Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/331
AuthorsCaltabiano, T.* 
Burton, M.* 
Giammanco, S.* 
Allard, P.* 
Bruno, N.* 
Murè, F.* 
Romano, R.* 
TitleVolcanic gas emissions from the summit craters and flanks of Mt. Etna, 1987-2000
Issue Date2004
URIhttp://hdl.handle.net/2122/331
ISBN0875904084
KeywordsGas emissions
Mt. Etna
Subject Classification04. Solid Earth::04.08. Volcanology::04.08.01. Gases 
AbstractIn the last 13 years gas emissions from both the summit and the flanks of Mount Etna volcano have been monitored using remote sensing techniques (COSPEC, and FTIR since 2000) and on-site monitoring devices. The SO2 flux variations (600 to 25,000 Mg/day) indicated: (i) low values coinciding with deep seismicity prior to eruptions or/and preceding increases in summit volcanic activity; (ii) increasing trends tracking the ascent of fresh magma within the shallow feeding system and whose rate seems proportional to the speed of magma rise; (iii) decreasing trends related to progressive degassing of magma batches; (iv) an imbalance between the amount of magma erupted and that which contributed the SO2 emission (~ 13 % of the degassing magma having been erupted during the studied period), implying that magma degassing is dominantly intrusive; (v) a seasonal component, probably due to variations in solar zenith angle, meteorological parameters and, possibly, tidal forces.FTIR monitoring allowed to recognize significant variations of SO2/HCl and SO2/HF ratios in the volcanic plume which, combined with COSPEC data, provided new insight into the dynamics of ascent and degassing of discrete magma bodies. Strong variations in CO2-rich soil degassing are interpreted as markers of gradual magma ascent from great depth (>10 km) to the upper (<5 km) feeding system of Mt. Etna. These changes appear to precede increases in SO2 plume flux at the craters and, so, provide additional constraints upon the interpretation of COSPEC data and the modeling of magma rise at that volcano.
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