Volcanic Clouds Characterization of the 2020–2022 Sequence of Mt. Etna Lava Fountains Using MSG-SEVIRI and Products’ Cross-Comparison
| dc.contributor.author | Guerrieri, L. | |
| dc.contributor.author | Corradini, S. | |
| dc.contributor.author | Theys, N. | |
| dc.contributor.author | Stelitano, D. | |
| dc.contributor.author | Merucci, L. | |
| dc.date | 2023 | |
| dc.date.accessioned | 2023-04-13T08:02:53Z | |
| dc.date.available | 2023-04-13T08:02:53Z | |
| dc.identifier.uri | https://orfeo.belnet.be/handle/internal/10867 | |
| dc.description | From December 2020 to February 2022, 66 lava fountains (LF) occurred at Etna volcano (Italy). Despite their short duration (an average of about two hours), they produced a strong impact on human life, environment, and air traffic. In this work, the measurements collected from the Spinning Enhanced Visible and InfraRed Imager (SEVIRI) instrument, on board Meteosat Second Generation (MSG) geostationary satellite, are processed every 15 min to characterize the volcanic clouds produced during the activities. In particular, a quantitative estimation of volcanic cloud top height (VCTH) and ash/ice/SO2 masses’ time series are obtained. VCTHs are computed by integrating three different retrieval approaches based on coldest pixel detection, plume tracking, and HYSPLIT models, while particles and gas retrievals are realized simultaneously by exploiting the Volcanic Plume Retrieval (VPR) real-time procedure. The discrimination between ashy and icy pixels is carried out by applying the Brightness Temperature Difference (BTD) method with thresholds obtained by making specific Radiative Transfer Model simulations. Results indicate a VCTH variation during the entire period between 4 and 13 km, while the SO2, ash, and ice total masses reach maximum values of about 50, 100, and 300 Gg, respectively. The cumulative ash, ice, and SO2 emitted from all the 2020–2022 LFs in the atmosphere are about 750, 2300, and 670 Gg, respectively. All the retrievals indicate that the overall activity can be grouped into 3 main periods in which it passes from high (December 2020 to March 2021), low (March to June 2021), and medium/high (June 2021 to February 2022). The different products have been validated by using TROPOspheric Monitoring Instrument (TROPOMI) polar satellite sensor, Volcano Observatory Notices for Aviation (VONA) bulletins, and by processing the SEVIRI data considering a different and more accurate retrieval approach. The products’ cross-comparison shows a generally good agreement, except for the SO2 total mass in case of high ash/ice content in the volcanic cloud. | |
| dc.language | eng | |
| dc.title | Volcanic Clouds Characterization of the 2020–2022 Sequence of Mt. Etna Lava Fountains Using MSG-SEVIRI and Products’ Cross-Comparison | |
| dc.type | Article | |
| dc.subject.frascati | Earth and related Environmental sciences | |
| dc.audience | Scientific | |
| dc.subject.free | Mount Etna eruption | |
| dc.subject.free | volcanic cloud top height | |
| dc.subject.free | volcanic ash/ice particles and SO2 retrievals | |
| dc.source.title | Remote Sensing | |
| dc.source.volume | 15 | |
| dc.source.page | A2055 | |
| Orfeo.peerreviewed | Yes | |
| dc.identifier.doi | 10.3390/rs15082055 | |
| dc.identifier.scopus |
