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    The plagioclase as archive of ascent dynamics: the 2001-2006 eruptive period at Mount Etna

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    Several studies are focused on textural and compositional features of plagioclase as an usefull tool to investigate magma chamber processes, ascent dynamics, and physico-chemical conditions. In particular water content, which plays a fundamental role in volcanic process, strongly affects plagioclase stability and, by conseguence, textural and compositional features. However, such reconstruction are usually biased by too many assumptions; particularly when dealing with past eruptions or remote volcanoes. Only few volcanoes provide an array of instrumental monitoring to constrain timing and modality of eruptive events. In this respect Mount Etna probably represents one of the most controlled volcano in the world and a great wealth of seismological and ground deformations data are available. In this work we present a textural and compositional study of plagioclases from lavas emitted during the 2001-2006 eruptive period on Mount Etna. Textural classification has been done on over 130 thin sections taking into account different portion of the crystals. This allow to recognize different types of core (ehuedral and rounded) and rims (dusty or with melt inclusion alignment) separated by oscillatory zoned overgrowth. Oxygen fugacity in magmas has been calculated using the method of [1] and results has been used to reequilibrate the melts to mantle equilibrium, adding back the appropriate quantity of fractionated material. Water content of the melt has been estimated using the hygrometer of [2]. These data were used in the MELT model to estimate the plagioclase stability field and to calculate theoretic composition at different water content. Results were integrated with monitoring data acquired during the entire period under study with the aim to reconstruct magma ascent and storage conditions, as well as the mechanism of eruption triggering. Results indicate the 2001-2006 eruptive period involved magmas with quite similar major element composition but different dissolved H2O. Complex zoning such as dusty areas and alignments of melt inclusions in outer portion of the phenocrysts suggest two different trigger mechanism respectively: i) magma input and mixing with a more basic and volatile-rich magma; ii) fracture migration that induce decompression of shallow magma batches

    Magma mixing during the 2001 event at Mount Etna (Italy): Effects on the eruptive dynamics.

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    During the 2001 eruptive episode three different magmas were erupted on the southern flank of Mount Etna volcano from distinct vent systems. Major and minor element chemistry of rocks and minerals shows that mixing occurred, and that the mixed magma was erupted during the last eruptive phases. The space–time integrated analysis of the eruption, supported by geophysical data, together with major and trace element bulk chemistry (XRF, ICP-MS) and major and trace mineral chemistry (EPMA, LAM ICP-MS), support the following model: 1) trachybasaltic magma rises through a NNW–SSE trending structure, connected to the main open conduit system; 2) ascent of an amphibole-bearing trachybasaltic magma from a 6 km deep eccentric reservoir through newly open N–S trending fractures; 3) just a few days following the eruption onset the two tectonic systems intersect at the Laghetto area; 4) at the Laghetto vent a mixed magma is erupted. Mixing occurred between the amphibole-bearing trachybasaltic magma and an inferred deep more basic end-member. The most relevant aspect in the eruptive dynamics is that the eruption of the mixed magma at the Laghetto vent was highly explosive due to volatile content in the magma. The gas phase formed, mainly because of the decreased volatile solubility due to rapid fractures opening and increased T, related to mixing, and partially because of the amphibole breakdown. D 2005 Elsevier B.V. All rights reserved

    The contemporaneous emission of low-K and high-K trachybasalts and the role of the NE rift during the 2002 eruptive event (Etna, Sicily)

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    Mount Etna volcano erupted almost simultaneously on its northeastern and southern flanks between October 27 and November 3, 2002. The eruption on the northeastern flank lasted for 8 days, while on the southern flank it continued for 3 months. The northeastern flank eruption was characterized by the opening of a long eruptive fracture system between 2,900 and 1,900 m.a.s.l. A detailed survey indicates that the fractures’ direction shifted during the opening from N10W (at the NE Crater, 2,900 m) to N45E (at its lowest portion, 1,900 m) and that distinct magma groups were erupted at distinct fracture segments. Based on their petrological features, three distinct groups of rocks have been identified. The first group, high-potassium porphyritic (HKP), is made up of porphyritic lavas with a Porphyritic Index (P.I.) of 20–32 and K2O content higher than 2 wt%. The second group is represented by lavas and tephra with low modal phenocryst abundance (P.I.<20) named here oligo-phyric (low-phyric), and K2O content higher than 2 wt% (HKO, high-potassium oligophyric). The third group, low-potassium oligophyric (LKO), consists of tephra with oligophyric texture (P.I.<20) but K2O content < 2 wt%. K-rich magmas (HKP and HKO) are similar to the magma erupted on the southern flank, and geochemical variations within these groups can be accounted for by a variable degree of fractionation from a single parent magma. The K-poor magma (LKO), erupted only in the upper segment of the fracture, cannot be placed on the same liquid line of descent of the HK groups, and it is similar to the magmas that fed the activity of Etna volcano prior to the eruption of 1971. This is the first time since then that a magma of this composition has been documented at Mt. Etna, thus providing a strong indication for the existence of distinct batches of magma whose rise and differentiation are independent from the main conduit system. The evolution of this eruption provides evidence that the NE Rift plays a very active role in the activity of Mt. Etna volcano, and that its extensional tectonics allows the intrusion and residence of magma bodies at various depths, which can therefore differentiate independently from the main open conduit system
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