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Figure F23. Magnetic susceptibility (top) and relative paleointensity (bottom) plotted against depth (mbsf), Hole U1344A. Relative paleointensity is estimated by normalizing natural remanent magnetization after 20 mT demagnetization (Int_{20 mT}) by magnetic susceptibility. Marine isotope Stages (MIS) 1–19 in the Brunhes Chron, numbered at top, were tentatively identified by correlating these features to other sites.

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