Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2265
Authors: de Lorenzo, S.* 
Di Renzo, V.* 
Civetta, L.* 
D’Antonio, M.* 
Gasparini, P.* 
Title: Thermal model of the Vesuvius magma chamber
Journal: GEOPHYSICAL RESEARCH LETTERS 
Series/Report no.: /33 (2006)
Publisher: AGU
Issue Date: 2006
DOI: 10.1029/2006GL026587
Keywords: NONE
Subject Classification04. Solid Earth::04.01. Earth Interior::04.01.02. Geological and geophysical evidences of deep processes 
04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrology 
04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risk 
Abstract: A thermal modeling of the Vesuvius is presented, based on its magmatic and volcanic history. A 2D numerical scheme has been developed to evaluate the heat transfer inside and around a magma body, the latent heat of crystallization and the inputs of magma from the asthenosphere to a crustal reservoir. Assuming a ratio >1 between velocities of magma ascending in the conduit and magma laterally displaced in the reservoir, the results indicate that, after 40 ka, the reservoir is vertically thermally zoned. As a consequence it hosts magma batches that can individually differentiate, mix and be contaminated by the crust, and produce the spectrum of isotopic compositions of the Vesuvian products. The thermal model reproduces the geothermal gradient and the brittle-ductile transition (250– 300 C) at 6 km of depth (the maximum depth of earthquake foci) only after 0.5–1 Ma, implying a long lived magma chamber below the volcano.
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