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  5. Lava flow field development and lava tube formation during the 1858–1861 eruption of Vesuvius (Italy), unravelled by historical documentation, lidar data and 3D mapping
 
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Lava flow field development and lava tube formation during the 1858–1861 eruption of Vesuvius (Italy), unravelled by historical documentation, lidar data and 3D mapping

Author(s)
Lemaire, Thomas
Morgavi, Daniele  
Petrosino, Paola  
Calvari, Sonia  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Repola, Leopoldo
Esposito, Lorenzo
Di Martire, Diego  
Morra, Vincenzo  
Frondini, Francesco  
Language
English
Obiettivo Specifico
OSV1: Verso la previsione dei fenomeni vulcanici pericolosi
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Journal of Volcanology and Geothermal Research  
Issue/vol(year)
/455 (2024)
ISSN
0377-0273
Publisher
Elsevier
Pages (printed)
108197
Date Issued
October 1, 2024
DOI
10.1016/j.jvolgeores.2024.108197
Last version
https://doi.org/10.1016/j.jvolgeores.2024.108197
URI
https://www.earth-prints.org/handle/2122/57645
Subjects
04.08. Volcanology  
Lava tubes
Vesuvius effusive activity
Subjects

Vesuvius

Effusive activity

Lava flow fields

Lava tubes

Abstract
Somma-Vesuvius is well known for its powerful Plinian explosive eruptions, however during the last eruptive cycle (1631-1944), persistent activity took place on the stratovolcano as mild and violent Strombolian, and effusive eruptions, forming more than one hundred lava flow fields. An important mechanism of lava transport within lava flow fields is the formation and development of lava tubes. The presence of lava tubes in a flow field can greatly increase their distance of emplacement. Observations of lava tubes
Journal Pre-proof
Journal Pre-proof
at Vesuvius have been documented in historical records and speleological reports but no modern scientific studies are available. This work focuses on lava tubes formed in the compound lava flow field of the long-lived 1858 eruption (from 27 May 1858 to 12 April 1861) that was fed by seven eruptive fissures. The temporal and spatial evolution of the 1858 lava flow field was reconstructed using historical documentation. The exposed lava flow field surface was analysed using a 1-m resolution lidar Digital Surface Model (DSM). Surveys to fully digitize the interior and the overlying surface of the largest lava tube found in the 1858 lava flow field were conducted using a terrestrial laser scanner, optical cameras, and an Unmanned Aerial Vehicle (UAV). The accurate 3D model obtained was used to precisely quantify the inner dimensions and to better constrain the morphologies of the lava tube. Observed internal features were described and used to gain information on the formation and activity of the lava tube. Our data allowed us to understand that the described lava tube formed as an inflated lava flow inside which lava flowed through during an extended period ultimately draining out completely at the end of the eruption. Understanding how lava flow fields develop and how lava tubes form on Vesuvius is crucial to re-evaluate the last effusive activity of the volcano and its impact on hazard assessment.
Sponsors
This research was funded by the project “UndersTanding lava tUBe formation and prEServation (TUBES)” PRIN – Bando 2022 PNRR Prot. P2022N55C3 (P.I. D. Morgavi). This research was also partially funded by the Project FIRST-ForecastIng eRuptive activity at Stromboli volcano: Timing, eruptive style, size, intensity, and duration; INGV-Progetto Strategico Dipartimento Vulcani 2019 (Deliberata n. 144/2020).
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