Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/16917
Authors: Bonfanti, Pietro* 
Branca, Stefano* 
Cassisi, Carmelo* 
Coltelli, Mauro* 
Prestifilippo, Michele* 
Scollo, Simona* 
Title: A fast compilation of the VONA messages using a computer-assisted procedure
Journal: Bulletin of Volcanology 
Series/Report no.: /86 (2024)
Publisher: Springer-Nature
Issue Date: 2024
DOI: 10.1007/s00445-024-01728-6
Keywords: Etna volcano
Monitoring activity
VONA messages
Computer-assisted procedure
Hazard mitigation
Subject Classification04.08. Volcanology 
Abstract: Mt. Etna, in Italy, is one of the most active volcanoes in the world, producing several explosive events in recent years. Those eruptions form high eruption columns that often reach the top of the troposphere (and sometimes even the lower part of the stratosphere) and create several disruptions to air traffic, mainly to the Fontanarossa International Airport in Catania, which is about 20 NM (~ 37 km; NM = Nautical Miles) away from the summit craters and is located in the main wind direction. In Italy, the institution responsible for volcano monitoring is the Istituto Nazionale di Geofisica e Vulcanologia (INGV). In 2007, the INGV, Osservatorio Etneo (INGV-OE) in Catania was appointed as “State Volcano Observatory” (SVO) and, in 2014, sent the first Volcano Observatory Notice for Aviation (VONA) message. Since that moment, several VONA messages have been sent, mainly due to the high frequency of Etna activity. In order to facilitate and speed in the generation and the dispatch of the VONA messages, a computer-assisted procedure has been designed and built to help the work done by the volcanologist on duty and by the two shift workers of the 24/7 Control Room of INGV-OE. Consequently, information on the explosive activity can be quickly provided to the Volcanic Ash Advisory Center (VAAC) in Toulouse and national air traffic offices, reducing risks to aviation operations. In this work, we describe how the computer-assisted procedure works, addressing the main advantages and possible improvements. We retain that a similar approach could be easily applied to other volcano observatories worldwide.
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