Temporal models for the occurrence of Etna eruptions and implications for hazard assessment
Abstract. Mt Etna volcanic activity is broadly divided into flank eruptions and summit paroxysms. Here, building on previously-available literature and data on the start time of these events, we collate two separate catalogs of the two activity types. Then we separately model their temporal occurrence. The catalog of flank eruptions, spanning the last 400 years, has been modelled by means of the most widely used renewal models, among which the best one (through Akaike Information Criterion) is the Brownian Passage Time. The catalog of summit paroxysms, covering the period 1986–2022, according to our cluster analysis is best characterized by 12 clusters of paroxysms. We separately analyze the inter-event times between onset times of successive clusters of paroxysms (inter-cluster inter-event times) and the inter-event times between successive paroxysms within clusters (intra-cluster inter-event times). Again, the Brownian Passage Time is the best-fitting model, obviously with very different parameters in the two cases. We test the best-fitting models by checking their ability to reproduce features of the real catalogs. Finally, we provide an example of how to use in practice such temporal models in the context of probabilistic hazard assessment, showing a possible use in the case of tephra fallout hazard from summit paroxysms.
Temporal models for the occurrence of Etna eruptions and implications for hazard assessment
by Laura Sandri, Alexander Garcia, Simona Scollo, Luigi Mereu, and Michele Prestifilippo
This manuscript develops a new database for eruptions at Mount Etna, separates it into flank and summit eruptions, and analyses the data to determine the best fitting model in the two cases. There are many examples of good practice in the analysis, including the testing of multiple hypotheses, the use of an appropriate information criterion to choose the best one, and the simulation of model variability and averaging by running an ensemble of models, not just using the best fit. The results show a clear difference between the two types of eruption, with summit eruptions showing clear evidence of short-term clustering, even in the primary data, and the best fit model for flank eruptions consistent with long-term anti-clustering indicating a renewal process with some memory. The results could in principle be used in managing the future risk of eruptions of the different types in operational forecasting mode for a time varying hazard rate, and some examples of this are given to illustrate this.
The paper is of a suitable standard for publication, and I recommend publication after addressing the following mostly minor points.
Ian Main, University of Edinburgh, 24 February 2026