Figure 10. The VGP path of the B-M reversal was calculated from the characteristic remanent magnetizations at Hole 1014D in the Tanner Basin of the California Borderland. The VGPs do not reach the North and South geographic Poles, probably because of the drilling-induced overprint. Directional data of the ChRMs are plotted in Figure 9.

Figure 10. The VGP path of the B-M reversal was calculated from the characteristic remanent magnetizations at Hole 1014D in the Tanner Basin of the California Borderland. The VGPs do not reach the North and South geographic Poles, probably because of the drilling-induced overprint. Directional data of the ChRMs are plotted in Figure 9.