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          Figure 14  Schematic representation of the substrate geology and the superimposed active
          volcanic system just prior to the climactic destructive Abrigo eruption. Abbreviation: DH,
          Diego Herna Ł ndez.

             Mafic cumulate body(s) have been identified from geophysical studies at depths
          of 5–14 km below central Tenerife (Ablay and Kearey, 2000; Aran ˜a et al., 2000) and
          are probably the source of the very rare syeno-gabbroid and gabbroid lithic clasts
          within the Abrigo ignimbrite. It is likely that syenite was a more dominant wall
          rock lithology. Mafic plutonic lithic clasts within the Abrigo ignimbrite are more
          common on the eastern flanks of the edifice and could be evidence for a higher
          abundance of syeno-gabbro/gabbros at the eastern end of the Abrigo chamber wall.


          3.6.2. Ancient hydrothermal systems
          The abundance of hydrothermally altered lithic clasts within the Abrigo ignimbrite
          (often up to 40%) indicates that a large subsurface region of hydrothermally altered
          rock was sampled during the eruption (Figure 14). Hydrothermal altered rocks are
          locally exposed along the margin of the caldera wall (Aran ˜a, 1971) and may be the
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