Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/6424
DC Field | Value | Language |
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dc.contributor.authorall | Hüsing, S. K.; Paleomagnetic Laboratory “Fort Hoofddijk”, Department of Earth Sciences, Budapestlaan 17, 3584 CD Utrecht, The Netherlands | en |
dc.contributor.authorall | Cascella, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Hilgen, F. J.; Stratigraphy/Paleontology, Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands | en |
dc.contributor.authorall | Krijgsman, W.; Paleomagnetic Laboratory “Fort Hoofddijk”, Department of Earth Sciences, Budapestlaan 17, 3584 CD Utrecht, The Netherlands | en |
dc.contributor.authorall | Kuiper, K. F.; Department of Isotope Geochemistry, Vrije Universiteit Amsterdam, De Boelelaan 1085, 1081 HV Amsterdam, The Netherlands | en |
dc.contributor.authorall | Turco, E.; Dip. di Scienze della Terra, Universita di Parma, Parco Area della Scienze 157/A, 43100 Parma, Italy | en |
dc.contributor.authorall | Wilson, D.; Department of Geological Sciences, University of California, Santa Barbara, CA 93106, USA | en |
dc.date.accessioned | 2010-12-20T14:39:25Z | en |
dc.date.available | 2010-12-20T14:39:25Z | en |
dc.date.issued | 2010-02 | en |
dc.identifier.uri | http://hdl.handle.net/2122/6424 | en |
dc.description.abstract | An integrated high-resolution magnetobiocyclostratigraphy including radioisotopic dating and astronomical tuning is presented for the interval between 15.29 and 14.17 Ma in the marine La Vedova section in northern Italy. The natural remanent magnetization is carried by the iron sulphide greigite and the resultant magnetostratigraphy can be correlated straightforwardly to the interval ranging from C5Bn.2n to C5ADn in the Astronomically Tuned Neogene Time Scale (ATNTS2004). Spectral analysis on high-resolution magnetic susceptibility and geochemical proxy records in the depth domain and, using our magnetobiostratigraphic age model, in the time domain demonstrate that the various scales of cyclicity in the section are related to astronomical climate forcing. Starting from our initial age model, larger-scale cycles were first tuned to eccentricity. This first-order tuning was followed by tuning the basic cycle to precession and boreal summer insolation using inferred phase relations between maxima in Ca/Al, redox-sensitive elements and Ba, and minima in magnetic susceptibility, and maxima in precession and minima in obliquity and boreal summer insolation. Our astronomical ages for reversal boundaries are supported by analysis of sea floor spreading rates and should replace the existing ages in the ATNTS2004 lacking direct astronomical control. Two major steps in the geochemical proxy records, astronomically dated at 15.074 and 14.489 Ma, coincide with abrupt changes in sedimentation rate, and are the result of the combined effect of the ∼400-kyr eccentricity cycle superimposed upon a longer-term climatic or tectonic induced trend. | en |
dc.language.iso | English | en |
dc.publisher.name | Elsevier | en |
dc.relation.ispartof | Earth and Planetary Science Letters | en |
dc.relation.ispartofseries | 3-4 / 290 (2010) | en |
dc.subject | Middle Miocene | en |
dc.subject | Langhian | en |
dc.subject | Mediterranean | en |
dc.subject | astronomical tuning | en |
dc.subject | palaeomagnetism | en |
dc.subject | biostratigraphy | en |
dc.subject | environmental changes | en |
dc.subject | orbital forcing | en |
dc.title | Astrochronology of the Mediterranean Langhian between 15.29 and 14.17 Ma | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | 254–269 | en |
dc.subject.INGV | 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy | en |
dc.subject.INGV | 04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetism | en |
dc.identifier.doi | 10.1016/j.epsl.2009.12.002 | en |
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This first-order tuning was followed by tuning the basic cycle to precession and boreal summer insolation using inferred phase relations between maxima in Ca/Al, redox-sensitive elements and Ba, and minima in magnetic susceptibility, and maxima in precession and minima in obliquity and boreal summer insolation. Our astronomical ages for reversal boundaries are supported by analysis of sea floor spreading rates and should replace the existing ages in the ATNTS2004 lacking direct astronomical control. Two major steps in the geochemical proxy records, astronomically dated at 15.074 and 14.489 Ma, coincide with abrupt changes in sedimentation rate, and are the result of the combined effect of the ∼400-kyr eccentricity cycle superimposed upon a longer-term climatic or tectonic induced trend.and astronomical tuning of the Blue Clay Formation on Malta. Paleoceanography 20, 1–17. Backman, J., Shackleton, N.J., 1983. 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dc.description.obiettivoSpecifico | 2.2. Laboratorio di paleomagnetismo | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | restricted | en |
dc.contributor.author | Hüsing, S. K. | en |
dc.contributor.author | Cascella, A. | en |
dc.contributor.author | Hilgen, F. J. | en |
dc.contributor.author | Krijgsman, W. | en |
dc.contributor.author | Kuiper, K. F. | en |
dc.contributor.author | Turco, E. | en |
dc.contributor.author | Wilson, D. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Stratigraphy/Paleontology, Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands | en |
dc.contributor.department | Paleomagnetic Laboratory “Fort Hoofddijk”, Department of Earth Sciences, Budapestlaan 17, 3584 CD Utrecht, The Netherlands | en |
dc.contributor.department | Department of Isotope Geochemistry, Vrije Universiteit Amsterdam, De Boelelaan 1085, 1081 HV Amsterdam, The Netherlands | en |
dc.contributor.department | Dip. di Scienze della Terra, Universita di Parma, Parco Area della Scienze 157/A, 43100 Parma, Italy | en |
dc.contributor.department | Department of Geological Sciences, University of California, Santa Barbara, CA 93106, USA | 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 Pisa, Pisa, Italia | - |
crisitem.author.dept | Stratigraphy/Paleontology, Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands | - |
crisitem.author.dept | Paleomagnetic Laboratory “Fort Hoofddijk,” Department of Earth Sciences, Utrecht University, Utrecht, Netherlands | - |
crisitem.author.dept | Department of Isotope Geochemistry, Vrije Universiteit Amsterdam, De Boelelaan 1085, 1081 HV Amsterdam, The Netherlands | - |
crisitem.author.dept | Dipartimento di Fisica e Scienze della Terra, Università di Parma | - |
crisitem.author.dept | Paleomagnetic Laboratory ‚Fort Hoofddijk | - |
crisitem.author.dept | Department of Earth Sciences, Utrecht University | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Institute for Crustal Studies, University of California in Santa Barbara, USA | - |
crisitem.author.orcid | 0000-0002-8255-3244 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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.classification.parent | 04. Solid Earth | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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