Bulk and step-heating hydrogen isotope measurements of glassy and vesicular
samples from three young rhyolite lavas demonstrate for the first time tha
t magmatic H2O can be distinguished from meteoric H2O added during rehydrat
ion. Step-heat extractions of gases obtained at five temperatures show that
most meteoric H2O is released at around 400 degreesC, while magmatic H2O c
omes off during the fusion step at 1100-1200 degreesC. Magmatic H2O content
s from vertically-arrayed lava samples show a downward increase consistent
with the equilibrium pressure-dependence of H2O solubility. These gradients
imply that volatile concentrations high enough to generate pyroclastic flo
ws during front collapse may be found in the upper portions of silicic dome
s produced by relatively high eruption rates. (C) 2001 Elsevier Science B.V
. All rights reserved.