新特提斯地区(突尼斯、西班牙北部和法国南部)的阿普tian序列、海平面、硅质通量和气候变化

IF 4 1区 地球科学 Q1 GEOGRAPHY, PHYSICAL
Najeh Ben Chabaane , Jihede Haj Messaoud , Fares Khemiri , Frans van Buchem
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引用次数: 0

摘要

利用突尼斯中部的露头剖面,构建了阿普提亚演替的碳酸盐岩台地-盆地样带。在新的生物地层信息和新的c同位素曲线的约束下,提出了高分辨率层序地层模型。将其与北特提斯边缘的三个参考剖面进行比较,以在新特提斯尺度上评价阿普提斯层序的时间和沉积模式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Aptian sequences, sea-level, siliciclastic flux and climate change in the Neo-Tethys domain (Tunisia, N. Spain and S. France)
A carbonate platform to basin transect of the Aptian succession has been constructed using outcrop sections in central Tunisia. Constrained by new biostratigraphic information and a new C-isotope curve a high-resolution sequence stratigraphic model is proposed. It is compared to three reference sections along the Northern Tethyan margin in order to evaluate the timing of the Aptian sequences and sedimentation patterns at the Neo-Tethys scale.
The Tunisian sections, which vary in thickness from 130 m in the inner platform to 850 m in the basin margin, display a rich variation in carbonate, siliciclastic and evaporite sedimentary facies. In the inner platform domain three significant stratigraphic hiatuses have been detected, whereas the basin margin section is complete, and comprises an 80 m thick siliciclastic/oolitic lowstand wedge deposited during the early late Aptian sealevel fall. This fall also marks the abrupt influx of continent-derived siliciclastics. Comparison of the Tunisian section to an equally extended basin margin section in northern Spain (Aralar platform), and basinal sections in southern France (Vocontian Basin) and southeastern Spain (Cau section), show a strikingly similar sequence stratigraphic organization at two orders. At the large scale, two supersequences can be correlated, of which the first one spans the early Aptian to the early part of the late Aptian, and is dominated by shales (including the OAE 1a), carbonates and evaporites. The second-order supersequence covers the remaining part of the late Aptian and earliest Albian and is characterized by a lowstand wedge caused by a eustatic sea-level drop of approx. 60-70 m, accompanied by a strong, basinwide, influx of siliciclastics around the Neo-Tethys Ocean. At the medium scale, six third-order sequences can be correlated across the Neo-Tethys domain.
The 2nd order lowstand wedge and siliciclastic influx are time equivalent with the coldest temperatures reported for the late Aptian, and coincide with the establishment of the Equatorial Humid Belt, all supporting a dramatic late Aptian climate change. The onfollowing overall transgression is co-eval with a gradual rise in temperatures, punctuated by short hyperthermal events. These events are locally expressed by the accumulation of organic matter (Jacob, Kilian, Paquier levels) and occur during the transgressions of the 3rd order sequences, interpreted here as the expression of a pulsed melting of the ice caps that caused the initital 2nd order sea level fall.
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来源期刊
Global and Planetary Change
Global and Planetary Change 地学天文-地球科学综合
CiteScore
7.40
自引率
10.30%
发文量
226
审稿时长
63 days
期刊介绍: The objective of the journal Global and Planetary Change is to provide a multi-disciplinary overview of the processes taking place in the Earth System and involved in planetary change over time. The journal focuses on records of the past and current state of the earth system, and future scenarios , and their link to global environmental change. Regional or process-oriented studies are welcome if they discuss global implications. Topics include, but are not limited to, changes in the dynamics and composition of the atmosphere, oceans and cryosphere, as well as climate change, sea level variation, observations/modelling of Earth processes from deep to (near-)surface and their coupling, global ecology, biogeography and the resilience/thresholds in ecosystems. Key criteria for the consideration of manuscripts are (a) the relevance for the global scientific community and/or (b) the wider implications for global scale problems, preferably combined with (c) having a significance beyond a single discipline. A clear focus on key processes associated with planetary scale change is strongly encouraged. Manuscripts can be submitted as either research contributions or as a review article. Every effort should be made towards the presentation of research outcomes in an understandable way for a broad readership.
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