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    Publication Date: 2019-04-01
    Print ISSN: 0012-8252
    Electronic ISSN: 1872-6828
    Topics: Geography , Geosciences
    Published by Elsevier
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    Publication Date: 2017-04-04
    Description: The astronomical time scale for the Paleocene is hampered by some uncertainties including discrepant number of 405-kyr eccentricity related cycles and correlation schemes among key records being proposed by different authors (Westerhold et al., 2008; Kuiper et al., 2008; Hilgen et al., 2010). Here we present a new Danian correlation framework resolved at the ~100-kyr short-eccentricity level between the land-based Zumaia and Sopelana hemipelagic sections from the Basque Basin and deep-sea records drilled during ODP Legs 198 (Shatsky Rise, North Pacific) and 208 (Walvis Ridge, South Atlantic) that reconciles both the magnetostratigraphy and the short and longeccentricity cycle patterns among the records and, hence, improves synchroneity of events. The correlation has been aided by composite images from ODP cores and a new wholerock 13C isotope record at Zumaia while its original magnetostratigraphy (Dinarès-Turell et al., 2003; 2010) is reinforced by new data from Sopelana. Notably, we challenge the correlation of the Pacific Sites 1209–1210 that were offset by as much as one 405-kyr cycle in previous interpretations (i.e., the Fasciculithus spp. LO, which approximates the Danian–Selandian (D–S) boundary, and the “Top chron C27n” climatic event were at odds between oceans in the interpretation of Hilgen et al. (2010). It is found that the Danian consists of 11 (and not 10) consecutive 405-kyr eccentricity cycles. The new consistent stratigraphic framework enables accurate estimates to be made of ages for magnetostratigraphic boundaries, bioevents, and sedimentation rates. Low sedimentation rates appear common in all records in the mid- Danian interval along the upper part of chron C28n, including conspicuous condensed intervals in some of the oceanic records that in the past have hampered the proper identification of cycles. The new chronological framework, spanning a duration of about 4.5 My, allows assessing the role of orbital forcing on the paleoclimatic variability as registered by the related isotope records. It appears clear that there exists a periodic beat at the 100-ky and 405-ky eccentricity cycles impressed in the record. The phase relationship between the benthic isotope record and eccentricity is similar to patterns documented for the Oligocene and Miocene, as indicated by others, confirming the role of orbital forcing as the pace maker for paleoclimatic variability on Milankovitch time scales. The preferred tuning to the La2011 orbital solution provides astronomically calibrated ages of 66.022±0.040 Ma and 61.607±0.040 Ma for the (D–S) and Cretaceous–Paleogene (K–Pg) boundaries respectively. Finally, we envisage that the Zumaia section, which already hosts the Selandian GSSP, could serve as the global Danian stratotype.
    Description: Published
    Description: 64-65
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: N/A or not JCR
    Description: restricted
    Keywords: cyclostratigraphy ; magnetostratigraphy ; ODP ; orbital tuning ; 03. Hydrosphere::03.01. General::03.01.06. Paleoceanography and paleoclimatology ; 04. Solid Earth::04.04. Geology::04.04.08. Sediments: dating, processes, transport ; 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 6
    Publication Date: 2017-04-04
    Description: Paleomagnetic and rock magnetic analyses were conducted on discrete samples from sediments drilled during Integrated Ocean Drilling Program Expedition 317 in the Canterbury Basin offshore New Zealand to assess the nature of magnetic remanence and to evaluate the directional data for a magnetic reversal stratigraphy. The sediments consist of relatively coarse grained lithologies from shelf to slope settings. The presence of several hiatuses, together with very low core recovery in some intervals as well as drillingrelated magnetic overprints, prevented establishment of a good shipboard magnetostratigraphy. In an effort to overcome some of the magnetic shortcomings and to substantiate shipboard measurements (overprints and partial demagnetization to 20 mT), natural remanent magnetization and subsequent full stepwise alternating field or thermal demagnetization measurements were taken on 765 individual discrete samples from Holes U1351B (131 samples), U1352B/U1352C (485 samples), U1353B (54 samples), and U1354B/U1354C (95 samples). Some rock magnetic measurements, including thermomagnetic curves, were taken on a few representative samples to acquire information on the magnetic carriers. The remanence intensity of the sediments is relatively low (usually 10–3 to 10–5 A/m) and often displays unstable behavior upon demagnetization. Demagnetization data have been separated into four different classes based on their quality. Classes 1 and 2 are of sufficient quality to be used for magnetostratigraphic purposes and represent ~40% of the studied samples (although some of them could still represent a steep magnetic drilling overprint). Considering the calculated characteristic remanent magnetization inclination, a number of polarity zones can be defined. However, the fragmentary nature of the data set, mostly related to core recovery in addition to detected and undetected sedimentary hiatuses, makes determination of the precise position of the reversal boundaries and their correlation to the geomagnetic polarity timescale a difficult task. Nevertheless, when combined shipboard and postcruise discrete measurements are placed within biostratigraphic constraints, some magnetostratigraphic insights can potentially refine the available age model. These insights include the identification of the Matuyama/Brunhes boundary (C1r1r/C1n, 0.778 Ma) at all four sites, the Gauss/Matuyama boundary (C2An.1n/C2r.2r, 2.581 Ma) in Hole U1351B, and also the position of the Olduvai Subchron (C2n, 1.778–1.945 Ma) in Hole U1351B, which relates to the position of the classical Pliocene/Pleistocene boundary.
    Description: Published
    Description: 1-31
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: N/A or not JCR
    Description: restricted
    Keywords: Deep Sea ; magnetostratigraphy ; rock magnetism ; Plio-Pleistecene ; Miocene ; 03. Hydrosphere::03.01. General::03.01.06. Paleoceanography and paleoclimatology ; 04. Solid Earth::04.04. Geology::04.04.08. Sediments: dating, processes, transport ; 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 7
    Publication Date: 2017-04-04
    Description: We present a new Danian correlation framework between the land-based Zumaia and Sopelana sections from the Basque Basin and marine-based sections drilled during ODP Legs 198 (Shatsky Rise, North Pacific) and 208 (Walvis Ridge, South Atlantic) that reconciles magnetostratigraphy and the short and long eccentricity cycle patterns among the records. A new whole-rock d13C isotope record at Zumaia is compared to that of Site 1262. This allows the question of whether the Danian consists of 10 or 11 consecutive 405-kyr eccentricity cycles to be tested. The new consistent stratigraphic framework enables accurate estimates to be made of ages for magnetostratigraphic boundaries, bioevents, and sedimentation rates. Low sedimentation rates appear common in all records in the mid-Danian interval along the upper part of chron C28n, including conspicuous condensed intervals in some of the oceanic records that in the past have hampered the proper identification of cycles. Notably, we challenge the correlation to the Pacific Sites 1209–1210 that were offset by as much as one 405-kyr cycle in previous interpretations (i.e., the Fasciculithus spp. LO, which approximates the Danian–Selandian boundary, and the TC27n event were at odds between oceans in the interpretation of Hilgen et al. 2010). Finally, we envisage that the Zumaia section, which already hosts the Selandian GSSP, could serve as the global Danian stratotype.
    Description: Published
    Description: Lisbona
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: restricted
    Keywords: Orbital tuning ; Magnetostratigraphy ; Cyclostratigraphy ; ODP ; 03. Hydrosphere::03.01. General::03.01.06. Paleoceanography and paleoclimatology ; 04. Solid Earth::04.04. Geology::04.04.08. Sediments: dating, processes, transport ; 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Extended abstract
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  • 8
    Publication Date: 2022-05-04
    Description: The Global Stratotype Section and Point (GSSP) for the base of the Bartonian (middle Eocene) stage is as yet undefined. Herein we assess the GSSP potential of the successions found in the Basque–Cantabrian and Aquitanian basins (western Pyrenees). On the basis of the available data, no outcrop in the Biarritz and Pamplona areas fulfilled the requirements outlined by the International Commission on Stratigraphy. However, the succession exposed on the eastern side of the Cape of Oyambre (San Vicente de la Barquera, province of Cantabria, northern Spain) did so, and yielded positive preliminary results.
    Description: Published
    Description: Lisbona
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: restricted
    Keywords: Eocene ; Bartonian ; GSSP ; Pyrenees ; Cantabria ; Oyambre ; 03. Hydrosphere::03.01. General::03.01.06. Paleoceanography and paleoclimatology ; 04. Solid Earth::04.04. Geology::04.04.08. Sediments: dating, processes, transport ; 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Extended abstract
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  • 9
    Publication Date: 2022-05-04
    Description: The Global Stratotype Section and Point (GSSP) for the base of the Bartonian (middle Eocene) stage is as yet undefined. Here, we assess the GSSP potential of the La Acebosa Formation exposed on the eastern side of the Cape of Oyambre (San Vicente de la Barquera, province of Cantabria, northern Spain). Sedimentological and benthic foraminiferal data indicate that the La Acebosa Formation represents a bathyal environment related to a deepening, eastwardfacing slope. Preliminary planktic foraminiferal and calcareous nannofossil results show that the upper part of the section corresponds to zones E11 and CP14a, respectively, and thus could include the Lutetian–Bartonian boundary. Although the quality of demagnetization is quite poor, preliminary magnetostratigraphic data suggest that Chron C19n, which is most likely to define the Bartonian GSSP, could be recorded in the upper part of the La Acebosa Formation. A denser magnetostratigraphic and biostratigraphic sampling is required in the upper part of this unit in order to accurately identify Chron C19n and to establish the sequence of events across the Lutetian–Bartonian transition.
    Description: Published
    Description: Lisbona
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: restricted
    Keywords: Eocene ; Bartonian ; GSSP ; Pyrenees ; Cantabria ; Oyambre ; 03. Hydrosphere::03.01. General::03.01.06. Paleoceanography and paleoclimatology ; 04. Solid Earth::04.04. Geology::04.04.08. Sediments: dating, processes, transport ; 04. Solid Earth::04.04. Geology::04.04.10. Stratigraphy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Extended abstract
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