Figure F66. Zr vs. TiO2 showing that the basalt units from Hole 1183A have broadly similar abundances of incompatible elements to Units C-G at Site 807 (Mahoney et al., 1993) and to the basalt flows of the Kwaimbaita Formation on Malaita (Tejada et al., in press).

Figure F66. Zr vs. TiO₂ showing that the basalt units from Hole 1183A have broadly similar abundances of incompatible elements to Units C-G at Site 807 (Mahoney et al., 1993) and to the basalt flows of the Kwaimbaita Formation on Malaita (Tejada et al., in press).