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The “van Zijl” Jurassic geomagnetic reversal revisited
Author(s) -
Moulin Maud,
Courtillot Vincent,
Fluteau Frédéric,
Valet JeanPierre
Publication year - 2012
Publication title -
geochemistry, geophysics, geosystems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.928
H-Index - 136
ISSN - 1525-2027
DOI - 10.1029/2011gc003910
Subject(s) - paleomagnetism , geology , polarity reversal , polarity (international relations) , geomagnetic reversal , equator , earth's magnetic field , geodesy , magnetostratigraphy , intensity (physics) , paleontology , reversing , dipole , latitude , physics , magnetic field , optics , chemistry , materials science , voltage , cell , composite material , biochemistry , quantum mechanics
We have collected two new detailed records of what could be the second oldest well documented reversal, the “van Zijl” Jurassic (∼180 Ma) reversal recorded in the thick basalt sequences of the Karoo large igneous province in Lesotho and South Africa. Sections yielded 10 and 8 independent transitional paleomagnetic directions respectively over two continuous 130 m and 160 m sequences. The corresponding VGP reversing paths share a number of consistent features and are integrated with a third record at Bushmen's Pass from Prévot et al. (2003) to yield a single reversal path with: 1‐ a large directional jump with no transitional poles between 45°S and 45°N in the first, main phase of the reversal, 2‐ a large elongated loop (multiple hairpin) to the SE with poles going down to ∼20° latitudes in the second phase of the reversal, and 3‐ a rebound before finally settling in normal polarity. We have measured relative paleo‐intensities on a set of carefully selected samples. Intensity was low prior to the directional changes and recovery to the following normal polarity was progressive. Transitional intensity is 80 to 90% lower than full polarity values. There is no significant increase in intensity at the time of transitional directional clusters. Our results are consistent with a weak non‐dipolar reversing field, with faster and larger directional secular variation as the equator is crossed by VGPs. They tend to vindicate the notion of a short duration of the directional reversal, though one cannot draw global conclusions from a record limited to essentially a single location.

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