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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 103, NO. B8,
PAGES 17,735–17,748,
1998
Analysis of 11 Myr of geomagnetic intensity variation
Catherine G. Constable
Scripps Institution of Oceanography, University of California at San Diego, La Jolla
Lisa Tauxe
Scripps Institution of Oceanography, University of California at San Diego, La Jolla
Robert L. Parker
Scripps Institution of Oceanography, University of California at San Diego, La Jolla
Abstract
We have conducted a detailed exploratory analysis of an 11 million year long almost continuous record of relative geomagnetic
paleointensity from a sediment core acquired on Deep Sea Drilling Project Leg 73, at Site 522 in the South Atlantic. We assess
the quality of the paleointensity record using spectral methods and conclude that the relative intensity record is minimally
influenced by climate variations. Isothermal remanence is shown to be the most effective normalizer for these data, although
both susceptibility and anhysteretic remanence are also adequate. Statistical analysis shows that the paleointensity variations
follow a gamma distribution, and are compatible with predictions from modified paleosecular variation models and global absolute
paleointensity data. When subdivided by polarity interval, the variability in paleointensity is proportional to the average,
and further, the average is weakly correlated with interval length. Spectral estimates for times from 28.77 until 22.74 Ma,
when the reversal rate is about 4 Myr−1, are compatible with a Poisson model in which the spectrum of intensity variations is dominated by the reversal process in
the frequency range 1–50 Myr−1. In contrast, between 34.7 and 29.4 Ma, when the reversal rate is about 1.6 Myr−1, the spectra indicate a different secular variation regime. The magnetic field is stronger, and more variable, and a strong
peak in the spectrum occurs at about 8 Myr−1. This peak may be a reflection of the same signal as recorded by the small variations known as tiny wiggles seen in marine
magnetic anomaly profiles.
Received 11
September
1997;
accepted 30
April
1998.
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Citation: Constable, C. G., L. Tauxe, and R. L. Parker
(1998),
Analysis of 11 Myr of geomagnetic intensity variation,
J. Geophys. Res.,
103(B8),
17,735–17,748.
Copyright 1998 by the American Geophysical Union.
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