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  • 2020-2024  (8)
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  • 1
  • 2
    Publication Date: 2023-02-01
    Description: Low-intensity emission of volcanic ash represents the most frequent eruptive activity worldwide, spanning the whole range of magma compositions, from basalts to rhyolites. The associated ash component is typically characterized by heterogeneous texture and chemical composition, leading to misinterpretation of the role of syn-eruptive processes, such as cooling and degassing during magma ascent or even magma fragmentation. Despite their low intensity, the ash emission eruptions can be continuous for enough time to create problems to health and life networks of the communities all around the volcano. The lack of geophysical and/or geochemical precursor signals makes the petrological monitoring of the emitted ash the only instrument we have to understand the leading mechanisms and their evolution. Formation of low-level plumes related to ash-rich emissions has increasingly become a common eruptive scenario at Mt. Etna (Italy). In January–February 2019, an eruptive cycle of ash-rich emissions started. The onset of this activity was preceded on 24 December 2018 by a powerful Strombolian-like eruption from a fissure opened at the base of the New Southeast Crater. A lava flow from the same fissure and an ash-rich plume, 8–9 km high a.s.l., from the crater Bocca Nuova occurred concurrently. After about 4 weeks of intra-crater strombolian-like activity and strong vent degassing at summit craters, starting from 23 January 2019, at least four episodes of ash rich emissions were recorded, mainly issued from the Northeast Crater. The episodes were spaced in time every 4–13 days, each lasting about 3–4 days, with the most intense phases of few hours. They formed weak plumes, up to 1 km high above the crater, that were rapidly dispersed toward different directions by dominant winds and recorded up to a distance of 30 km from the vent. By combining observations on the deposits with data on textural and chemical features of the ash components, we were able to discriminate between clasts originated from different crater sources and suggest an interpretive model for syn-eruptive processes and their evolution. Data indicate the occurrence of scarce (〈10 vol.%) fresh juvenile material, including at least four groups of clasts with marked differences in microlite content and number density, and matrix glasses and minerals Moreover, a large amount of non-juvenile clasts has been recognized, particularly abundant at the beginning of each episode. We propose that the low amount of juvenile ash results from episodic fast ascent of small magma batches from shallow reservoirs, traveling within a slow rising magma column subjected to cooling, degassing, and crystallization. The large number of non-juvenile clasts deriving from the thick crater infill of variably sealed or thermally altered material at the top of the magma column is suggested to contribute to the ash generation. The presence of a massive, granular crater infilling accumulating in the vent area may contribute to buffer the different geophysical signals associated with the active magma fragmentation process during the low-energy ash eruptions, as already evidenced at other volcanoes.
    Description: Published
    Description: 824872
    Description: 5V. Processi eruttivi e post-eruttivi
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 3
    Publication Date: 2023-02-01
    Description: We report on the ash cloud related to the gravitational collapse of a portion of the Stromboli volcano crater rim that occurred on 19 May 2021. The collapse produced a pyroclastic density current (PDC) that spread along the northwest flank of the volcano and propagated in the sea for about 1 km. The PDC was associated with a convective ash cloud that rapidly dispersed eastward and deposited a thin layer (〈 1 mm) of very fine pinkish ash over the village of Stromboli. The deposit was sampled shortly after the emplacement (within a few hours) and prior to any significant reworking or re-sedimentation. We present a comprehensive description of the deposit including dispersal, sedimentological characteristics and textural and geochemical features. We also compare the 19 May 2021 deposit with fine-ash deposits connected to other PDCs and landslides previously occurring at Stromboli and with the distal ash of a paroxysmal explosive eruption of Mt. Etna volcano. Results indicate that the distributions of the mass on the ground and of the grain size are not correlated with the distance from the source. Also, the componentry reflects a preponderance of remobilized material ingested by the PDC. Therefore, the great amount of fine ash can be ascribed to clasts comminution processes, although the prevalence of dense crystalline components records an overall equiaxial shape, revealing a paucity of elongated clast with complex morphology. Furthermore, the outcomes of this work aim to create a collection of data of a co-PDC ash cloud that may prove useful for comparison with other deposits worldwide.
    Description: Published
    Description: 10777
    Description: 5V. Processi eruttivi e post-eruttivi
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2023-03-14
    Description: New textural and petrological data are presented on products from five paroxysms at Stromboli (Aeolian Islands, Italy) including the two from 2019 and three historical (1930, undated, sixteenth century) eruptions. The data are used to con- strain timescales associated with the initiation of paroxysms and to examine current models for their triggering. Samples were collected from the deposits and a subset selected for mineral separation and petrological and textural characterization. Minerals and glass were imaged by scanning electron microscopy (SEM), and chemical composition and zonation were analysed by electron microprobe. Trace elements in olivine were also determined. Vesicle number densities, vesicularities and vesicle diameters were measured by X-ray microCT techniques. The data were systematically compared with results of experiments simulating, on the one hand, ascent, vesiculation, degassing and crystallization of LP (low-porphyricity) magma and, on the other hand, interaction between LP and HP (high-porphyricity) magma. Paroxysm samples are mixed and include portions representative of both LP and HP magma. They host in variable proportions minerals and glass textur- ally and compositionally typical of these two magma types. Small but systematic variations in matrix glass compositions are found between each of the five eruptions considered. All samples host a population of vesicles ranging from 〈 15 to 〉 1000 μm in diameter and whose size distributions follow mixed exponential to power law distributions. Vesicularities are high (75% on average) and vesicle number densities range from 102-103 to 103-104 mm-3. Using experimental calibrations, the vesicle textural data suggest average LP magma ascent rates of 1–2 m/s (i.e. ~1.5 hours from depths between 7 and 1.5 km). The correlation between ascent rate and textures demonstrates systematic variations between eruptions, the most ener- getic (i.e. that of 1930) being associated with the highest ascent rate (~2 m/s). Widths of plagioclase reaction zones indicate that LP and HP magmas interacted for a maximum a few hours before eruption. Olivine reaction also implies durations of a few hours for LP-HP interaction and is followed by crystallization for 20 hours in the HP magma. Our results stress the fast ascent of LP magma from their storage region and their short residence times at shallow levels before being erupted. They clarify the respective roles of the deep and shallow feeding systems. An integrated phenomenological model for paroxysm initiation at Stromboli is outlined. Keywords
    Description: This study was supported by the Labex Vol- taire (ANR-10-LABX-100-01), by INGV Progetti Ricerca Libera (timescale of magma transfer within the Stromboli plumbing sys- tem) and by the “DisEqm” (quantifying disequilibrium processes in basaltic volcanism) and “Shedding new light on volcanoes: real-time synchrotron X-ray tomography of magmatic phenomena” projects funded by NERC (NE/N018575/1 and NE/M013561/1).
    Description: Published
    Description: 36
    Description: 1V. Storia eruttiva
    Description: 2V. Struttura e sistema di alimentazione dei vulcani
    Description: 3V. Proprietà chimico-fisiche dei magmi e dei prodotti vulcanici
    Description: 5V. Processi eruttivi e post-eruttivi
    Description: JCR Journal
    Keywords: Stromboli ; Paroxysms ; 04.08. Volcanology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 5
    Publication Date: 2023-01-27
    Description: The remobilization and avalanching of fresh pyroclastic deposits are relatively common at Stromboli. They are usually confined to the Sciara del Fuoco (SdF), a steep depression on the northwestern side of the island. However, at least during the Strombolian paroxysms in 1944, 1930, and possibly in 1906, pyroclastic avalanches occurred out of SdF, flowed in the valleys on the volcano flanks, inundated regions at low elevation, and, finally, they reached the sea and produced vaste temporary deltas. In particular, in the 1930 event, the pyroclastic avalanche reached San Vincenzo village, causing victims and damage to the buildings. In this study we perform an uncertainty quantification on the inputs of the 2D depth-averaged model, preliminary to a comparison with the available field data. In particular, because the source location of the flow is also assumed uncertain, we adopt a simplified source zonation based on the analysis of topographic slopes, distance from the eruptive craters, and watersheds basins in the upper part of the island, where thick tephra deposits could more likely accumulate during a future paroxysm.
    Description: Published
    Description: St. Pierre (Martinique) and Tampa (USA), virtual
    Description: 6V. Pericolosità vulcanica e contributi alla stima del rischio
    Keywords: pyroclastic flows ; Stromboli
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Conference paper
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  • 6
    Publication Date: 2024-04-17
    Description: Over the past decades, significant efforts have been made to understand the nature, dynamics and evolution of volcanic systems. In parallel, the continuous demographic expansion and extensive urbanization of volcanic areas have increased the exposure of our society to these natural phenomena. This increases the need to improve our capacities to accurately assess projected volcanic hazards and their potential socioeconomic and environmental impact, and Antarctica and the sub-Antarctic islands are no exception. More than a hundred volcanoes have been identified in Antarctica, some of which are entirely buried beneath the ice sheet and others as submarine volcanoes. Of these, at least eight large (basal diameters 〉 c. 20-30 km) volcanoes are known to be active and pose a considerable threat to scientific and ever-increasing tourism activities being carried out in the region. Despite the scientific and socioeconomic interest, many aspects of the past volcanic activity and magmatic processes in Antarctica, and current volcanic hazards and risks, remain unknown. Moreover, many of Antarctica’s volcanoes preserve a remarkable history of the eruptive environment, from which multiple parameters of past configurations of the Antarctic ice sheet (AIS) can be deduced. Given the critical role that the AIS plays in regulating Earth’s climate, Antarctica’s volcanoes therefore can be regarded as the ground truth for current models of past climates derived from modelling and studies of marine sediments. Here, we provide a succinct overview of the evolution of volcanism and magmatism in Antarctica and the sub-Antarctic region over the past 200 million years. Then, we briefly review the current state of knowledge of the most crucial aspects regarding Antarctica’s volcanic and magmatic processes, and the contributions volcanic studies have made to our understanding of ice sheet history and evolution, geothermal heat flow, as well as present-day and future volcanic hazard and risk. A principal objective is to highlight the problems and critical limitations of the current state of knowledge and to provide suggestions for future potential directions of volcanic-driven investigations in Antarctica. Finally, we also discuss and assess the importance and scope of education and outreach activities specifically relating to Antarctic volcanism, and within the context of broader polar sciences.
    Description: Published
    Description: 107941
    Description: OSV2: Complessità dei processi vulcanici: approcci multidisciplinari e multiparametrici
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 7
    Publication Date: 2024-03-13
    Description: The catalog consists of the dataset of the major explosions and paroxysms recorded at Stromboli from Jan. 1970 to Oct. 2023, as reconstructed through a detailed review of monitoring bulletins and reports, previous catalogs, and scientific literature of the last ca. 50 years. The catalog includes the calendar date, GMT time and phenomena descriptions for 89 explosive events, of which 4 were paroxysms, 51 were major explosions, and 34 were uncertain major explosions, i.e. explosions of unclear characterization that could have been major explosions or ordinary activity. We detailed the event information content in five columns – (i) seismicity, (ii) sound/air shock, (iii) vents involved, (iv) ash plume/fallout, (v) ballistic projectiles. In addition, we indicated if there were any: (vi) field survey, (vii) pumices erupted, (viii) fires, (ix) map of the products, (x) photo/video of the event, (xi) hot avalanche, (xii) lava flow. The catalog also includes a list of the original literature sources that helped us in the complex characterization of the explosive events. We finally reported if there were people affected by the events, and any previous catalog that comprised them. In our analysis (see also Bevilacqua et al., 2020b), we mostly relied on the detailed characterization of major explosions and paroxysms in Rosi et al. 2013 that provided quantitative constraints on total duration, fallout volume, mass discharge rate, ballistic size, ballistic range and column height of ordinary activity, major explosions, and paroxysms. In several cases, we had to carefully evaluate the original description of the phenomena, due to insufficient quantitative information in the scientific literature. In particular, we considered the hazardous area affected by large ballistic projectiles as the main discriminant factor to distinguish between ordinary activity, major explosions and paroxysms. This area is limited to the Crater Terrace and upper Sciara del Fuoco in case of ordinary activity, to the summit area of the volcano and Sciara del Fuoco during major explosions, and can extend down to low elevations along large part of the island, and sometimes beyond the shoreline, during the paroxysms (Barberi et al., 1993). We also considered several other factors, including the height of the plume, the amount of ash and scoria fallout, the occurrence and strength of any associated shock wave. The occurrence of fires associated with the violent explosive activity was assumed as a good marker for a major explosion too (Rosi et al., 2013). Whilst identifying the paroxysms was relatively straightforward, several possible major explosions were not clearly distinguishable from particularly violent episodes of ordinary Strombolian activity. Thus, our historical record includes the quantification of the main sources of uncertainty, i.e. the possibility of 34 major explosions of uncertain characterization because of insufficient information. We followed a conservative approach and we classified as “uncertain major explosions” all the explosive events for which we could not exclude they were major explosions. This particular case often occurs in the 1970s, 1980s and 1990s, before the installation of surveillance cameras, and, afterwards, when these cameras were not operating for bad weather conditions or temporary malfunctions. In addition, the catalog includes 41 seismic sequences typically associated with higher-than-usual explosive activity but with a size significantly smaller than that of major explosions. These events may have produced a limited ballistic fallout just outside of the crater terrace, i.e. few tens of meters, or short lived effusive activity (e.g. intra-crateric), but they are not associated with the dangerous ballistic fallout of major explosions. About these seismic sequences, we relied on the characterization in Falsaperla & Spampinato, 2003, that is a variable number of explosion quakes in rapid succession (i.e. from tens of seconds to a few minutes), associated with a notable increment in the amplitude of volcanic tremor. This definition relies on the availability of seismic registrations, and therefore a significant under-recording may affect the period before June, 1985, when seismic records started to be acquired continuously at Stromboli. Afterwards, short lapses in the available registrations possibly generated slight underrecording of the seismic sequences in the 1990s and 2000s. Since 2003/2004 the improvement in the seismic network significantly reduced the possible underrecording of seismic sequences. The catalog is accompanied by four supporting files. Supporting Material S1 is a table summary of all the events in the catalog, including a synoptic panel comparing the new catalog to the pre-existing catalogs. Supporting Material S2 is the collection of excerpts from the source documents, including the original figures and descriptions. Supporting Material S3 is the bibliography; a digital version of the literature sources referenced is available from the corresponding author. Supporting Material S4 is an addendum catalog that comprises the descriptions of a number of supplementary explosive events reported as anomalous in literature or monitoring files for various reasons, but not classified by us as paroxysms, major explosions, uncertain major explosions, or seismic sequences. This catalog is complementary to the historical catalog Bevilacqua et al. (2020a), which comprises the years from 1879 to 1960. In the time interval between 1960 and 1970 no major explosions or paroxysms were recorded; however, some under-recording of major explosions might affect that decade. The modeling and estimation of inter-event time and temporal rate of major explosions and paroxysms at Stromboli volcano is detailed in Bevilacqua et al. (2020b) based on the data available at that time. Finally, it is worth mentioning that the present catalog is based on the above reported criteria to characterize the ordinary activity, major explosions and paroxysms which are mostly oriented to the assessment of the hazard associated with the explosive activity of Stromboli. It should also be recognized that a well-defined boundary between these categories may not exist. The catalog is open and dynamic and welcomes contributions from other sources and new information in order to make it more complete and robust.
    Description: Dipartimento della Protezione Civile, Italia
    Description: Published
    Description: OSV1: Verso la previsione dei fenomeni vulcanici pericolosi
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: report
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  • 8
    Publication Date: 2024-05-03
    Description: Although many studies have demonstrated that arc magmas are more oxidized than mid-ocean ridge (MORB) and oceanic island basalts (OIB), the oxidation state of their mantle source is still debated. This ongoing debate is mainly due to contradictory fO2 values obtained from different proxies (e.g., Fe3+/ΣFe of olivine-hosted melt inclusions and glasses; Zn/ΣFe, V/Sc, V/Ga of lavas). On the one hand, some studies using V/Sc, V/Ga and Zn/ ΣFe of lavas tend to show that the oxidation state of the mantle beneath arcs cannot be distinguished from that of the MORB mantle. On the other, Fe3+/ΣFe of glasses and olivine-hosted melt inclusions suggest that the sub-arc mantle is more oxidized than the mantle beneath ridges. Here, we estimate the oxygen fugacity of high-Mg olivine-hosted melt inclusions from various mid-ocean ridges and arcs, from one hot spot (Reunion Island) and Mount Etna using two fO2 proxies: the Fe3+/ΣFe of melts and the partition coefficient of V between olivine and melt (Dv Ol/Melt). After assessing the role of secondary processes such as volatile degassing and fractional crystallization on the fO2 of melts and reconstructing primary melt compositions, we show that (1) fO2 values derived from Fe3+/ΣFe and Dv Ol/Melt are comparable and (2) arc and Mount Etna primary melts are more oxidized than mid-ocean ridge and Reunion Island primary melts. We then demonstrate, from Zr/Nb, that the observed variability in primary melt fO2 is not due to chemical variability of the mantle source. Finally, the correlations between incompatible trace element ratios such as Th/La, Ba/La, Ba/Th and La/Yb and the fO2 of primary melts reveal a link between the oxidized nature of arc and Mount Etna primary magmas to slab fluid and/or sediment melt influence. Our arc dataset displays a variety of subduction influences, from fluid-dominated (Aoba and Mount Meager) to sediment melt-dominated (La Sommata) influences. The origin of the oxidation of Mount Etna magmas is more complicated to identify and the nature of the oxidized metasomatic fluids that likely percolated through the mantle source before magma generation is yet to be determined. 1.
    Description: Published
    Description: 121701
    Description: OSV2: Complessità dei processi vulcanici: approcci multidisciplinari e multiparametrici
    Description: JCR Journal
    Keywords: 04.08. Volcanology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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