Unraveling remagnetization sources using statistical learning
Carregando...
Data
Título da Revista
ISSN da Revista
Título de Volume
Editor
Resumo
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.
Descrição
Palavras-chave
Citação
GALLO, L. C. et al. Unraveling remagnetization sources using statistical learning. Earth and Planetary Science Letters, Amsterdam, v. 662, e119390, 2025. DOI: 10.1016/j.epsl.2025.119390. Disponível em: . Acesso em: 5 jul. 2026. DOI: . Disponível em: https://www.sciencedirect.com/science/article/pii/S0012821X2500189X. Acesso em: 5 jul. 2026.