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Physics of The Earth and Planetary Interiors
Volume 156, Issues 3-4, 14 July 2006, Pages 205-212
ODP Contributions to Paleomagnetism
 
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doi:10.1016/j.pepi.2005.03.020    
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Copyright © 2006 Elsevier B.V. All rights reserved.

A comparison of relative paleointensity records of the Matuyama Chron for the period 0.75–1.25 Ma

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Yohan Guyodoa, b, Corresponding Author Contact Information, E-mail The Corresponding Author and Jean-Pierre Valetc

aLaboratoire des Sciences du Climat et de l’Environnement, Domaine du CNRS, Bât 12, Ave de la Terrasse, 91198 Gif-sur-Yvette Cedex, France

bInstitute for Rock Magnetism, Department of Geology and Geophysics, 108 Pillsbury Hall, University of Minnesota, Minneapolis, MN 55455, USA

cInstitut de Physique du Globe de Paris, 4, Place Jussieu, 75252 Paris Cedex 05, France


Received 15 April 2004; 
revised 1 March 2005; 
accepted 11 March 2005. 
Available online 24 February 2006.

Abstract

A comparison of 15 records of relative geomagnetic paleointensity, spanning the time interval 0.75–1.25 Ma, has been performed after synchronizing the records at the paleointensity minima corresponding to geomagnetic reversals. Filtering and smoothing of the records indicated that, after synchronization, paleointensity features with wavelengths larger than about 20 ky can be matched from one record to another, although age offsets can still be observed in several records. Further synchronization of the records, using intensity minima, permitted construction of a composite stack of these records. This stack provides useful information about the long-term evolution of the geomagnetic field intensity over this period of time, and confirms the existence of a rapid recovery of the field intensity after each reversal. Analysis of the standard deviation and jackknife calculation suggest that improvement in the stack accuracy and resolution could still be achieved with better-constrained age models.

Keywords: Geomagnetism; Paleomagnetism; Relative paleointensity; Matuyama

Article Outline

1. Introduction
2. First approach: reducing age discrepancies and filtering the records
3. Second approach: stacking the records
4. Conclusion
Acknowledgements
References








Corresponding Author Contact InformationCorresponding author. Tel.: +33 1 69 82 35 62; fax: +33 1 69 82 35 68.

Physics of The Earth and Planetary Interiors
Volume 156, Issues 3-4, 14 July 2006, Pages 205-212
ODP Contributions to Paleomagnetism
 
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