We review pre-eruptive dynamics and evidence of open-system behavior in the volcanic plumbing system beneath Campi Flegrei Caldera, together with estimates of magma residence time, magma ascent, and mixing-to-eruption timescales. In detail, we compile pre- and syn-eruptive dynamics reported in the literature for (a) the Campanian Ignimbrite ~ 40 ka, (b) the Neapolitan Yellow Tuff (~ 15 ka), and (c) the recent activity within the Phlegrean area. We first summarize geochemical and textural evidence (e.g., magma mixing, crystal disequilibria, vertical zonings, and isotopic records) of open-system behavior for the pyroclasts erupted in the last 40 ky at Campi Flegrei Caldera. We show that the fingerprint of open-system dynamics is ubiquitous in the deposits associated with the volcanic activity at the Campi Flegrei Caldera in the last 40 ky. Then, we describe the results of geophysical and petrological investigations that allow us to hypothesize the structure of the magma feeding system. We point to a trans-crustal magmatic feeding system characterized by a main storage reservoir hosted at ~ 9 km that feeds and interacts with shallow reservoirs, mainly placed at 2–4 km. Finally, we define a scenario depicting pre-eruptive dynamics of a possible future eruption and provide new constraints on timescales of magma ascent with a physical model based on magma-driven ascending dyke theory. Results show that considerably fast ascent velocities (i.e., of the order of m/s) can be easily achieved for eruptions fed by both shallow (i.e., 3–4 km) and deep (i.e., ~ 9 km) reservoirs. Comparing the results from experimental and numerical methods, it emerges that mixing-to-eruption timescales occurring at shallow reservoirs could be on the order of minutes to hours. Finally, we highlight the volcanological implications of our timescale estimates for magma ascent and mixing to eruption. In particular, explosive eruptions could begin with little physical ‘warning’, of the order of days to months. In this case, the onset of volatile saturation might provide pre-eruptive indicators. Graphical Abstract
<p>The climate-controlled variations of the glacio-lithostatic load in glaciated terrains can potentially affect the tempo of volcanic eruptions, by modifying the pressure conditions acting on the underlying plumbing system. During glacial periods, increasing ice load hinders magma eruption, thus leading to prolonged residence time in the crust. This allows the magma to crystallise, differentiate and accumulate volatiles over a longer time span with respect to non-glacial periods.</p> <p>In Antarctica, volcanism in glaciated regions has been acting since the Miocene. In detail, in northern Victoria Land, volcanoes are located either in attenuated or thick cratonic lithosphere. Among the volcanic edifices built on thick crust, the quaternary Pleiades Volcanic Complex (PVC) is made up of some 20 monogenetic, partly overlapping scoria and spatter cones, that erupted over the last 900 ka. The erupted products range in composition from hawaiite to trachyte, defining a complete mildly Na-alkaline differentiation trend, which is quite unusual among alkaline monogenetic volcanic fields.</p> <p>Six samples from the PVC, representative of the whole differentiation trend, have been investigated by means of electron microscopy, electron microprobe and laser ablation ICP-MS. The parageneses of the rocks includes dominant feldspar and clinopyroxene with minor olivine. The mafic phenocrysts are characterised by significant resorption textures: specifically, the olivine presents deep embayments with absence of compositional zoning, while clinopyroxene frequently shows spongy texture and compositionally zoned mantle and rims, often with patchy and convoluted patterns.</p> <p>Petrography, textures and mineral chemistry suggest that the magma experienced first a rapid decompression, followed by a prolonged residence time, likely supported by increased ice load. During this time interval, resorption of the early formed mineral phases occurred, probably also enhanced by crustal assimilation processes, coupled with re-crystallization under isobaric conditions. Moreover, the prolonged residence time, coupled with the occurrence of (multiple) magma recharge(s) caused the mixing of a basaltic magma with other differentiated magmas stalling in the plumbing system, yielding to the formation of intermediate magma compositions. Finally, magma refilling of the plumbing system during an ice loss period, favoured the eruption. Machine-learning based thermo-barometric estimates consistently indicate crystallization of clinopyroxene at transcrustal pressures, ranging from the crust-mantle interface (early crystallization) to shallow crust (late crystallization in a shallow plumbing system under glacial load).</p>
<p>The Colli Albani volcano is an ultrapotassic caldera complex located 30 km to the SE of Rome and has displayed a wide range of eruptive behaviors, ranging from effusive activity to highly explosive and large volume eruptions (up to 63 km<sup>3</sup> dense rock equivalent per eruption) despite its mafic nature.</p><p>We combine physical volcanology, petrology, and geochemistry to focus on the mildly explosive to effusive products of two sections (Tuscolo and Artemisio) which are located on opposite sides of the main caldera and stratigraphically between the last large ignimbrite, Villa Senni. The target of this study is to identify the processes responsible for the transition from the smaller explosions to the larger caldera-forming ignimbrite eruptions, and eventually trace how the magmatic system rebuilds in the interim.</p><p>Whole rock analyses, mineral chemistry, and petrography of fall deposits from both field localities are compared with an existing dataset for the Villa Senni ignimbrites. We will use unsupervised and supervised machine learning approaches to identify similarities and differences between large caldera-forming eruptions and mild-explosive to effusive activity and identify the processes modulating the transition between these two behaviours.</p>
We review the evidence of open-system behavior in the volcanic plumbing system of the Campi Flegrei Caldera. Also, we highlight the estimates of magma residence time, magma ascent, and mixing-to-eruption timescales. In detail, we concentrate on the Campanian Ignimbrite ~ 40ka, the Neapolitan Yellow Tuff (~ 15ka), and the recent activity within the Phlegrean area. We start highlighting the evidence of magma mixing on the pyroclastic rocks deriving from different sources (e.g., crystal disequilibria, vertical zonings, and isotopic records). Then we describe geophysical and geochemical data of the magma feeding system with a focus on magma residence times and mixing to eruption timescales. Also, we link the timescales of magma ascent reported in the literature with a physically constrained model based on the magma-driven ascending dyke theory. Results show that considerably fast ascent velocities (i.e., units to tens m/s) can be easily achieved for eruptions fed by both shallow (i.e., 3–4 km) and deep (i.e., ~ 9 Km) reservoirs when characterized by large enough overpressures (i.e., > 25 MPa). Finally, we highlight the volcanological implications of timescale estimates for residence time and ascent in both open- and closed-system behavior of the volcanic plumbing system. The main aim is to provide constraints to the volcanic hazard definition of the area.
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