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130 A. Pittari et al.
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