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Satellite‐based constraints on explosive SO 2 release from Soufrière Hills Volcano, Montserrat
Author(s) -
Carn Simon A.,
Prata Fred J.
Publication year - 2010
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2010gl044971
Subject(s) - volcano , dome (geology) , explosive eruption , explosive material , lava dome , lava , geology , volcanic gases , seismology , satellite , magma , geochemistry , geomorphology , aerospace engineering , chemistry , organic chemistry , engineering
Numerous episodes of explosive degassing have punctuated the 1995–2009 eruption of Soufrière Hills volcano (SHV), Montserrat, often following major lava dome collapses. We use ultraviolet (UV) and infrared (IR) satellite measurements to quantify sulfur dioxide (SO 2 ) released by explosive degassing, which is not captured by routine ground‐based and airborne gas monitoring. We find a total explosive SO 2 release of ∼0.5 Tg, which represents ∼6% of total SO 2 emissions from SHV since July 1995. The majority of this SO 2 (∼0.4 Tg) was vented following the most voluminous SHV dome collapses in July 2003 and May 2006. Based on our analysis, we suggest that the SO 2 burden measured following explosive disruption of lava domes depends on several factors, including the instantaneous lava effusion rate, dome height above the conduit, and the vertical component of directed explosions. Space‐based SO 2 measurements merit inclusion in routine gas monitoring at SHV and other dome‐forming volcanoes.

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