Dipole fluctuations and the duration of geomagnetic polarity transitions
Geomagnetic polarity transitions are often accompanied by a decrease in magnetic intensity. The time required to reestablish the magnetic intensity after a transition is usually longer than the duration based on magnetic direction. Analysis of the paleomagnetic axial dipole moment from the PADM2M mo...
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Published in | Geophysical research letters Vol. 42; no. 18; pp. 7444 - 7451 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Washington
Blackwell Publishing Ltd
28.09.2015
John Wiley & Sons, Inc |
Subjects | |
Online Access | Get full text |
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Summary: | Geomagnetic polarity transitions are often accompanied by a decrease in magnetic intensity. The time required to reestablish the magnetic intensity after a transition is usually longer than the duration based on magnetic direction. Analysis of the paleomagnetic axial dipole moment from the PADM2M model shows a return to the time‐averaged intensity after 42 kyr. A shorter time is required to recover a fraction of the time‐averaged moment, but the correspondence between recovery time and fraction of recovery is nonlinear. Predictions of a stochastic model reproduce the general trends in recovery time and suggest that fluctuations in dipole generation increase substantially during polarity transitions relative to times of stable polarity. These large fluctuations could reflect larger convective velocities in the core or represent a change in the efficiency of dipole generation. In either case, large fluctuations during polarity transitions can flip the sign of the axial dipole field several times before a polarity transition is completed.
Key Points
Reversal duration predicted using stochastic model
Fluctuations in dipole generation increase during polarity transition
Axial dipole may flip several times during a reversal |
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Bibliography: | ark:/67375/WNG-XTZF1HS2-L ArticleID:GRL53465 Data S1Supporting Information S1 istex:80E7D08F59504A6BA8A5F303221BB594AE9E5B6C ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1002/2015GL065700 |