Unraveling remagnetization sources using statistical learning

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
L.C. Gallo , M. Domeier , P.Y. Antonio , F. Sapienza , A. Rapalini , E. Font , T. Adatte , R.I.F. Trindade , F. Temporim , J. Tonti-Filippini , P. Silkoset , L. Warren
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引用次数: 0

Abstract

The paleomagnetic archive provides invaluable insights into Earth's history, but its records are often obscured by various geological processes. A prime example is remagnetization, which can replace the original natural remanent magnetization. Although magnetic overprints can be detected by traditional paleomagnetic tests, the mechanisms responsible for them often remain elusive because linking bulk magnetic properties to their microscopic sources is inherently challenging. Here, we bridge this gap by pairing an extensive rock magnetic and geochemical dataset with statistical learning techniques for the first time. Using a Random Forest regressor trained on geochemical data, we accurately predict the growth of fine-grained magnetite in an undeformed late Ediacaran section of remagnetized carbonate rocks from Paraguay. Our modeling results identify the K/Al ratio—alongside K and Sr contents—as key predictors of this remagnetization mechanism. Notably, clay mineralogy analyses further link the K/Al ratio to enhanced clay authigenesis (illitization) driven by K-feldspar dissolution and albitization—processes that also release iron. Together, these findings indicate that remagnetization occurred via authigenic magnetite formation under isochemical diagenesis—without the involvement of external fluids. This novel application of statistical learning to uncover the geochemical drivers of chemical remagnetizations provides a robust framework to investigate and understand these events. It could also open new avenues for their direct dating, thereby significantly enriching the global paleomagnetic record.
利用统计学习揭示再磁化源
古地磁档案为了解地球历史提供了宝贵的见解,但其记录往往被各种地质过程所掩盖。一个最好的例子是再磁化,它可以代替原来的自然剩余磁化。虽然磁性套印可以通过传统的古地磁测试检测到,但其机制往往仍然难以捉摸,因为将整体磁性与其微观来源联系起来本身就是一项挑战。在这里,我们首次将广泛的岩石磁性和地球化学数据集与统计学习技术相结合,弥补了这一差距。利用地球化学数据训练的随机森林回归器,我们准确地预测了巴拉圭埃迪卡拉世晚期未变形的重磁化碳酸盐岩剖面中细粒磁铁矿的生长。我们的建模结果确定了K/Al比以及K和Sr含量是这种再磁化机制的关键预测因素。值得注意的是,粘土矿物学分析进一步将K/Al比值与钾长石溶解和钠化作用(也释放铁)驱动的粘土自生作用(illi石化)联系起来。总之,这些发现表明,在等化学成岩作用下,再磁化是通过自生磁铁矿形成的,没有外部流体的参与。这种统计学习的新应用揭示了化学再磁化的地球化学驱动因素,为调查和理解这些事件提供了一个强大的框架。它还可以为它们的直接测年开辟新的途径,从而显著丰富全球古地磁记录。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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