The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study

Satellite data provide crucial information to better understand volcanic processes and mitigate associated risks. In recent years, exploiting the growing number of spaceborne polar platforms, several automated volcanic monitoring systems have been developed. These, however, rely on good geometrical...

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Main Authors: Simone Aveni, Marco Laiolo, Adele Campus, Francesco Massimetti, Diego Coppola
Format: Article
Language:English
Published: MDPI AG 2023-05-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/15/10/2528
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author Simone Aveni
Marco Laiolo
Adele Campus
Francesco Massimetti
Diego Coppola
author_facet Simone Aveni
Marco Laiolo
Adele Campus
Francesco Massimetti
Diego Coppola
author_sort Simone Aveni
collection DOAJ
description Satellite data provide crucial information to better understand volcanic processes and mitigate associated risks. In recent years, exploiting the growing number of spaceborne polar platforms, several automated volcanic monitoring systems have been developed. These, however, rely on good geometrical and meteorological conditions, as well as on the occurrence of thermally detectable activity at the time of acquisition. A multiplatform approach can thus increase the number of volcanological-suitable scenes, minimise the temporal gap between acquisitions, and provide crucial information on the onset, evolution, and conclusion of both transient and long-lasting volcanic episodes. In this work, we assessed the capabilities of the MEdium Resolution Spectral Imager-II (MERSI-II) sensor aboard the Fengyun-3D (FY-3D) platform to detect and quantify heat flux sourced from volcanic activity. Using the Middle Infrared Observation of Volcanic Activity (MIROVA) algorithm, we processed 3117 MERSI-II scenes of Mount Etna acquired between January 2020 and February 2023. We then compared the Volcanic Radiative Power (VRP, in Watt) timeseries against those obtained by MODIS and VIIRS sensors. The remarkable agreement between the timeseries, both in trends and magnitudes, was corroborated by correlation coefficients (ρ) between 0.93 and 0.95 and coefficients of determination (R<sup>2</sup>) ranging from 0.79 to 0.84. Integrating the datasets of the three sensors, we examined the effusive eruption of Mount Etna started on 27 November 2022, and estimated a total volume of erupted lava of 8.15 ± 2.44 × 10<sup>6</sup> m<sup>3</sup> with a Mean Output Rate (MOR) of 1.35 ± 0.40 m<sup>3</sup> s<sup>−1</sup>. The reduced temporal gaps between acquisitions revealed that rapid variations in cloud coverage as well as geometrically unfavourable conditions play a major role in thermal volcano monitoring. Evaluating the capabilities of MERSI-II, we also highlight how a multiplatform approach is essential to enhance the efficiency of satellite-based systems for volcanic surveillance.
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spelling doaj.art-f94504c3bdf0474e8f67eb7ef5b9e3b82023-11-18T03:06:23ZengMDPI AGRemote Sensing2072-42922023-05-011510252810.3390/rs15102528The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case StudySimone Aveni0Marco Laiolo1Adele Campus2Francesco Massimetti3Diego Coppola4Department of Civil, Constructional and Environmental Engineering (DICEA), Sapienza University of Rome, Via Eudossiana 18, 00184 Rome, ItalyDepartment of Earth Sciences, University of Turin, Via Valperga Caluso 35, 10125 Turin, ItalyDepartment of Earth Sciences, University of Turin, Via Valperga Caluso 35, 10125 Turin, ItalyDepartment of Earth Sciences, University of Turin, Via Valperga Caluso 35, 10125 Turin, ItalyDepartment of Earth Sciences, University of Turin, Via Valperga Caluso 35, 10125 Turin, ItalySatellite data provide crucial information to better understand volcanic processes and mitigate associated risks. In recent years, exploiting the growing number of spaceborne polar platforms, several automated volcanic monitoring systems have been developed. These, however, rely on good geometrical and meteorological conditions, as well as on the occurrence of thermally detectable activity at the time of acquisition. A multiplatform approach can thus increase the number of volcanological-suitable scenes, minimise the temporal gap between acquisitions, and provide crucial information on the onset, evolution, and conclusion of both transient and long-lasting volcanic episodes. In this work, we assessed the capabilities of the MEdium Resolution Spectral Imager-II (MERSI-II) sensor aboard the Fengyun-3D (FY-3D) platform to detect and quantify heat flux sourced from volcanic activity. Using the Middle Infrared Observation of Volcanic Activity (MIROVA) algorithm, we processed 3117 MERSI-II scenes of Mount Etna acquired between January 2020 and February 2023. We then compared the Volcanic Radiative Power (VRP, in Watt) timeseries against those obtained by MODIS and VIIRS sensors. The remarkable agreement between the timeseries, both in trends and magnitudes, was corroborated by correlation coefficients (ρ) between 0.93 and 0.95 and coefficients of determination (R<sup>2</sup>) ranging from 0.79 to 0.84. Integrating the datasets of the three sensors, we examined the effusive eruption of Mount Etna started on 27 November 2022, and estimated a total volume of erupted lava of 8.15 ± 2.44 × 10<sup>6</sup> m<sup>3</sup> with a Mean Output Rate (MOR) of 1.35 ± 0.40 m<sup>3</sup> s<sup>−1</sup>. The reduced temporal gaps between acquisitions revealed that rapid variations in cloud coverage as well as geometrically unfavourable conditions play a major role in thermal volcano monitoring. Evaluating the capabilities of MERSI-II, we also highlight how a multiplatform approach is essential to enhance the efficiency of satellite-based systems for volcanic surveillance.https://www.mdpi.com/2072-4292/15/10/2528MERSI-IIFY-3DEtnaMODISVIIRSMIROVA
spellingShingle Simone Aveni
Marco Laiolo
Adele Campus
Francesco Massimetti
Diego Coppola
The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
Remote Sensing
MERSI-II
FY-3D
Etna
MODIS
VIIRS
MIROVA
title The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
title_full The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
title_fullStr The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
title_full_unstemmed The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
title_short The Capabilities of FY-3D/MERSI-II Sensor to Detect and Quantify Thermal Volcanic Activity: The 2020–2023 Mount Etna Case Study
title_sort capabilities of fy 3d mersi ii sensor to detect and quantify thermal volcanic activity the 2020 2023 mount etna case study
topic MERSI-II
FY-3D
Etna
MODIS
VIIRS
MIROVA
url https://www.mdpi.com/2072-4292/15/10/2528
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