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dc.contributor.author Favalli M.
dc.contributor.author Pareschi M.T.
dc.contributor.author Zanchetta G.
dc.date.accessioned 2024-10-18T08:57:45Z
dc.date.available 2024-10-18T08:57:45Z
dc.date.issued 2006
dc.identifier https://www.elibrary.ru/item.asp?id=51172140
dc.identifier.citation Bulletin of Volcanology, 2006, 68, 4, 349-362
dc.identifier.issn 0258-8900
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/46004
dc.description.abstract During explosive eruptions the deposition of fine-grained volcanic ash fallout reduces soil permeability, favouring runoff of meteoric water and thus increasing the occurrence of catastrophic floods. A fully dynamic, two-dimensional model was used to simulate flooding scenarios in the Vesuvian area following an explosive volcanic eruption. The highest risk occurs in the catchment area of the Acerra-Nola Plain N and NE of Vesuvius. This plain has a population of 70,000 living in low-lying areas. This catchment area is vulnerable to ash fall because it lies downwind of the dominant synoptic circulation and it lacks a natural outflow toward the sea. Our numerical simulations predict dangerous scenarios, even in quiescent periods, during extreme rain events (return periods of 200 years have been considered), and a significant increase in the extent of the flooded areas due to renewed volcanic activity. Based on these simulations a hazard zonation has been proposed.
dc.subject VESUVIUS
dc.subject FLOOD
dc.subject FLOOD SIMULATION
dc.subject VOLCANIC HAZARD
dc.subject SOUTHERN ITALY
dc.subject PHREATOMAGMATIC ASH
dc.subject EXPLOSIVE ERUPTION
dc.title SIMULATION OF SYN-ERUPTIVE FLOODS IN THE CIRCUMVESUVIAN PLAIN (SOUTHERN ITALY)
dc.type Статья
dc.identifier.doi 10.1007/s00445-005-0011-z


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