Very fast canyon formation and evolution along active volcanic flanks: A case from Stromboli Island
Journal
GEOMORPHOLOGY
Date Issued
2025-08-07
Author(s)
Petronelli, Denise
Abstract
Active insular volcanoes are generally characterized by their rapid morphological evolution, as a close interplay exists between eruptive activity and erosive-depositional processes in such volcanoes. The Sciara del Fuoco depression, a sector collapse scar on the NW flank of the Stromboli volcano (Italy), is considered a natural laboratory for studying the response of a volcanic slope to such a dynamic evolution. In this study, we report the very fast morphological evolution that affected the subaerial and submarine Sciara del Fuoco slope from May 2022 to May 2023, a period of time marked by the occurrence of two crater rim failures, pyroclastic density currents and multiple lava flows. The analysis of repeated topo-bathymetric surveys demonstrates that a narrow (100 m wide at maximum) and steep-sided canyon, tens of meters deep, formed in the central part of the Sciara del Fuoco. The canyon was mainly related to the erosive activity of the pyroclastic density currents, which led to the remobilization of (at least) 3.7 × 106 m3 volcanic material, mainly in the subaerial slope. The canyon was initially formed by retrogressive erosion upslope, starting from an initial submarine/coastal landslide. It then evolved through a progressive widening of its flanks through small-scale landslides. The study shows that landslide location, as well as the final canyon shape, were strongly controlled by the lithological limits of pre- vious lava flows, highlighting the importance of inherited morpho-stratigraphy and lateral heterogeneities in slope stability. Since its formation, the canyon has acted as a main conduit for lava flows and volcaniclastic materials supplied on their way to the sea. About 1 × 106 m3 of material filled the subaerial canyon floor through time, and another 1 × 106 m3 of slope accretion was estimated for the submarine part of the Sciara del Fuoco, down to 400 m below sea level. Comparing the volumes associated with slope erosion and accretion, it is evident that a large part of the remobilized material bypassed the Sciara del Fuoco shallow-water sector and was emplaced at greater depths. This study highlights the relevance of an integrated system for monitoring the submarine and subaerial morphological evolution of insular volcanic flanks, contributing to an improved geo- hazard assessment during eruptive crises.
Project(s)
The first author thanks also the funding provided by Progetto di Ateneo 2021 and 2022, University Sapienza of Rome, P.I. Daniele Casalbore as well as the RETURN (VS2) Extended Partnership. This research has benefited from the support from the following projects: “Convenzione B2 DPC-INGV 2022-2024, Stromboli”; INGV project Pia- neta Dinamico 2023-2025 - ORME; INGV project Reti Multi- parametriche (Task A2); INGV Progetto Strategico Dipartimentale 2019 “UNO”; INGV Progetto Strategico Dipartimentale 2019 “FIRST” (Delib- era n. 144/2020); Accordo tra Universita` degli Studi di Firenze e Pres- idenza del Consiglio dei Ministri - Dipartimento della Protezione Civile 2022–2024; Accordo tra IREA-CNR e Presidenza del Consiglio dei Ministri - Dipartimento della Protezione Civile 2022–2024; Accordo tra IGAG-CNR e Presidenza del Consiglio dei Ministri - Dipartimento della Protezione Civile 2022–2024. The data used in this study were provided by INGV, UniFI, IGAG-CNR, UniRoma1 “La Sapienza”, and IREA-CNR. We would like to acknowledge also the support of the Presidenza del Consiglio dei Ministri - Dipartimento della Protezione Civile. The con- tents of this paper represent the authors' ideas and do not necessarily correspond to the official opinion and policies of the Presidenza del Consiglio dei Ministri - Dipartimento della Protezione Civile. Partly funded by the European Union – Next Generation EU, National Recovery and Resilience Plan Mission 4 - Component 2. Project title: “Causes and consequences of deposit-derived pyroclastic density currents” (P20222BP7J). We also acknowledge the support of EPOS-RI, including the one obtained through the EPOS-Italia JRU. The SSAP software research and development was funded by CONAHCYT (Mexico): Proyectos Ciencia Basica: CB-2016/286764. SSAP2010 is FREEWARE software, i.e. it is distributed free of charge only at HTTPS://WWW.SSAP.EU. There is only one full version of the SSAP2010 software and it is the free version that can be downloaded from the official website. The SSAP2010 User Licence allows the user unlimited use of the software with the ability to download all future updates from the web. SSAP20010 software is non- commercial software. Its distribution is non-profit (see SSAP User Licence).
