Cyclostratigraphy of a type-Maastrichtian chalk record, based on high-resolution geochemical analysis of the Gulpen Formation, NE Belgium 

Jarno Huygh, J. Vellekoop, M. Sinnesael, P. Kaskes, J. Jagt, P. Claeys
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Abstract

Cyclostratigraphic studies on carbonate successions have proved invaluable for understanding palaeoclimate and for constructing improved, high-resolution age models of the Late Cretaceous. Whereas carbonate strata from the type-Maastrichtian from the Netherlands and Belgium have provided a wealth of palaeontological data, so far, dating of these deposits has relied mainly on biostratigraphy and preliminary attempts at cyclostratigraphy. The existing basic cyclostratigraphic framework is based principally on apparent cyclic variations in bioclast composition and suggested Milankovitch-paced flint cycles. Until now, these strata have not yet been examined using a cyclostratigraphic approach based on high-resolution multi-proxy geochemical data sets. Within the scope of the Maastrichtian Geoheritage Project, we attempt to construct an improved astrochronological age model for Maastrichtian chalk deposits of the Gulpen Formation.
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基于比利时东北部Gulpen组高分辨率地球化学分析的马斯特里赫特型白垩系旋回地层
碳酸盐层序的旋回地层学研究对于理解古气候和构建改进的、高分辨率的晚白垩世年龄模型是非常宝贵的。尽管荷兰和比利时的马斯特里赫特型碳酸盐地层提供了丰富的古生物学资料,但迄今为止,这些沉积物的测年主要依赖于生物地层学和旋回地层学的初步尝试。现有的基本旋回地层格架主要基于生物碎屑组成的明显旋回变化和米兰科维奇节奏的燧石旋回。到目前为止,这些地层还没有使用基于高分辨率多代理地球化学数据集的旋回地层方法进行检测。在马斯特里赫特地质遗产项目的范围内,我们试图建立一个改进的马斯特里赫特Gulpen组白垩沉积的天文年代学模型。
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