Volcanic SO2 by UV-TIR satellite retrievals: validation by using ground-based network at Mt. Etna

• Published in: Annals of geophysics Vol. 57
• Main Authors: Claudia Spinetti, Giuseppe Giovanni Salerno, Tommaso Catalbiano, Elisa Carboni, Lieven Clarisse, Stefano Corradini, Roy Gordon Grainger, Pascal Andre Hedelt, Maria Elissavet Koukouli, Luca Merucci, Richard Siddans, Lucia Tampellini, Nicolas Theys, Pieter Valks, Claus Zehner
• Format: Journal Article
• Language: English
• Published: Istituto Nazionale di Geofisica e Vulcanologia (INGV) 01.01.2014
• ISSN: 1593-5213; 2037-416X
• DOI: 10.4401/ag-6641

Mt. Etna volcano in Italy is one of the most active degassing volcanoes worldwide, emitting a mean of 1.7 Mt/year of Sulphur Dioxide (SO2) in quiescent periods. In this work, SO2 measurements retrieved by Moderate Resolution Imaging Spectroradiometer (MODIS), hyper-spectral Infrared Atmospheric Sounding Interferometer (IASI) and the second Global Ozone Monitoring Experiment (GOME-2) data are compared with the ground-based data from the FLux Automatic MEasurement monitoring network (FLAME). Among the eighteen lava fountain episodes occurring at Mt. Etna in 2011, the 10 April paroxysmal event has been selected as a case-study for the simultaneous observation of the SO2 cloud by satellite and ground-based sensors. For each data-set two retrieval techniques were adopted and the measurements of SO2 mass and flux with their respective uncertainty were obtained. With respect to the FLAME SO2 mass of 4.5 Gg, MODIS, IASI and GOME-2 differ by about 10%, 15% and 30%, respectively. The SO2 flux correlation coefficient between MODIS and FLAME is 0.84. All the retrievals within the respective errors are in agreement with the ground-based measurements supporting the validity of these space measurements.