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Oligocene–Miocene magnetostratigraphy of deep-sea sediments from the equatorial Pacific (IODP Site U1333)

By
E. P. Guidry
E. P. Guidry
School of Geosciences, University of Louisiana at Lafayette, PO Box 44530, Lafayette, LA 70504, USA
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C. Richter
C. Richter
School of Geosciences, University of Louisiana at Lafayette, PO Box 44530, Lafayette, LA 70504, USA
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G. D. Acton
G. D. Acton
Department of Geology, University of California, Davis, One Shields Avenue, Davis, CA 95616, USA
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J. E. T. Channell
J. E. T. Channell
Department of Geological Sciences, University of Florida, PO Box 112120, Gainesville, FL 32611-2120, USA
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H. F. Evans
H. F. Evans
LDEO, PO Box 1000, Palisades, NY 10964-8000, USA
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C. Ohneiser
C. Ohneiser
Geology Department, University of Otago, PO Box 56, Dunedin 9054, New Zealand
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Y. Yamamoto
Y. Yamamoto
Center for Advanced Marine Core Research, Kochi University, B200 Monobe, Nankoku, Kochi 783-8502, Japan
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T. Yamazaki
T. Yamazaki
Geological Survey of Japan, AIST Tsukuba Central 7, Tsukuba 305-8567, Japan
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Published:
January 01, 2013

Abstract

We present palaeomagnetic results from the Oligocene through Miocene part of the Integrated Ocean Drilling Program Site U1333 (1030.996′N, 138°25.159′W), which is located in 4853 m-deep water over seafloor with an estimated crustal age of 46 Ma. Detailed magnetostratigraphic investigations are essential to provide a sound age model for the study of the palaeoclimatic and palaeo-oceanographic history of the Cenozoic of the Equatorial Pacific and to improve the database of Pacific magnetostratigraphy. Rock magnetic measurements were carried out at 1 cm resolution on 81 U-channel samples from the spliced section with the goal of extracting a high-resolution record of the magnetostratigraphy. Stepwise demagnetization of the natural remanent magnetization yielded a well-defined magnetostratigraphy over a time interval of approximately 10 Ma between the base of Chron C6n (19.722 Ma) and the middle of Chron C11r (>29.9 Ma) and identification of the Oligocene–Miocene transition at the base of Subchron C6Cn.2n. The palaeomagnetic data are characterized by shallow inclinations, and by 180° alternations in declinations downhole, reflecting magnetic polarity zones. The relatively high temporal resolution allowed for the identification of three possible excursions previously not identified on the geomagnetic polarity time scale, which were recorded in Subchrons C8n.1r and C11n.2n and in Chron C11r.

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Contents

Geological Society, London, Special Publications

Magnetic Methods and the Timing of Geological Processes

L. Jovane
L. Jovane
Universidade de Saão Paulo, Brazil
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E. Herrero-Bervera
E. Herrero-Bervera
University of Hawaii at Manoa, USA
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L.A. Hinnov
L.A. Hinnov
Johns Hopkins University, USA
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B. Housen
B. Housen
Western Washington University, USA
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Geological Society of London
Volume
373
ISBN electronic:
9781862396364
Publication date:
January 01, 2013

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