TERRAPUB Earth, Planets and Space

Earth Planets Space, Vol. 51 (No. 5), pp. 329-336, 1999

Magnetic intensity loss and core diagenesis in long-core samples from the East Cortez Basin and the San Nicolas Basin (California Borderland)

Carl Richter1, Akira Hayashida2, Yohan Guyodo3, Jean-Pierre Valet3, and Kenneth L. Verosub4

1Ocean Drilling Program, 1000 Discovery Drive, Texas A&M University, College Station, TX 77845-9547, U.S.A.
2Science and Engineering Research Institute, Doshisha University, Kyoto 610-0321, Japan
3Institut de Physique du Globe de Paris,4, Place Jussieu, 75252 Paris Cedex 05, France
4Geology Department, University of California, Davis, CA 95616, U.S.A.

(Received July 16, 1998; Revised May 6, 1999; Accepted May 6, 1999)

Abstract: We performed high resolution magnetic measurements on about 180 m of continuous U-channel samples from Sites 1012 (East Cortez Basin) and 1013 (San Nicolas Basin) that were recovered during Ocean Drilling Program Leg 167 to the California Margin. Measurements were made at 1-2 cm intervals from near-complete composite stratigraphic sequences at both of the studied sites with the goal of obtaining high spatial resolution of sediment magnetic properties, including detailed characterization of variations in magnetic mineralogy, concentration, and grain size. The decay of a metastable magnetic mineral or the dissolution of fine-grained magnetite by organic matter reduction had strongly affected both cores, reducing the magnetic intensity to 7%-10% of the initial magnetization. Measurements were carried out ca. 4-6 months after the cores were drilled. Despite the reduced magnetic signal we were able to define a stable characteristic remanence for most of the core. Cyclic variations that were observed over short and long stratigraphic intervals are strongly driven at Earth orbital periodicities and have been used to obtain a detailed age model based on comparison with the insolation record.


Corresponding author E-mail: Richter@tamu.edu


[Full text] (PDF 996 KB)