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Report on Etna (Italy) — 1 September-7 September 2010

Smithsonian / US Geological Survey Weekly Volcanic Activity Report, 1 September-7 September 2010
Managing Editor: Sally Kuhn Sennert

Please cite this report as:

Global Volcanism Program, 2010. Report on Etna (Italy). In: Sennert, S K (ed.), Weekly Volcanic Activity Report, 1 September-7 September 2010. Smithsonian Institution and US Geological Survey.

Volcano Profile |  Weekly Report (1 September-7 September 2010)



37.748°N, 14.999°E; summit elev. 3295 m

All times are local (unless otherwise noted)

INGV-CT reported that on 25 August a powerful explosion from Etna's Bocca Nuova crater initiated a series of ash emissions, which continued at decreasing strength for about 20 minutes. A thermal camera located at La Montagnola, 3 km S of the summit craters, showed ejected hot material and a cauliflower-shaped, dark gray ash plume that rose about 1 km and drifted E. Ashfall was reported in areas SE from Etna to Catania (27 km S). An inspection the next morning revealed that the W wall of the BN-1 crater of Bocca Nuova had collapsed. During 25-29 August a total of seven explosions were recorded.

Geologic Background. Mount Etna, towering above Catania, Sicily's second largest city, has one of the world's longest documented records of historical volcanism, dating back to 1500 BCE. Historical lava flows of basaltic composition cover much of the surface of this massive volcano, whose edifice is the highest and most voluminous in Italy. The Mongibello stratovolcano, truncated by several small calderas, was constructed during the late Pleistocene and Holocene over an older shield volcano. The most prominent morphological feature of Etna is the Valle del Bove, a 5 x 10 km horseshoe-shaped caldera open to the east. Two styles of eruptive activity typically occur, sometimes simultaneously. Persistent explosive eruptions, sometimes with minor lava emissions, take place from one or more summit craters. Flank vents, typically with higher effusion rates, are less frequently active and originate from fissures that open progressively downward from near the summit (usually accompanied by Strombolian eruptions at the upper end). Cinder cones are commonly constructed over the vents of lower-flank lava flows. Lava flows extend to the foot of the volcano on all sides and have reached the sea over a broad area on the SE flank.

Source: Sezione di Catania - Osservatorio Etneo (INGV)