Academic Journal

Volcanic Emissions, Plume Dispersion, and DownwindRadiative Impacts Following Mount Etna Series of Eruptionsof February 21–26, 2021

التفاصيل البيبلوغرافية
العنوان: Volcanic Emissions, Plume Dispersion, and DownwindRadiative Impacts Following Mount Etna Series of Eruptionsof February 21–26, 2021
المؤلفون: Sellitto, Pasquale, Salerno, Giuseppe, Corradini, Stefano, Xueref-Remy, Irène, Riandet, Aurélie, Bellon, Clémence, Khaykin, Sergey, Ancellet, Gérard, Lolli, Simone, Welton, Ellsworth, J., Boselli, Antonella, Sannino, Alessia, Cuesta, Juan, Guermazi, Henda, Eremenko, Maxim, Merucci, Luca, Stelitano, Dario, Guerrieri, Lorenzo, Legras, Bernard
المساهمون: Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Osservatorio Etneo di Catania, Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Catania (INGV), Istituto Nazionale di Geofisica e Vulcanologia-Istituto Nazionale di Geofisica e Vulcanologia, Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Roma (INGV), Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Nazionale Terremoti, Institut méditerranéen de biodiversité et d'écologie marine et continentale (IMBE), Avignon Université (AU)-Aix Marseille Université (AMU)-Institut de recherche pour le développement IRD : UMR237-Centre National de la Recherche Scientifique (CNRS), TROPO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Istituto di Metodologie per l'Analisi Ambientale (IMAA), Consiglio Nazionale delle Ricerche Potenza (CNR), NASA Goddard Space Flight Center (GSFC), Dipartimento di Fisica "Ettore Pancini", University of Naples Federico II = Università degli studi di Napoli Federico II, Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-École nationale des ponts et chaussées (ENPC)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS-PSL, École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)
المصدر: ISSN: 2169-897X ; EISSN: 2169-8996.
بيانات النشر: CCSD
American Geophysical Union
سنة النشر: 2023
المجموعة: Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ
مصطلحات موضوعية: [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph], [SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/Volcanology
الوصف: soumis a JGR Atmospheres - First posted online: Fri, 8 Oct 2021 ; International audience ; During the extended activity of Mount Etna volcano in February-April 2021, three distinct paroxysmal events took place from 21 to 26 February, which were associated with a very uncommon transport of the injected upper-tropospheric plumes towards the north. Using a synergy of observations and modelling, we characterised the emissions and three-dimensional dispersion for these three plumes, we monitor their downwind distribution and optical properties, and we estimate their radiative impacts at selected locations. With a satellite-based source inversion, we estimate the emitted sulphur dioxide (SO2) mass at an integrated value of 55 kt and plumes injections at up to 12 km altitudes, which qualifies this series as an extreme event for Mount Etna. Then, we combine Lagrangian dispersion modelling, initialised with measured temporally-resolved SO2 emission fluxes and altitudes, with satellite observations to track the dispersion of the three individual plumes. The transport towards the north allowed the height-resolved downwind monitoring of the plumes at selected observatories in France, Italy and Israel, using LiDARs and photometric aerosol observations. Volcanic-specific aerosol optical depths in the visible spectral range ranging from about 0.004 to 0.03 and local daily average shortwave radiative forcing ranging from about -0.2 to -1.2 W/m2 (at the top of atmosphere) and from about -0.2 to -3.0 W/m2 (at the surface) are found. The composition (possible presence of ash), aerosol optical depth and radiative forcing of the plume has a large inter- and intra-plume variability and thus depend strongly on the position of the sampled section of the plumes.
نوع الوثيقة: article in journal/newspaper
اللغة: English
DOI: 10.1029/2021JD035974
الاتاحة: https://insu.hal.science/insu-03437407
https://insu.hal.science/insu-03437407v2/document
https://insu.hal.science/insu-03437407v2/file/JGR%20Atmospheres%20-%202023%20-%20Sellitto%20-%20Volcanic%20.pdf
https://doi.org/10.1029/2021JD035974
Rights: info:eu-repo/semantics/OpenAccess
رقم الانضمام: edsbas.42C7D4ED
قاعدة البيانات: BASE