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AURELL, M., BÁDENAS, B. (2004) Facies and depositional sequence evolution controlled by high-frequency sea-level changes in a shallow-water carbonate ramp (late Kimmeridgian, NE Spain) Geological Magazine, 141 (6) 717-733 doi:10.1017/s0016756804009963

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Reference TypeJournal (article/letter/editorial)
TitleFacies and depositional sequence evolution controlled by high-frequency sea-level changes in a shallow-water carbonate ramp (late Kimmeridgian, NE Spain)
JournalGeological Magazine
AuthorsAURELL, M.Author
BÁDENAS, B.Author
Year2004 (November)Volume141
Issue6
PublisherCambridge University Press (CUP)
DOIdoi:10.1017/s0016756804009963Search in ResearchGate
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Mindat Ref. ID259528Long-form Identifiermindat:1:5:259528:7
GUID0
Full ReferenceAURELL, M., BÁDENAS, B. (2004) Facies and depositional sequence evolution controlled by high-frequency sea-level changes in a shallow-water carbonate ramp (late Kimmeridgian, NE Spain) Geological Magazine, 141 (6) 717-733 doi:10.1017/s0016756804009963
Plain TextAURELL, M., BÁDENAS, B. (2004) Facies and depositional sequence evolution controlled by high-frequency sea-level changes in a shallow-water carbonate ramp (late Kimmeridgian, NE Spain) Geological Magazine, 141 (6) 717-733 doi:10.1017/s0016756804009963
In(2004, November) Geological Magazine Vol. 141 (6) Cambridge University Press (CUP)
Abstract/NotesThe outcrops of the Sierra de Albarracín (NE Spain) allow a precise reconstruction of the shallow sedimentary domains of a late Kimmeridgian carbonate ramp, developed in western marginal areas of the Iberian Basin. The sedimentary record shows a hierarchical sequence stratigraphic organization, which implies sea-level changes of different frequencies. The studied succession is arranged in a long-term transgressive–regressive sequence, which is likely to reflect local variation in the subsidence rates. This sequence includes four higher-order sequences A to D, which have variable thickness (from 3 to 21 m). The similar sedimentary evolution observed in distant localities suggests the existence of high-frequency sea-level fluctuations controlling the sequence development. The average amplitude of these cycles would range from 5 to 10 m. The precise estimation of their duration (some few hundreds of kyr) and their possible assignment to any of the long-term orbital cycles (the 100 or the 400 kyr eccentricity cycles) is uncertain. Sequences A and B, formed during the long-term transgressive interval, are relatively thin (from 3 to 9 m) give-up sequences that were never subaerially exposed. These sequences are locally formed by five shallowing-upward elementary sequences. Sequences C and D are catch-down sequences with evidence of emersion of subtidal facies. Sequence C, formed during the stage of maximum gain of long-term accommodation, is the thickest sequence (from 13 to 21 m) and includes coral–microbial reefs (pinnacles up to 16 m in height). The increased production rates were able to fill part of the accommodation created during the early stage of high-frequency sea-level rise and the shallow platform was eventually exposed to subaereal erosion and meteoric cementation.


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