Spectral Emissivity of Phonolite Lava at High Temperature

International audience The rheology and thermodynamical evolution of magma, either in reservoirs, conduits or at the surface, are governed by temperature. To determine the field temperature, remote sensing methods based on measuring the infrared radiance are widely applied, but they are subject to a...

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Published in:IEEE Transactions on Geoscience and Remote Sensing
Main Authors: Li, Hao, Andujar, Joan, Slodczyk, Aneta, de Sousa Meneses, Domingos, Scaillet, Bruno, Echegut, Patrick, Biren, Jonas, Oppenheimer, Clive
Other Authors: Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO), Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Magma - UMR7327, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Conditions Extrêmes et Matériaux : Haute Température et Irradiation (CEMHTI), Université d'Orléans (UO)-Institut de Chimie - CNRS Chimie (INC-CNRS)-Centre National de la Recherche Scientifique (CNRS), University of Cambridge UK (CAM), TelluS program of CNRS/INSU with RADIABAR project, ANR-10-LABX-0100,VOLTAIRE,Geofluids and Volatil elements – Earth, Atmosphere, Interfaces – Resources and Environment(2010), ANR-11-EQPX-0036,PLANEX,Planète Expérimentation: simulation et analyse in-situ en conditions extrêmes(2011)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2022
Subjects:
Online Access:https://insu.hal.science/insu-03433900
https://insu.hal.science/insu-03433900/document
https://insu.hal.science/insu-03433900/file/FINAL_VERSION-IEEE-2021.pdf
https://doi.org/10.1109/TGRS.2021.3104657
id ftanrparis:oai:HAL:insu-03433900v1
record_format openpolar
institution Open Polar
collection Portail HAL-ANR (Agence Nationale de la Recherche)
op_collection_id ftanrparis
language English
topic Emissivity
phonolite lava
radiative transfer
remote sensing
temperature measurement
thermal infrared
[SDU]Sciences of the Universe [physics]
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle Emissivity
phonolite lava
radiative transfer
remote sensing
temperature measurement
thermal infrared
[SDU]Sciences of the Universe [physics]
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Li, Hao
Andujar, Joan
Slodczyk, Aneta
de Sousa Meneses, Domingos
Scaillet, Bruno
Echegut, Patrick
Biren, Jonas
Oppenheimer, Clive
Spectral Emissivity of Phonolite Lava at High Temperature
topic_facet Emissivity
phonolite lava
radiative transfer
remote sensing
temperature measurement
thermal infrared
[SDU]Sciences of the Universe [physics]
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description International audience The rheology and thermodynamical evolution of magma, either in reservoirs, conduits or at the surface, are governed by temperature. To determine the field temperature, remote sensing methods based on measuring the infrared radiance are widely applied, but they are subject to assumptions and caveats that can propagate into large uncertainties. This is related to the poor knowledge of one of the most critical parameters, namely the spectral emissivity. In this work we aim at filling this gap through in situ spectral emissivity measurements performed over wide temperature (700-1600 K) and spectral ranges (1.25-25 µm) on two representative phonolitic compositions from Erebus (Antartica) and Teide (Spain) volcanoes. The laboratory spectra allow to determine precisely spectral emissivity in the thermal infrared (TIR), middle infrared (MIR), and shortwave infrared (SWIR) ranges. The results reveal the complexity and contrasted behavior of the radiative properties of the two rocks melts, despite their broadly similar composition. The spectral emissivity varies significantly as a function of temperature, composition, crystallinity, thickness, and thermal history. Altogether, the data reveal that emissivity cannot be considered as a constant value and question previous arguments that active lava always has lower emissivity than frozen lava. Finally, the laboratory-measured values of spectral emissivity were used to refine the temperature of Erebus lava lake gathered from previous remote sensing methods.
author2 Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO)
Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)
Magma - UMR7327
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC)
Conditions Extrêmes et Matériaux : Haute Température et Irradiation (CEMHTI)
Université d'Orléans (UO)-Institut de Chimie - CNRS Chimie (INC-CNRS)-Centre National de la Recherche Scientifique (CNRS)
University of Cambridge UK (CAM)
TelluS program of CNRS/INSU with RADIABAR project
ANR-10-LABX-0100,VOLTAIRE,Geofluids and Volatil elements – Earth, Atmosphere, Interfaces – Resources and Environment(2010)
ANR-11-EQPX-0036,PLANEX,Planète Expérimentation: simulation et analyse in-situ en conditions extrêmes(2011)
format Article in Journal/Newspaper
author Li, Hao
Andujar, Joan
Slodczyk, Aneta
de Sousa Meneses, Domingos
Scaillet, Bruno
Echegut, Patrick
Biren, Jonas
Oppenheimer, Clive
author_facet Li, Hao
Andujar, Joan
Slodczyk, Aneta
de Sousa Meneses, Domingos
Scaillet, Bruno
Echegut, Patrick
Biren, Jonas
Oppenheimer, Clive
author_sort Li, Hao
title Spectral Emissivity of Phonolite Lava at High Temperature
title_short Spectral Emissivity of Phonolite Lava at High Temperature
title_full Spectral Emissivity of Phonolite Lava at High Temperature
title_fullStr Spectral Emissivity of Phonolite Lava at High Temperature
title_full_unstemmed Spectral Emissivity of Phonolite Lava at High Temperature
title_sort spectral emissivity of phonolite lava at high temperature
publisher HAL CCSD
publishDate 2022
url https://insu.hal.science/insu-03433900
https://insu.hal.science/insu-03433900/document
https://insu.hal.science/insu-03433900/file/FINAL_VERSION-IEEE-2021.pdf
https://doi.org/10.1109/TGRS.2021.3104657
genre antartic*
genre_facet antartic*
op_source ISSN: 0196-2892
IEEE Transactions on Geoscience and Remote Sensing
https://insu.hal.science/insu-03433900
IEEE Transactions on Geoscience and Remote Sensing, 2022, 60, pp.1-15. ⟨10.1109/TGRS.2021.3104657⟩
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insu-03433900
https://insu.hal.science/insu-03433900
https://insu.hal.science/insu-03433900/document
https://insu.hal.science/insu-03433900/file/FINAL_VERSION-IEEE-2021.pdf
doi:10.1109/TGRS.2021.3104657
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1109/TGRS.2021.3104657
container_title IEEE Transactions on Geoscience and Remote Sensing
container_volume 60
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spelling ftanrparis:oai:HAL:insu-03433900v1 2024-05-19T07:32:45+00:00 Spectral Emissivity of Phonolite Lava at High Temperature Li, Hao Andujar, Joan Slodczyk, Aneta de Sousa Meneses, Domingos Scaillet, Bruno Echegut, Patrick Biren, Jonas Oppenheimer, Clive Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO) Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS) Magma - UMR7327 Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC) Conditions Extrêmes et Matériaux : Haute Température et Irradiation (CEMHTI) Université d'Orléans (UO)-Institut de Chimie - CNRS Chimie (INC-CNRS)-Centre National de la Recherche Scientifique (CNRS) University of Cambridge UK (CAM) TelluS program of CNRS/INSU with RADIABAR project ANR-10-LABX-0100,VOLTAIRE,Geofluids and Volatil elements – Earth, Atmosphere, Interfaces – Resources and Environment(2010) ANR-11-EQPX-0036,PLANEX,Planète Expérimentation: simulation et analyse in-situ en conditions extrêmes(2011) 2022 https://insu.hal.science/insu-03433900 https://insu.hal.science/insu-03433900/document https://insu.hal.science/insu-03433900/file/FINAL_VERSION-IEEE-2021.pdf https://doi.org/10.1109/TGRS.2021.3104657 en eng HAL CCSD Institute of Electrical and Electronics Engineers info:eu-repo/semantics/altIdentifier/doi/10.1109/TGRS.2021.3104657 insu-03433900 https://insu.hal.science/insu-03433900 https://insu.hal.science/insu-03433900/document https://insu.hal.science/insu-03433900/file/FINAL_VERSION-IEEE-2021.pdf doi:10.1109/TGRS.2021.3104657 info:eu-repo/semantics/OpenAccess ISSN: 0196-2892 IEEE Transactions on Geoscience and Remote Sensing https://insu.hal.science/insu-03433900 IEEE Transactions on Geoscience and Remote Sensing, 2022, 60, pp.1-15. ⟨10.1109/TGRS.2021.3104657⟩ Emissivity phonolite lava radiative transfer remote sensing temperature measurement thermal infrared [SDU]Sciences of the Universe [physics] [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/article Journal articles 2022 ftanrparis https://doi.org/10.1109/TGRS.2021.3104657 2024-04-30T17:07:54Z International audience The rheology and thermodynamical evolution of magma, either in reservoirs, conduits or at the surface, are governed by temperature. To determine the field temperature, remote sensing methods based on measuring the infrared radiance are widely applied, but they are subject to assumptions and caveats that can propagate into large uncertainties. This is related to the poor knowledge of one of the most critical parameters, namely the spectral emissivity. In this work we aim at filling this gap through in situ spectral emissivity measurements performed over wide temperature (700-1600 K) and spectral ranges (1.25-25 µm) on two representative phonolitic compositions from Erebus (Antartica) and Teide (Spain) volcanoes. The laboratory spectra allow to determine precisely spectral emissivity in the thermal infrared (TIR), middle infrared (MIR), and shortwave infrared (SWIR) ranges. The results reveal the complexity and contrasted behavior of the radiative properties of the two rocks melts, despite their broadly similar composition. The spectral emissivity varies significantly as a function of temperature, composition, crystallinity, thickness, and thermal history. Altogether, the data reveal that emissivity cannot be considered as a constant value and question previous arguments that active lava always has lower emissivity than frozen lava. Finally, the laboratory-measured values of spectral emissivity were used to refine the temperature of Erebus lava lake gathered from previous remote sensing methods. Article in Journal/Newspaper antartic* Portail HAL-ANR (Agence Nationale de la Recherche) IEEE Transactions on Geoscience and Remote Sensing 60 1 15