“…difference in the compositions of the dunite residues in columns that differ in the amount of melt focusing. Consequently, as discussed by Kelemen et al (1997), it roman peridotite (Takahashi, 1992;Takazawa et al, is difficult to do more than place a lower bound on the 1992), the Trinity peridotite (Quick, 1981; melt flux required to produce a dunite vein; further melt al., 1992), the Josephine peridotite (Dick, 1976(Dick, , 1977 flux beyond this point may leave no detectable trace. Kelemen & Dick, 1995), and the Oman ophiolite [Kelemen et al (1997) and references therein].…”