Figure F20. Magnetic susceptibility (top) and relative paleointensity (bottom) vs. depth, Hole U1345A. Relative paleointensity was estimated by normalizing remanent magnetization after 20 mT AF demagnetization (Int20 mT) by magnetic susceptibility. MIS 1–12 in the Brunhes Chron, numbered at top, were tentatively identified by correlating these features to other sites.
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