Figure F59. Histograms of stable remanent inclinations determined for archive-halves from Hole 1275D, illustrating how different depth intervals preserve distinctly different remanence inclinations. The top 50 m of the hole apparently records a mixture of normally and reversely polarized magnetization. The middle of the hole, from 50 to 140 mbsf, preserves a well-defined shallow negative inclination. Below a relatively sharp break at ~140 mbsf, the lower portion of the hole has a significantly higher negative inclination.