“…These fluidal gabbro clasts are hosted in narrow zones of featureless, silicified tuff adjacent to bedded, fine-grained felsic tuffs (Figure 162). These zones probably represent intense fluidization due to heating of interstitial pore fluids (Kokelaar, 1982;Kano, 1989Kano, , 1991McPhie, 1993;Hanson and Hargrove, 1999;Dadd and Van Wagoner, 2002) during the initial injection of hot mafic magma (Figure 169). Subsequent passive mingling was possible due to fluid instabilities (Wohletz, 1983) together with contrasting densities (Kokelaar, 1982;McPhie, 1993;Donaire et al, 2002), whereby oscillations along the magma -host sediment interface may generate globules of fluidal magma (Busby-Spera and White, 1987).…”