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    Implications of Dipole Movement Secular Variation from 50,000-10,000 Years for the Radiocarbon Record

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    Author
    Sternberg, R. S.
    Damon, Paul E.
    Issue Date
    1992-01-01
    Keywords
    cosmochronology
    cosmochemistry
    dipole moment
    paleomagnetism
    secular variations
    magnetic field
    Pleistocene
    Cenozoic
    Quaternary
    C 14
    carbon
    isotopes
    radioactive isotopes
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    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.
    Publisher
    Department of Geosciences, The University of Arizona
    Journal
    Radiocarbon
    URI
    http://hdl.handle.net/10150/653325
    DOI
    10.1017/S0033822200013618
    Additional Links
    http://radiocarbon.webhost.uits.arizona.edu/
    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.
    Type
    Article
    text
    Language
    en
    ISSN
    0033-8222
    ae974a485f413a2113503eed53cd6c53
    10.1017/S0033822200013618
    Scopus Count
    Collections
    Radiocarbon, Volume 34, Number 2 (1992)

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