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Late Cambrian geomagnetic instability after the onset of inner core nucleation
The Ediacaran Period marks a pivotal time in geodynamo evolution when the geomagnetic field is thought to approach the weak state where kinetic energy exceeds magnetic energy, as manifested by an extremely high frequency of polarity reversals, high secular variation, and an ultralow dipole field str...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10390560/ https://www.ncbi.nlm.nih.gov/pubmed/37524710 http://dx.doi.org/10.1038/s41467-023-40309-7 |
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author | Li, Yong-Xiang Tarduno, John A. Jiao, Wenjun Liu, Xinyu Peng, Shanchi Xu, Shihua Yang, Aihua Yang, Zhenyu |
author_facet | Li, Yong-Xiang Tarduno, John A. Jiao, Wenjun Liu, Xinyu Peng, Shanchi Xu, Shihua Yang, Aihua Yang, Zhenyu |
author_sort | Li, Yong-Xiang |
collection | PubMed |
description | The Ediacaran Period marks a pivotal time in geodynamo evolution when the geomagnetic field is thought to approach the weak state where kinetic energy exceeds magnetic energy, as manifested by an extremely high frequency of polarity reversals, high secular variation, and an ultralow dipole field strength. However, how the geodynamo transitioned from this state into one with more stable field behavior is unknown. Here, we address this issue through a high-resolution magnetostratigraphic investigation of the ~494.5 million-year-old Jiangshanian Global Standard Stratotype and Point (GSSP) section in South China. Our paleomagnetic results document zones with rapid reversals, stable polarity and a ~80 thousand-year-long interval without a geocentric axial dipole field. From these changes, we suggest that for most of the Cambrian, the solid inner core had not yet grown to a size sufficiently large to stabilize the geodynamo. This unusual field behavior can explain paleomagnetic data used to define paradoxical true polar wander, supporting instead the rotational stability of the solid Earth during the great radiation of life in the Cambrian. |
format | Online Article Text |
id | pubmed-10390560 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-103905602023-08-02 Late Cambrian geomagnetic instability after the onset of inner core nucleation Li, Yong-Xiang Tarduno, John A. Jiao, Wenjun Liu, Xinyu Peng, Shanchi Xu, Shihua Yang, Aihua Yang, Zhenyu Nat Commun Article The Ediacaran Period marks a pivotal time in geodynamo evolution when the geomagnetic field is thought to approach the weak state where kinetic energy exceeds magnetic energy, as manifested by an extremely high frequency of polarity reversals, high secular variation, and an ultralow dipole field strength. However, how the geodynamo transitioned from this state into one with more stable field behavior is unknown. Here, we address this issue through a high-resolution magnetostratigraphic investigation of the ~494.5 million-year-old Jiangshanian Global Standard Stratotype and Point (GSSP) section in South China. Our paleomagnetic results document zones with rapid reversals, stable polarity and a ~80 thousand-year-long interval without a geocentric axial dipole field. From these changes, we suggest that for most of the Cambrian, the solid inner core had not yet grown to a size sufficiently large to stabilize the geodynamo. This unusual field behavior can explain paleomagnetic data used to define paradoxical true polar wander, supporting instead the rotational stability of the solid Earth during the great radiation of life in the Cambrian. Nature Publishing Group UK 2023-07-31 /pmc/articles/PMC10390560/ /pubmed/37524710 http://dx.doi.org/10.1038/s41467-023-40309-7 Text en © The Author(s) 2023, corrected publication 2023 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Li, Yong-Xiang Tarduno, John A. Jiao, Wenjun Liu, Xinyu Peng, Shanchi Xu, Shihua Yang, Aihua Yang, Zhenyu Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title | Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title_full | Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title_fullStr | Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title_full_unstemmed | Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title_short | Late Cambrian geomagnetic instability after the onset of inner core nucleation |
title_sort | late cambrian geomagnetic instability after the onset of inner core nucleation |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10390560/ https://www.ncbi.nlm.nih.gov/pubmed/37524710 http://dx.doi.org/10.1038/s41467-023-40309-7 |
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