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首页> 外文期刊>Quaternary International >Integrated stratigraphy and astronomical tuning of lower-middle Pleistocene Montalbano Jonico section (southern Italy)
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Integrated stratigraphy and astronomical tuning of lower-middle Pleistocene Montalbano Jonico section (southern Italy)

机译:下中新世蒙塔尔巴诺乔尼科断层(意大利南部)的地层和天文综合调谐

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摘要

Astronomical calibration of the lower-middle Pleistocene Montalbano Jonico section located in the Lucania Basin (Southern Italy) is presented. Previous papers widely discussed the integrated stratigraphy (calcareous nannofossils, sapropel stratigraphy, benthic and planktonic oxygen stable isotopes) and the paleoenvironmental features of this section and its potential suitability for the selection of the Middle Pleistocene Global Stratotype Section and Point (GSSP). In this study, new planktonic δ~(18)O data, additional biostratigraphical constraints and new tephrochronology on volcaniclastic layers occurring within the studied record are reported. The new chronostratigraphic framework provides a robust base for correlation of the oxygen isotope stratigraphy for the Montalbano Jonico section with the glacial and interglacial fluctuations of the Oceanic and Mediterranean δ~(18)O reference deep-sea records. Specifically, the lower part of the Montalbano Jonico section (Interval A) provides correlation of the planktonic and benthic δ~(18)O cycles to Marine Isotope Stage (MIS) 36 to MIS 23. Interval A includes a distinct peak of left-coiled neo-globoquadrinids, the Globoratalia crassaformis influx, the First Occurrence of Gephyrocapsa omega, and the First Common Occurrence and Last Common Occurrence of Reticulofenestra asanoi. These stratigraphical constraints support the tuning of five sapropel layers included in this part of the section to insolation cycles i-112, i-104, i-102, i-90 and i-86. The upper part of the section (Interval B), which includes the temporary disappearance (td2) of G. omega and tephra layer V5, Ar/Ar age dated at 719.5 ± 12.6 ka, is consistent with identification of MIS 22 to MIS 16 in the planktonic δ~(18)O pattern. The δ~(18)O time series of the whole section was reconstructed using the midpoints of individual sapropels and their correlative precession minima, visual comparison of the δ~(18)O pattern with the record available at the Mediterranean ODP Site 975, and, in the upper part of the section, the Ar/Ar age of tephra V5. The developed astronomical tuning revealed that the Montalbano Jonico section covers an interval from 1240 ka to 645 ka. A significant change in sedimentation rate occurs between Intervals A (0.53 m/ky) and Interval B (0.91 m/ky) at about 870 ka and is consistent with a sea-level drop from a bathyal to a circalittoral environment. Bioevents recognised in the Montalbano Jonico section have been dated according to the astronomical calibration, and age assignments of tephra V1-V4 and V6-V9 are also proposed. The Montalbano Jonico section fills the gap between the top of the Vrica section and the base of the Ionian informal Middle Pleistocene stage, and represents a Mediterranean reference section for the Mid-Pleistocene transition.
机译:介绍了位于卢卡尼亚盆地(意大利南部)的下中更新世蒙塔尔巴诺乔尼科断层的天文校准。先前的论文广泛讨论了综合地层学(钙质纳米化石,腐殖质地层,底栖和浮游性氧稳定同位素)和本节的古环境特征及其对选择中更新世全球层状剖面和点(GSSP)的潜在适用性。在这项研究中,报道了新的浮游性δ〜(18)O数据,附加的生物地层学约束和研究记录中火山碎屑层的新年代学。新的年代地层学框架为Montalbano Jonico断面的氧同位素地层与海洋和地中海δ〜(18)O参考深海记录的冰川和冰川间波动的相关性提供了坚实的基础。具体而言,蒙塔尔巴诺乔尼科区的下部(区间A)提供了浮游和底栖δ〜(18)O循环与海洋同位素阶段(MIS)36到MIS 23的相关性。区间A包含一个明显的左旋峰新球藻,类球藻大量涌入,初次发生的gephyrocapsa omega以及初次发生和最后一次发生网状网脉。这些地层学约束支持将本节此部分中包括的五个腐腐土层调整到日晒周期i-112,i-104,i-102,i-90和i-86。该部分的上部(间隔B)包括G. omega和Tephra V5层的临时消失(td2),Ar / Ar年龄为719.5±12.6 ka,与MIS 22到MIS 16的识别相一致。浮游δ〜(18)O型整个剖面的δ〜(18)O时间序列是使用单个腐殖质的中点及其相关的岁差最小值,δ〜(18)O模式的视觉比较和地中海ODP站点975上的记录重建的,在该部分的上部,是tephra V5的Ar / Ar年龄。发达的天文调谐表明,蒙塔尔巴诺乔尼科断面的时间间隔为1240 ka至645 ka。区间A(0.53 m / ky)和区间B(0.91 m / ky)之间的沉积速率发生了显着变化,大约为870 ka。这与从海底环境到周缘环境的海平面下降是一致的。 Montalbano Jonico部分中认可的生物事件已根据天文学标定了日期,并且还提出了Tephra V1-V4和V6-V9的年龄分配。 Montalbano Jonico剖面填补了Vrica剖面顶部和爱奥尼亚非正式中更新世​​阶段底部之间的空隙,并且代表了地中海中更新世过渡的参考剖面。

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  • 来源
    《Quaternary International》 |2010年第2010期|109-120|共12页
  • 作者单位

    Dipartimento di Geologia e Geofisica, Universita di Bari, Via E. Orabona 4, 70125 Ban, Italy;

    Istituto per l'Ambiente Marino Costiero (IAMC) Sede Napoli - CNR, Calata Porta di Massa, Intemo Porto di Napoli, 80133, Napoli, Italy;

    Dipartimento di Scienze della Terra, Universita degli Studi di Napoli Federico II, Lgo San Marcellino 10, 80138 Napoli, Italy;

    Faculty of Geosciences, Department of Earth Sciences, Utrecht University, Utrecht, The Netherlands;

    Dipartimento di Geologia e Geofisica, Universita di Bari, Via E. Orabona 4, 70125 Ban, Italy;

    Dipartimento di Geologia e Geofisica, Universita di Bari, Via E. Orabona 4, 70125 Ban, Italy;

    Dipartimento di Scienze della Terra, Universita degli Studi di Napoli Federico II, Lgo San Marcellino 10, 80138 Napoli, Italy;

    Istituto per l'Ambiente Marino Costiero (IAMC) Sede Napoli - CNR, Calata Porta di Massa, Intemo Porto di Napoli, 80133, Napoli, Italy;

    Dipartimento di Geologia e Geofisica, Universita di Bari, Via E. Orabona 4, 70125 Ban, Italy;

    Istituto di Geologia Ambientale e Geoingegneria (IGAG)-CNR, Via Bolognola 7, 00138 Rome, Italy;

    Dipartimento di Geologia e Geofisica, Universita di Bari, Via E. Orabona 4, 70125 Ban, Italy;

    UMR 5125 PEPS, CNRS, France Universite Lyon 1, Campus de La Doua, Batiment Geode, 69622 Villeurbanne Cedex, France;

    Istituto per l'Ambiente Marino Costiero (IAMC) Sede Napoli - CNR, Calata Porta di Massa, Intemo Porto di Napoli, 80133, Napoli, Italy;

    Istituto per l'Ambiente Marino Costiero (IAMC) Sede Napoli - CNR, Calata Porta di Massa, Intemo Porto di Napoli, 80133, Napoli, Italy;

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