramp (Kimmendgian, Iberian basin)eng
dc.typeinfo:eu-repo/semantics/articleen_US
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessen_US


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