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doi:10.1016/S0031-9201(03)00063-3    
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Copyright © 2003 Elsevier Science B.V. All rights reserved.

Inter-laboratory calibration of low-field magnetic and anhysteretic susceptibility measurements

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Leonardo SagnottiCorresponding Author Contact Information, E-mail The Corresponding Author, a, Pierre Rochetteb, Mike Jacksonc, Fabienne Vadeboinb, Jaume Dinarès-Turella, Aldo Winkler and “Mag-Net” Science Team1a

a Istituto Nazionale di Geofisica e Vulcanologia, Via Vigna Murata 605, 00143, Rome, Italy

b CEREGE, University of Aix-Marseille 3, BP80 13545, Aix en Provence, Cedex 4, France

c Institute for Rock Magnetism, University of Minnesota, Minneapolis, MN 55455, USA


Received 25 October 2002; 
revised 27 February 2003; 
accepted 2 March 2003. ;
Available online 9 May 2003.

Abstract

Inter-laboratory and absolute calibrations of rock magnetic parameters are fundamental for grounding a rock magnetic database and for semi-quantitative estimates about the magnetic mineral assemblage of a natural sample. Even a dimensionless ratio, such as anhysteretic susceptibility normalized by magnetic susceptibility (Ka/K) may be biased by improper calibration of one or both of the two instruments used to measure Ka and K. In addition, the intensity of the anhysteretic remanent magnetization (ARM) of a given sample depends on the experimental process by which the remanence is imparted. We report an inter-laboratory calibration of these two key parameters, using two sets of artificial reference samples: a paramagnetic rare earth salt, Gd2O3 and a commercial “pozzolanico” cement containing oxidized magnetite with grain size of less than 0.1 μm according to hysteresis properties. Using Gd2O3 the 10 Kappabridges magnetic susceptibility meters (AGICO KLY-2 or KLY-3 models) tested prove to be cross-calibrated to within 1%. On the other hand, Kappabridges provide a low-field susceptibility value that is ca. 6% lower than the tabulated value for Gd2O3, while average high-field susceptibility values measured on a range of instruments are indistinguishable from the tabulated value. Therefore, we suggest that Kappabridge values should be multiplied by 1.06 to achieve absolute calibration. Bartington Instruments magnetic susceptibility meters with MS2B sensors produce values that are 2–13% lower than Kappabridge values, with a strong dependence on sample centering within the sensor. The Ka/K ratio of ca. 11, originally obtained on discrete cement samples with a 2G Enterprises superconducting rock magnetometer and a KLY-2, is consistent with reference parameters for magnetites of grain size <0.1 μm. On the other hand, Ka values from a 2G Enterprises magnetometer and K values from a Bartington Instruments MS2C loop sensor for u-channel and discrete cement samples, will produce average Ka/K values that are unrealistically high if not properly corrected for the nominal volume detected by the sensors for these instruments. Inter-laboratory measurements of K and Ka for standard paleomagnetic plastic cubes filled with cement indicate remarkable differences in the intensity of the newly produced ARMs (with a standard deviation of ca. 21%), that are significantly larger than the differences observed from the calibration of the different magnetometers employed in each laboratory. Differences in the alternating field decay rate are likely the major source of these variations, but cannot account for all the observed variability. With such large variations in experimental conditions, classical interpretation of a “King plot” of Ka versus K would imply significant differences in the determination of grain size of magnetite particles on the same material.

Author Keywords: Rock magnetism; Magnetic susceptibility; Anhysteretic remanent magnetization; Calibration; Instrumentation; Relative paleointensity

Article Outline

1. Introduction
2. Material and instruments
3. Results
3.1. Gd2O3
3.2. Cement
4. Discussion
5. Conclusions
Acknowledgements
References










Corresponding Author Contact InformationCorresponding author. Tel.: +39-0651860321; fax: +39-0651860397.

1 Barbara Maher, Eva Moreno: University of Lancaster, UK; Monika Hanesch, Robert Scholger: University of Leoben, Austria; Robert Jude, John Shaw: University of Liverpool, UK; Gregg McIntosh, Maria Luisa Osete: University of Madrid, Spain; Jürgen Matzka, Nikolai Petersen: Ludwig-Maximilians-Universität München, Germany; Juan Cruz Larrasoaña, Matthew O’Reagan, Andrew P. Roberts: University of Southampton, UK; Tom Mullender, Clare Peters: University of Utrecht, The Netherlands; Kais J. Mohamed, Daniel Rey: University of Vigo, Spain; Jacqueline Hannam, Friedrich Heller: Institut für Geophysik, ETH Zürich, Switzerland; Thomas Frederichs, Ulrich Bleil: University of Bremen, Germany.


 
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