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New insights into the relationship between mass eruption rate and volcanic column height based on the IVESPA dataset

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  • معلومة اضافية
    • Contributors:
      University of Exeter; University of Cambridge UK (CAM); British Geological Survey Edinburgh; British Geological Survey (BGS); Université de Genève = University of Geneva (UNIGE); United States Geological Survey (USGS); Institut de Physique du Globe de Paris (IPGP (UMR_7154)); Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité); Observatoire de Physique du Globe de Clermont-Ferrand (OPGC); Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA); Department of Atmospheric, Oceanic and Planetary Physics Oxford (AOPP); University of Oxford; Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Catania (INGV); Istituto Nazionale di Geofisica e Vulcanologia; University of British Columbia Vancouver; German Aerospace Center (DLR); ANR-10-LABX-0006,CLERVOLC,Clermont-Ferrand centre for research on volcanism(2010); ANR-16-IDEX-0001,CAP 20-25,CAP 20-25(2016)
    • بيانات النشر:
      HAL CCSD
      American Geophysical Union
    • الموضوع:
      2023
    • Collection:
      Institut national des sciences de l'Univers: HAL-INSU
    • نبذة مختصرة :
      co-auteur étranger ; International audience ; Rapid and simple estimation of the mass eruption rate (MER) from column height is essential for real-time volcanic hazard management and reconstruction of past explosive eruptions. Using 134 eruptive events from the new Independent Volcanic Eruption Source Parameter Archive (IVESPA, v1.0), we explore empirical MER-height relationships for four measures of column height: spreading level, sulfur dioxide height, and top height from direct observations and as reconstructed from deposits. These relationships show significant differences and highlight limitations of empirical models currently used in operational and research applications. The roles of atmospheric stratification, wind, and humidity remain challenging to detect acrossthe wide range of eruptive conditions spanned in IVESPA, ultimately resulting in empirical relationships outperforming analytical models that account for atmospheric conditions. This finding highlights challenges in constraining the MER-height relation using heterogeneous observations and empirical models, which reinforces the need for improved eruption source parameter data sets and physics-based models.
    • Relation:
      hal-03917579; https://uca.hal.science/hal-03917579; https://uca.hal.science/hal-03917579/document; https://uca.hal.science/hal-03917579/file/Aubry_etal_2023_GRL_IVESPA.pdf
    • الرقم المعرف:
      10.22541/essoar.167214588.86276236/v1
    • Rights:
      http://creativecommons.org/licenses/by/ ; info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.79A396F7