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Local equilibrium the reactive magma and experimental studies of silicic systems.

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HAL Id: hal-00080097

https://hal-insu.archives-ouvertes.fr/hal-00080097

Submitted on 14 Jun 2006

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Local equilibrium the reactive magma and experimental

studies of silicic systems.

Michel Pichavant, Fidel Costa Rodriguez, Bruno Scaillet, Caroline Martel,

Stéphane Poussineau

To cite this version:

Michel Pichavant, Fidel Costa Rodriguez, Bruno Scaillet, Caroline Martel, Stéphane Poussineau. Local

equilibrium the reactive magma and experimental studies of silicic systems.. Geophysical Research

Abstracts, 2004, Nice, France. pp.Vol. 6, 04668. �hal-00080097�

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Geophysical Research Abstracts, Vol. 6, 04668, 2004 SRef-ID: 1607-7962/gra/EGU04-A-04668

c

European Geosciences Union 2004

LOCAL EQUILIBRIUM THE REACTIVE MAGMA

AND EXPERIMENTAL STUDIES OF SILICIC

SYSTEMS

M. Pichavant, F. Costa, B. Scaillet, C. Martel, S. Poussineau ISTO, UMR 6113 CNRS, Orléans, France (pichavan@cnrs-orleans.fr)

Experimental phase equilibria are being increasingly used for the determination of pre-eruptive conditions of subvolcanic magma bodies. In comparison with mineral-melt thermobarometry combined with analysis of glass inclusions, the experimental ap-proach offers greater sensitivity and accuracy on key parameters such as melt H$_2$O content and pressure. Yet, numerous petrologic studies of silicic volcanic rocks have documented textural and chemical evidence for disequilibrium. Thus, the applicabil-ity of equilibrium experiments requires clarification especially in the context of open magmatic systems. It must be recognized that, although bulk equilibrium is generally not attained in silicic magmas, a subsystem of the magma which is in local equilib-rium (hereafter designated as the reactive magma) can be typically identified. Reactive magma volumes differ between magmatic systems, yet some generalizations can be made. Reactive magma volumes are much larger in chemically homogeneous than in chemically zoned magma bodies because interstitial melt compositions are homo-geneous in the former and heterohomo-geneous in the latter. They can also vary during the lifetime of the magma: remobilization due to mafic magma recharge generates disequi-librium (ie, reduce the reactive magma volume). Reactive magma volumes appropriate for pre-eruptive magma storage differ from (ie, are generally larger than) those appro-priate for syn-eruptive magma ascent because conduit processes have much shorter timescales than magma storage processes. These considerations stress the need of a careful choice of the starting composition for the experiments. For pre-eruptive con-ditions of equilibration of silicic magmas to be reliably determined experimentally, a starting material closely approaching the composition of the corresponding reac-tive magma must be used. Phase compositions and proportions provide a critical test of the choice of the starting material because both should match simultaneously (for

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given P-T-H$_2$Omelt-fO$_2$) in experimental and natural products if the starting material correctly approximates the reactive magma. Certain discrepancies between experimental phase and phenocryst assemblages in recent studies can be explained by differences between experimental and natural P-T-H$_2$Omelt-fO$_2$ conditions, but others likely result from a poor matching between the starting composition and the appropriate reactive magma. The reactive magma concept is thus a useful theoreti-cal tool for the evaluation of the state of chemitheoreti-cal equilibrium in silicic volcanic rocks and for the planning and interpretation of experimental studies on silicic magmas.

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