Implications of Dipole Movement Secular Variation from 50,000-10,000 Years for the Radiocarbon Record
dc.contributor.author | Sternberg, R. S. | |
dc.contributor.author | Damon, Paul E. | |
dc.date.accessioned | 2021-02-11T20:33:11Z | |
dc.date.available | 2021-02-11T20:33:11Z | |
dc.date.issued | 1992-01-01 | |
dc.identifier.citation | Sternberg, R. S., & Damon, P. E. (1992). Implications of dipole moment secular variation from 50,000–10,000 years for the radiocarbon record. Radiocarbon, 34(2), 189-198. | |
dc.identifier.issn | 0033-8222 | |
dc.identifier.doi | 10.1017/S0033822200013618 | |
dc.identifier.uri | http://hdl.handle.net/10150/653325 | |
dc.description.abstract | Sparse paleointensity data from 10–50 ka suggest that the average dipole moment (DM) was 50–75% of the average of 8.67 X 1022 A m2 for the past 5 Ma, and 8.75 X 1022 for the past 12 ka. A linear ramp function, increasing the DM from 4 to 8.75 X 1022 A m2 between 50–10 ka BP, generates a total 14C inventory of 126 dpm/cme^2, agreeing very well with an inventory assay of 128 dpm/cme^2, which includes 14C in sediments. With the Lingenfelter and Ramaty (1970) production function and a model DC gain of about 100, this DM function would give a Delta-14C of 500 per mil at 20 ka BP, consistent with the Barbados coral record, and also gives a good match to the Holocene record. A Laschamp geomagnetic event at about 45 ka BP, with a DM of 25% of its average value and lasting 5 ka, would only increase the present inventory by 0.3–1.2 dpm/cme 2, and would probably have only a small effect on Delta-14C at 20 ka BP, but could produce a short-lived 14C spike of over 500 per mil. | |
dc.language.iso | en | |
dc.publisher | Department of Geosciences, The University of Arizona | |
dc.relation.url | http://radiocarbon.webhost.uits.arizona.edu/ | |
dc.rights | Copyright © by the Arizona Board of Regents on behalf of the University of Arizona. All rights reserved. | |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
dc.subject | cosmochronology | |
dc.subject | cosmochemistry | |
dc.subject | dipole moment | |
dc.subject | paleomagnetism | |
dc.subject | secular variations | |
dc.subject | magnetic field | |
dc.subject | Pleistocene | |
dc.subject | Cenozoic | |
dc.subject | Quaternary | |
dc.subject | C 14 | |
dc.subject | carbon | |
dc.subject | isotopes | |
dc.subject | radioactive isotopes | |
dc.title | Implications of Dipole Movement Secular Variation from 50,000-10,000 Years for the Radiocarbon Record | |
dc.type | Article | |
dc.type | text | |
dc.identifier.journal | Radiocarbon | |
dc.description.note | This material was digitized as part of a cooperative project between Radiocarbon and the University of Arizona Libraries. | |
dc.description.collectioninformation | The Radiocarbon archives are made available by Radiocarbon and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information. | |
dc.eprint.version | Final published version | |
dc.description.admin-note | Migrated from OJS platform February 2021 | |
dc.source.volume | 34 | |
dc.source.issue | 2 | |
dc.source.beginpage | 189 | |
dc.source.endpage | 198 | |
refterms.dateFOA | 2021-02-11T20:33:11Z |