Cyclostratigraphy of the Middle Jurassic Aalenian Sha-1 member lacustrine record in central Sichuan Basin, southwestern China

Xiao-Fei Feng , Xiao-Ming Zhao , Massine Bouchakour , Xi Zhang , Jia-Wang Ge , Yue-Li Liang , Chang-Cheng Yang
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Abstract

Cyclostratigraphic studies enable to reconstruct the geological timescales of many marine formations. However, these investigations are still lacking a precise astronomical tuning in lacustrine environments, particularly in the Middle Jurassic, due to the paucity of biological traces and the lack of data. In this study, detailed spectral analyses of natural gamma ray (GR) logging data were conducted on the lacustrine Sha-1 member from two wells in the Sichuan Basin, southwestern China. Core data samples were calibrated to test the lithological changes for proceeding with cyclostratigraphic analysis with more confidence. The spectral analysis and evolutionary spectral analysis of the GR logs reveal that the wavelength ratios of the stratigraphic cycles are ∼20:5:2:1, being consistent with the period ratios of astronomical cycles (long eccentricity, short eccentricity, obliquity, and precession). Correlation coefficient (COCO) analyses were applied to quantitatively measure the fitting of the witnessed sedimentary cycles to astronomical periods and provide a possible sedimentation rate range. The results show that astronomical time scale of the studied interval comprises 58.4–60.6 m cycles, representing the 405 kyr eccentricity cycles, and 14.9–16.6 m cycles, representing the ∼100 kyr eccentricity cycles. This study reveals a ∼2.43 Myr duration for the Sha-1 member. Sedimentary noise modeling reveals that long-term million-year period (1.2 Myr) astronomical forcing may have been a significant driver of lake-level changes in the Sichuan Basin. Moreover, high-frequency (405 kyr scale) lake-level variations associated with the mid-term base-level cycles (4th-order sequences) were linked to climato-eustatic changes. This study suggests comparison between parameters of cyclostratigraphic records and sequence stratigraphic base-level cycles in lacustrine sediments. The stratigraphic surfaces of mid-term base-level cycles correspond to minima ∼405 kyr-long eccentricity cycle curve and high values of DYNOT (dynamic noise after orbital tuning). Integrating cyclostratigraphy with the base-level cycles is, therefore, a vital approach for defining the short-term oscillations of lake-level, and proved to be a useful tool for characterizing thin-bedded lacustrine reservoirs.
四川盆地中部中侏罗统阿勒世沙一段湖相记录旋回地层学
旋回地层学研究使我们能够重建许多海相地层的地质时间尺度。然而,由于缺乏生物痕迹和缺乏数据,这些研究仍然缺乏精确的湖泊环境天文调整,特别是在中侏罗世。本文对四川盆地沙1段两口井的自然伽马测井资料进行了详细的谱分析。对岩心数据样本进行了校准,以测试岩性变化,从而更有信心地进行旋回地层分析。GR测井资料的光谱分析和演化光谱分析表明,地层旋回的波长比为~ 20:5:2:1,与天文旋回的周期比(长偏心率、短偏心率、倾角和进动)一致。相关系数(COCO)分析定量测量了观测到的沉积旋回与天文周期的拟合,并提供了可能的沉积速率范围。结果表明,研究区间的天文时标为58.4 ~ 60.6 m周期,代表405 kyr的偏心周期;14.9 ~ 16.6 m周期,代表~ 100 kyr的偏心周期。这项研究揭示了Sha-1成员的持续时间为2.43 Myr。沉积噪声模型显示,长期的百万年(1.2 Myr)天文强迫可能是四川盆地湖泊水位变化的重要驱动因素。此外,与中期基准面旋回(4级序列)相关的高频(405 kyr尺度)湖泊水位变化与气候上升变化有关。提出了湖相沉积物旋回地层记录参数与层序地层基准面旋回参数的比较。中期基准面旋回的地层表面对应于最小~ 405 kyr-长的偏心旋回曲线和高DYNOT(轨道调谐后的动态噪声)值。因此,将旋回地层学与基准面旋回相结合是确定湖平面短期波动的重要方法,并被证明是表征薄层湖相储层的有用工具。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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