Early Cambrian renewal of the geodynamo and the origin of inner core structure
dc.contributor.author | Zhou, T. | |
dc.contributor.author | Tarduno, J.A. | |
dc.contributor.author | Nimmo, F. | |
dc.contributor.author | Cottrell, R.D. | |
dc.contributor.author | Bono, R.K. | |
dc.contributor.author | Ibanez-Mejia, M. | |
dc.contributor.author | Huang, W. | |
dc.contributor.author | Hamilton, M. | |
dc.contributor.author | Kodama, K. | |
dc.contributor.author | Smirnov, A.V. | |
dc.contributor.author | Crummins, B. | |
dc.contributor.author | Padgett, F., III | |
dc.date.accessioned | 2022-08-25T00:52:15Z | |
dc.date.available | 2022-08-25T00:52:15Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Zhou, T., Tarduno, J. A., Nimmo, F., Cottrell, R. D., Bono, R. K., Ibanez-Mejia, M., Huang, W., Hamilton, M., Kodama, K., Smirnov, A. V., Crummins, B., & Padgett, F., III. (2022). Early Cambrian renewal of the geodynamo and the origin of inner core structure. Nature Communications, 13(1). | |
dc.identifier.issn | 2041-1723 | |
dc.identifier.pmid | 35853855 | |
dc.identifier.doi | 10.1038/s41467-022-31677-7 | |
dc.identifier.uri | http://hdl.handle.net/10150/665954 | |
dc.description.abstract | Paleomagnetism can elucidate the origin of inner core structure by establishing when crystallization started. The salient signal is an ultralow field strength, associated with waning thermal energy to power the geodynamo from core-mantle heat flux, followed by a sharp intensity increase as new thermal and compositional sources of buoyancy become available once inner core nucleation (ICN) commences. Ultralow fields have been reported from Ediacaran (~565 Ma) rocks, but the transition to stronger strengths has been unclear. Herein, we present single crystal paleointensity results from early Cambrian (~532 Ma) anorthosites of Oklahoma. These yield a time-averaged dipole moment 5 times greater than that of the Ediacaran Period. This rapid renewal of the field, together with data defining ultralow strengths, constrains ICN to ~550 Ma. Thermal modeling using this onset age suggests the inner core had grown to 50% of its current radius, where seismic anisotropy changes, by ~450 Ma. We propose the seismic anisotropy of the outermost inner core reflects development of a global spherical harmonic degree-2 deep mantle structure at this time that has persisted to the present day. The imprint of an older degree-1 pattern is preserved in the innermost inner core. © 2022, The Author(s). | |
dc.language.iso | en | |
dc.publisher | Nature Research | |
dc.rights | Copyright © The Author(s) 2022. This article is licensed under a Creative Commons Attribution 4.0 International License. | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.title | Early Cambrian renewal of the geodynamo and the origin of inner core structure | |
dc.type | Article | |
dc.type | text | |
dc.contributor.department | Department of Geosciences, University of Arizona | |
dc.identifier.journal | Nature Communications | |
dc.description.note | Open access journal | |
dc.description.collectioninformation | This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu. | |
dc.eprint.version | Final published version | |
dc.source.journaltitle | Nature Communications | |
refterms.dateFOA | 2022-08-25T00:52:15Z |