Absolute paleointensity results from the Equator and the Pliocene-Pleistocene dipole field
Abstract
The current geomagnetic field (GMF) of the Earth is mostly geocentric dipolar with intensities in polar regions (~60 μT) about twice as high as in equatorial regions (~30 μT). However, Lawrence et al. [2009] found that the 0-5 Ma average paleointensity from 41 lava flow sites in Antarctica (~78°S) was only 31.5 μT. We present absolute paleointensity results from lava flows of similar age (0-3 Ma) from the Galapagos Islands located within 1°S of the Equator using a recently developed multidomain (MD) correction technique [Wang and Kent, 2013] on fresh subsets of the same samples that were recently analyzed for PSV [Kent, Wang & Rochette, 2010]. After standard Thellier series paleointensity experiments, we gave the samples total thermal remanent magnetizations (tTRM) by cooling from their Curie point in the presence of a laboratory-applied field (15 μT). We then repeated the paleointensity experiment on each sample, with the laboratory-applied tTRM as a synthetic natural remanent magnetization (NRM), using the same laboratory-applied field and temperature steps to obtain a synthetic Arai signature, which should only represent the domain-state dependent properties of the sample. We corrected the Arai diagrams from the original paleointensity experiment by using the Arai signatures from the repeated experiment, which neutralizes the typical MD concave-up Arai effect. We experimented on 3 specimens from each of 51 lava sites, 29 of which gave acceptable paleointensity results from one or more specimen(s). The average paleointensity of the 29 successful lava flow sites is ~29 μT (~23 μT for geometric mean). In these 29 sites, 12 of them are of normal polarity, yielding an average paleointensity of ~32 μT (geometric mean ~24 μT), and 17 of them are of reverse polarity, yielding an average paleointensity of ~27 μT (geometric mean ~23 μT). Mean paleomagnetic directions of the normal and reverse polarity sites are statistically antipodal and within a few degrees expected from the geocentric axial dipole (GAD) field, which together indicate that these data should be representative of the time-averaged geomagnetic field with no resolvable contributions from persistent non-dipole fields. These preliminary results from the Galapagos suggest that the average GMF intensity for the last few million years is comparable to the intensity of the present day field at the Equator. The results of Lawrence et al. [2009] from Antarctica also have mean paleomagnetic directions of normal and reverse polarity sites that are antipodal and conform to expectations from a GAD field, yet the mean GMF intensity is low by a factor of two compared to that from the Galapagos (or the present GMF). Either strongly biased paleointensity results or strong fluxes associated with the tangent cylinders in the outer core of the dynamo could be explanations of these observations.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2013
- Bibcode:
- 2013AGUFMGP53D..03W
- Keywords:
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- 1521 GEOMAGNETISM AND PALEOMAGNETISM Paleointensity;
- 1522 GEOMAGNETISM AND PALEOMAGNETISM Paleomagnetic secular variation;
- 1507 GEOMAGNETISM AND PALEOMAGNETISM Core processes