“…Olivine slip system relative activities have thus been extensively studied, although mostly at relatively low hydrostatic pressure (P < 3 GPa) because of experimental limitations (Raleigh, 1968;Carter and Avé Lallemant, 1970;Phakey et al 1972;Kohlstedt and Goetze, 1974;Poirier, 1975;Kohlstedt et al, 1976Kohlstedt et al, , 1980Durham et al, , 1979Gueguen, 1979;Jaoul et al, 1979;Darot and Gueguen, 1981;Gueguen and Darot, 1982;Mackwell and Kohlstedt, 1985;Ricoult and Kohlstedt, 1985;Bai et al, 1991;Kohlstedt, 1992a, 1992b;Jin et al, 1994). At P < 3 GPa, mantle temperature (T > 1173 K), moderate differential stress and in dry condition, olivine [100] (010) Yet, recent deformation experiments carried out at high pressure on forsterite (Fo100) crystals (Couvy et al, 2004;Raterron et al, 2007), as well as theoretical studies based on first-principle calculations (Durinck et al, 2005;Durinck et al, 2007), show that olivine c-slip may dominate deformation in the P and T ranges of the deep upper A c c e p t e d M a n u s c r i p t 3 mantle. This may promote a shear-parallel slow-velocity [001] axis, which could explain the seismic-velocity attenuation with depth (Mainprice et al, 2005) observed in the upper mantle.…”