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Completing the Neogene geological time scale between 8.5 and 12.5 Ma

机译:完成8.5至12.5 Ma之间的新近纪地质时标

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摘要

A much improved high-resolution magnetostratigraphy is presented for the interval between 8.5 and 12.5 Ma in the deep marine astronomically tuned Monte dei Corvi Beach section in northern Italy. This section contains the formally designated boundary between the Middle and Upper Miocene defined by the Tortonian GSSP. The natural remanent magnetization is carried by an unusual low-temperature component of primary origin. According to interpretations of isothermal remanent magnetization (IRM) acquisition curves, the palaeomagnetic signal is most probably carried by iron sulphides, such as greigite or pyrrhotite. The resultant magnetostratigraphy is reliable and can be straightforwardly calibrated to the Astronomically Tuned Neogene Time Scale (ATNTS2004) showing that the section ranges from Chron C5An.2n up to C4.2r-1. The inferred correlation of the Tortonian GSSP to the older part of Chron C5r.2n is confirmed, thereby guaranteeing global correlation potential. In addition, the Monte dei Corvi Beach section has been re-tuned to the new numerical solution La2004 for the interval between 8.5 and 12.9 Ma. This exercise shows that the characteristic cycle patterns are not consistent with a single solution with fixed values for dynamical ellipticity and tidal dissipation. For the younger part of the section, sedimentary cycles show an excellent fit with intricate details of precession/obliquity interference in the nominal La2004((1,1)) solution. However, this solution produces serious mismatches between the sedimentary cycles and the precession/obliquity interference in the interval older than similar to 10.2 Ma. For this interval changes in tidal dissipation value (while keeping dynamical ellipticity constant at its present-day value) are necessary to maintain a perfect fit. A detailed visual comparison reveals a very good to excellent fit with La2004((1,1.2)) and, to lesser extent, with La2004((1,0.5)). However, La2004((1,1.2)) is the preferred tuning target for the moment in the interval older than 10.2 Ma. The astronomical (re)tuning on precessional scale to La2004((1,1)) yielded slightly different astronomical ages for each basic cycle and, hence, also for the calcareous plankton events and magnetic reversal boundaries with uncertainties ranging within a few thousand years. The age of the Tortonian GSSP turns into 11.625 Ma instead of the previously published 11.608 Ma. Our ages should replace existing ages in the Astronomically Tuned Neogene Time Scale (ATNTS2004). (c) 2006 Elsevier B.V. All rights reserved.
机译:在意大利北部深海天文调谐的Monte dei Corvi海滩剖面中,对于8.5 Ma和12.5 Ma之间的区间,提出了一种大大改善的高分辨率地层学。此部分包含由Tortonian GSSP定义的中新世与上中新世之间的正式边界。自然剩余的磁化强度是由主要来源的异常低温成分携带的。根据等温剩余磁化(IRM)采集曲线的解释,古磁信号极有可能由诸如铁镁铁矿或黄铁矿的硫化铁携带。由此产生的地层学是可靠的,并且可以直接校准为天文调整的新近纪时标(ATNTS2004),显示该剖面的范围从Chron C5An.2n到C4.2r-1。证实了Tortonian GSSP与Chron C5r.2n较早部分的推断相关性,从而保证了整体相关性。此外,Monte dei Corvi海滩部分已重新调整为新的数值解La2004,间隔为8​​.5-12.9 Ma。此练习表明,特征周期模式与动态椭圆率和潮汐耗散的固定值的单个解决方案不一致。对于该部分的较年轻部分,沉积旋回显示出极佳的拟合度,并具有名义上的La2004((1,1))解决方案中进动/倾斜干扰的复杂细节。但是,这种解决方案在比约10.2 Ma更早的时间间隔内,在沉积循环和旋进/倾角干扰之间产生了严重的失配。对于此间隔,必须保持潮汐耗散值的变化(同时将动态椭圆率保持在当前值不变),以保持最佳配合。详细的视觉比较揭示了与La2004((1,1.2))的匹配性非常好,而与La2004((1,0.5))的匹配程度较小。但是,对于时间间隔大于10.2 Ma的那一刻,La2004((1,1.2))是首选的调整目标。进动规模至La2004((1,1))的天文(再)调谐产生的每个基本周期的天文年龄略有不同,因此,钙质浮游生物事件和磁性反转边界的不确定性在几千年内。 Tortonian GSSP的年龄变为11.625 Ma,而不是先前发布的11.608 Ma。我们的年龄应该代替天文调整的新近纪时间量表(ATNTS2004)中的现有年龄。 (c)2006 Elsevier B.V.保留所有权利。

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