Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/2436
DC Field | Value | Language |
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dc.contributor.authorall | Jovane, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Florindo, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Sprovieri, M.; Istituto Ambiente Marino Costiero (CNR), Calata Porta di Massa (Interno Porto di Napoli), I-80133 Naples, Italy | en |
dc.contributor.authorall | Palike, H.; National Oceanography Centre, Southampton, University of Southampton, European Way, Southampton SO14 3ZH, UK | en |
dc.date.accessioned | 2007-09-04T11:55:58Z | en |
dc.date.available | 2007-09-04T11:55:58Z | en |
dc.date.issued | 2006 | en |
dc.identifier.uri | http://hdl.handle.net/2122/2436 | en |
dc.description.abstract | We present an astronomically tuned polarity timescale for the late Eocene/early Oligocene based on a cyclic limestone/marls sedimentary succession exposed at Massignano, Italy (GSSP for the Eocene- Oligocene boundary). Here we applied spectral analysis techniques to the high-resolution magnetic susceptibility record. The results provide clear evidence of a regular and cyclic signal that allows us to discard a stochastic mechanism as controlling these fluctuations. Conversely, these outcomes reveal the presence of stable and notable periodicities that are in tune with those associated with orbital forcing. Through a cyclostratigraphic analysis of the rhythmic sedimentary alternations and combination with the results of time series analysis of the proxy record, we refine the late Eocene portion of the GPTS. Through astronomical tuning of the rhythmic sedimentary alternations to recent astronomically calculated variations of Earth’s orbit we recalibrated the polarity boundaries ages and the main stratigraphic events recognized throughout the sedimentary record. Among these, an age of 33.714 Ma is proposed for the E/O boundary. | en |
dc.language.iso | English | en |
dc.publisher.name | Agu | en |
dc.relation.ispartof | Geochem. Geophys. Geosyst. | en |
dc.relation.ispartofseries | 7/7 (2006) | en |
dc.subject | environmental magnetism; | en |
dc.subject | Eocene/Oligocene | en |
dc.title | Astronomic calibration of the late Eocene/early Oligocene Massignano section (central Italy) | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | Q07012 | en |
dc.subject.INGV | 04. Solid Earth::04.05. Geomagnetism::04.05.07. Rock magnetism | en |
dc.identifier.doi | 10.1029/2005GC001195 | en |
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Laskar (1999), Astronomical calibration of Oligocene-Miocene time, Philos. Trans. R. Soc. London, Ser. A, 357, 1909–1927. Spezzaferri, S., D. Basso, and R. Coccioni (2002), Late Eocene planktonic foraminiferal response to an extraterrestrial impact at Massignano GSSP (northeastern Apennines, Italy), J. Foraminiferal Res., 32, 188–199. Torrence, C., and G. P. Compo (1998), A practical guide to wavelet analysis, Bull. Am. Meteorol. Soc., 79, 61–78. Turco, E., F. J. Hilgen, L. J. Lourens, N. J. Shackleton, andW. J. Zachariasse (2001), Punctuated evolution of global climate cooling during the late middle to early late Miocene; highresolution planktonic foraminiferal and oxygen isotope records from the Mediterranean, Paleoceanography, 16(4), 405–423. Vonhof, H. B., J. Smit, H. Brinkhuis, A. Montanari, and A. J. Nederbragt (2000), Global cooling accelerated by early late Eocene impacts?, Geology, 28, 687–690. Wade, B. S., and H. Pa¨like (2004), Oligocene climate dynamics, Paleoceanography, 19, PA4019, doi:10.1029/ 2004PA001042. Weedon, G. P. (2003), Time-Series Analysis and Cyclostratigraphy, 259 pp., Cambridge Univ. Press, New York. | en |
dc.description.fulltext | reserved | en |
dc.contributor.author | Jovane, L. | en |
dc.contributor.author | Florindo, F. | en |
dc.contributor.author | Sprovieri, M. | en |
dc.contributor.author | Palike, H. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Ambiente Marino Costiero (CNR), Calata Porta di Massa (Interno Porto di Napoli), I-80133 Naples, Italy | en |
dc.contributor.department | National Oceanography Centre, Southampton, University of Southampton, European Way, Southampton SO14 3ZH, UK | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | restricted | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione AC, Roma, Italia | - |
crisitem.author.dept | CNR-IAMC, Napoli | - |
crisitem.author.orcid | 0000-0002-6058-9748 | - |
crisitem.author.orcid | 0000-0003-3386-0923 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 04. Solid Earth | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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