Tephra characterization andmulti-disciplinary determination of Eruptive Source Parameters of a weak paroxysm at Mount Etna (Italy)

被引:8
|
作者
Freret-Lorgeril, Valentin [1 ]
Bonadonna, Costanza [1 ]
Corradini, Stefano [2 ]
Guerrieri, Lorenzo [2 ]
Lemus, Jonathan [1 ]
Donnadieu, Franck [3 ]
Scollo, Simona [4 ]
Gurioli, Lucia [3 ]
Rossi, Eduardo [1 ]
机构
[1] Univ Geneva, Dept Earth Sci, 13 Rue Maraichers, CH-1205 Geneva, Switzerland
[2] Ist Nazl Geofis & Vulcanol INGV, Ctr Nazl Terremoti CNT, I-00143 Rome, Italy
[3] Univ Clermont Auvergne, Lab Magmas & Volcans, OPGC, CNRS,IRD, F-63000 Clermont Ferrand, France
[4] Ist Nazl Geofis & Vulcanol, Osservatorio Etneo, Sez Catania, Catania, Italy
基金
欧盟地平线“2020”;
关键词
Volcanic ash; Total erupted mass; Total Grain-Size Distribution; Tephra deposit; Satellite retrievals; GRAIN-SIZE DISTRIBUTION; EXPLOSIVE VOLCANIC-ERUPTIONS; PHYSICAL-CHARACTERIZATION; ASH CONTENT; MT ETNA; RETRIEVAL; DISPERSAL; SATELLITE; EVOLUTION; VOLUME;
D O I
10.1016/j.jvolgeores.2021.107431
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The determination of Eruptive Source Parameters (ESPs) is a major challenge especially for weak volcanic explosions associated with poorly exposed tephra-fallout deposits. In such a case, the combination of deposit analyses and remote sensing observations can provide fundamental insights. We use the 29 August 2011 weak paroxysm at Mount Etna (Italy) as a case study to discuss some of the challenges associated with multi-disciplinary determination of ESPs of poorly exposed tephra-fallout deposits. First, we have determined the erupted mass from a combination of field and synthetic data to fill a significant gap in data sampling; synthetic data have been derived based on extrapolation of field observations and validated based on comparisons with other tephra deposits at Etna and TEPHRA2 modelling. Second, we have combined the estimates of erupted mass and grain-size distribution as derived both from deposit observations and satellite retrievals. Analytical modelling was applied to characterize the size fractions most likely represented in satellite retrievals and tephra deposits, respectively. In addition, the Rosin-Rammler distribution fitting is shown to inform on missing parts of the grain-size distributions and reproduce a tail of very fine ash (1-20 mu m) whose mass proportion is close to the satellite estimates (1.3-1.6% versus 1.9%, respectively). Finally, it was found that this very-fine-ash fraction increases as a function of satellite-derived Mass Eruption Rate for a set of eruptions for which independent estimates are available. This critical combination of field observations, analytical modelling and satellite retrievals demonstrates the potential and importance of multidisciplinary strategies for the derivation of ESPs even for small-size explosive events and poorly exposed deposits such as that of the 29 August 2011 paroxysm of Mt. Etna. (C) 2021 The Authors. Published by Elsevier B.V.
引用
收藏
页数:16
相关论文
共 4 条
  • [1] Examples of Multi-Sensor Determination of Eruptive Source Parameters of Explosive Events at Mount Etna
    Freret-Lorgeril, Valentin
    Bonadonna, Costanza
    Corradini, Stefano
    Donnadieu, Franck
    Guerrieri, Lorenzo
    Lacanna, Giorgio
    Marzano, Frank Silvio
    Mereu, Luigi
    Merucci, Luca
    Ripepe, Maurizio
    Scollo, Simona
    Stelitano, Dario
    [J]. REMOTE SENSING, 2021, 13 (11)
  • [2] Reconstructing eruptive source parameters from tephra deposit: a numerical study of medium-sized explosive eruptions at Etna volcano
    Spanu, Antonio
    Vitturi, Mattia de' Michieli
    Barsotti, Sara
    [J]. BULLETIN OF VOLCANOLOGY, 2016, 78 (09)
  • [3] Reconstructing eruptive source parameters from tephra deposit: a numerical study of medium-sized explosive eruptions at Etna volcano
    Antonio Spanu
    Mattia de’ Michieli Vitturi
    Sara Barsotti
    [J]. Bulletin of Volcanology, 2016, 78
  • [4] SOURCE PARAMETERS OF SEISMIC EVENTS AT MOUNT ETNA VOLCANO, ITALY, DURING THE OUTBURST OF THE 1991-1993 ERUPTION
    PATANE, G
    COCO, G
    CORRAO, M
    IMPOSA, S
    MONTALTO, A
    [J]. PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1995, 89 (3-4) : 149 - 162