2015
DOI: 10.1016/j.epsl.2014.12.038
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Open-path FTIR spectroscopy of magma degassing processes during eight lava fountains on Mount Etna

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Cited by 42 publications
(45 citation statements)
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“…As already observed by La Spina et al . [] and based on this evidence, we suggest that the longer the interevent time, and thus the time needed for the NSEC feeding system to reach the threshold pressure to trigger the subsequent lava fountain, the greater the energy accumulated and then released. Figure details the relation between interevent time (i.e., interevent time between the start of a fountain episode and the start of the previous one) and time of occurrence.…”
Section: Data Interpretation and Discussionmentioning
confidence: 79%
See 1 more Smart Citation
“…As already observed by La Spina et al . [] and based on this evidence, we suggest that the longer the interevent time, and thus the time needed for the NSEC feeding system to reach the threshold pressure to trigger the subsequent lava fountain, the greater the energy accumulated and then released. Figure details the relation between interevent time (i.e., interevent time between the start of a fountain episode and the start of the previous one) and time of occurrence.…”
Section: Data Interpretation and Discussionmentioning
confidence: 79%
“…Lava fountains are spectacular manifestations of active volcanism, characterized by incandescent lava jets of heights from tens‐to‐hundreds of meters that can last from minutes to days [e.g., Wilson and Head , ; Oppenheimer and Francis , ; Parfitt , ]. The nature and conditions leading to lava fountains have been widely discussed using methodologies spanning from ground‐based observations to satellite imagery and laboratory experiments [e.g., Jaupart and Vergniolle , ; Alparone et al ., ; Allard et al ., ; Friedman et al ., ; Spampinato et al ., ; Ganci et al ., ; Gouhier et al ., ; La Spina et al ., ]. The rapidity, with which lava fountains develop, and the high energy released have forced the volcanology community to make efforts to better understand this eruptive regime [e.g., Endo et al ., ; Hayashi et al ., ; Mangan and Cashman , ; Parfitt , ; Vergniolle and Ripepe , ; Staudacher et al ., ; Stovall et al ., ; Bonaccorso et al ., ].…”
Section: Introductionmentioning
confidence: 99%
“…This indicates pre-eruptive storage at 40 MPa (~1.5 km of lithostatic pressure). The presence of a significant mass of exsolved volatiles, presumably derived either from volatile exsolution within a deeper part of the volcanic system or by vapor/fluid accumulation via closed system exsolution in crustal chambers, is often proposed to play a significant role in basaltic eruptions (Allard et al, 2005;La Spina et al, 2015;Spilliaert et al, 2006;Vergniolle and Jaupart, 1986). Geochemical evidence for this can theoretically be found in melt inclusions (e.g.…”
Section: Decompression Model Resultsmentioning
confidence: 99%
“…Prior to the development of ultra violet (UV) camera technology [10,11], measurement techniques were constrained by sampling rate and therefore lacked The detection of periodic behavior is not restricted to SO2 flux measurements alone, and periodicity can also be identified in timeseries of molar gas ratios [16,[24][25][26][27]. Open-Path Fourier Transform Infrared Spectroscopy (OP-FTIR) can capture high temporal resolution datasets of molar gas ratios for a broad range of gases, including trace species such as chlorine [28][29][30][31][32]. In combination with thermodynamic models of volatile solubility, molar gas ratios can be directly related to the pressure (depth) of gas-melt separation and are therefore critical to the identification and tracking of new magma inputs and their subsequent ascent through the shallow magmatic system [33][34][35][36] or to discriminate between redox-and solubility-driven processes [24,37].…”
Section: Introductionmentioning
confidence: 99%