Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion

Mars has a complex climate, characterized by carbon dioxide and water cycles, and dust transport at all scales. These cycles are mainly controlled by the seasonal condensation of CO₂ and water ice deposits at high latitudes during the polar night and their sublimation during the local spring. There...

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Main Author: Andrieu, François
Other Authors: Géosciences Paris Sud (GEOPS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Université Paris Saclay (COmUE), Frédéric Schmidt
Format: Doctoral or Postdoctoral Thesis
Language:French
Published: HAL CCSD 2015
Subjects:
Online Access:https://theses.hal.science/tel-01328824
https://theses.hal.science/tel-01328824/document
https://theses.hal.science/tel-01328824/file/72780_ANDRIEU_2015_diffusion.pdf
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spelling ftuniparissaclay:oai:HAL:tel-01328824v1 2024-06-16T07:42:48+00:00 Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion Caractérisation des surfaces glacées de Mars par imagerie hyperspectrale : inversion du transfert radiatif Andrieu, François Géosciences Paris Sud (GEOPS) Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS) Université Paris Saclay (COmUE) Frédéric Schmidt 2015-12-11 https://theses.hal.science/tel-01328824 https://theses.hal.science/tel-01328824/document https://theses.hal.science/tel-01328824/file/72780_ANDRIEU_2015_diffusion.pdf fr fre HAL CCSD NNT: 2015SACLS178 tel-01328824 https://theses.hal.science/tel-01328824 https://theses.hal.science/tel-01328824/document https://theses.hal.science/tel-01328824/file/72780_ANDRIEU_2015_diffusion.pdf info:eu-repo/semantics/OpenAccess https://theses.hal.science/tel-01328824 Matière Condensée [cond-mat]. Université Paris Saclay (COmUE), 2015. Français. ⟨NNT : 2015SACLS178⟩ Mars Radiative Transfer Remote sensing CO₂ Ice Water Ice Massive inversion Transfert Radiatif Télédétection Glace de CO₂ Glace d'eau Inversion massive [PHYS.COND]Physics [physics]/Condensed Matter [cond-mat] info:eu-repo/semantics/doctoralThesis Theses 2015 ftuniparissaclay 2024-05-17T00:13:48Z Mars has a complex climate, characterized by carbon dioxide and water cycles, and dust transport at all scales. These cycles are mainly controlled by the seasonal condensation of CO₂ and water ice deposits at high latitudes during the polar night and their sublimation during the local spring. There are a lot of interactions between the CO₂ , water and dust cycles on Mars and they influence each other. An active seasonal process illustrates particularly well these links: the cryoventing, cold CO₂ gas jets triggered by seasonal sublimation of CO₂ deposits, which can put dust from the regolith in suspension into the atmosphere durably, and whose activity seems to be modulated by the exchange of water at the surface.The purpose of this thesis is to allow the use of the available hyperspectral imaging data to their full potential, to bring new constraints on seasonal exchanges between surface and atmosphere and the interactions between the different cycles (CO₂ , water , dust), focusing on cold gas jets. To achieve this, a semi-analytical radiative transfer model in compact ices and an effective inversion method were developed and validated.The radiative transfer model describes the interaction of light with a surface quantitatively, using the following parameters: thickness of the layer, volume proportions and grain-sizes of impurities, surface roughness. It is based on several key assumptions: geometrical optics, piecewise-continuous media quasi-spherical inclusions. The two-stream approximation is used for the radiative transfer inside the layer, but the surface specular reflectance is estimated taking into account the variability of the facets orientations from the surface roughness. This model was validated both numerically and on laboratory data.The inversion method consists in exploring synthetic databases generated by the radiative transfer model and determining the most likely sets of parameters to reproduce a given measure. The inversion is based on the Bayesian formalism: the manipulated variables are ... Doctoral or Postdoctoral Thesis polar night Archives ouvertes de Paris-Saclay
institution Open Polar
collection Archives ouvertes de Paris-Saclay
op_collection_id ftuniparissaclay
language French
topic Mars
Radiative Transfer
Remote sensing
CO₂ Ice
Water Ice
Massive inversion
Transfert Radiatif
Télédétection
Glace de CO₂
Glace d'eau
Inversion massive
[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]
spellingShingle Mars
Radiative Transfer
Remote sensing
CO₂ Ice
Water Ice
Massive inversion
Transfert Radiatif
Télédétection
Glace de CO₂
Glace d'eau
Inversion massive
[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]
Andrieu, François
Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
topic_facet Mars
Radiative Transfer
Remote sensing
CO₂ Ice
Water Ice
Massive inversion
Transfert Radiatif
Télédétection
Glace de CO₂
Glace d'eau
Inversion massive
[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]
description Mars has a complex climate, characterized by carbon dioxide and water cycles, and dust transport at all scales. These cycles are mainly controlled by the seasonal condensation of CO₂ and water ice deposits at high latitudes during the polar night and their sublimation during the local spring. There are a lot of interactions between the CO₂ , water and dust cycles on Mars and they influence each other. An active seasonal process illustrates particularly well these links: the cryoventing, cold CO₂ gas jets triggered by seasonal sublimation of CO₂ deposits, which can put dust from the regolith in suspension into the atmosphere durably, and whose activity seems to be modulated by the exchange of water at the surface.The purpose of this thesis is to allow the use of the available hyperspectral imaging data to their full potential, to bring new constraints on seasonal exchanges between surface and atmosphere and the interactions between the different cycles (CO₂ , water , dust), focusing on cold gas jets. To achieve this, a semi-analytical radiative transfer model in compact ices and an effective inversion method were developed and validated.The radiative transfer model describes the interaction of light with a surface quantitatively, using the following parameters: thickness of the layer, volume proportions and grain-sizes of impurities, surface roughness. It is based on several key assumptions: geometrical optics, piecewise-continuous media quasi-spherical inclusions. The two-stream approximation is used for the radiative transfer inside the layer, but the surface specular reflectance is estimated taking into account the variability of the facets orientations from the surface roughness. This model was validated both numerically and on laboratory data.The inversion method consists in exploring synthetic databases generated by the radiative transfer model and determining the most likely sets of parameters to reproduce a given measure. The inversion is based on the Bayesian formalism: the manipulated variables are ...
author2 Géosciences Paris Sud (GEOPS)
Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)
Université Paris Saclay (COmUE)
Frédéric Schmidt
format Doctoral or Postdoctoral Thesis
author Andrieu, François
author_facet Andrieu, François
author_sort Andrieu, François
title Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
title_short Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
title_full Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
title_fullStr Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
title_full_unstemmed Characterization of icy surfaces on Mars using hyper spectral data : a radiative transfer inversion
title_sort characterization of icy surfaces on mars using hyper spectral data : a radiative transfer inversion
publisher HAL CCSD
publishDate 2015
url https://theses.hal.science/tel-01328824
https://theses.hal.science/tel-01328824/document
https://theses.hal.science/tel-01328824/file/72780_ANDRIEU_2015_diffusion.pdf
genre polar night
genre_facet polar night
op_source https://theses.hal.science/tel-01328824
Matière Condensée [cond-mat]. Université Paris Saclay (COmUE), 2015. Français. ⟨NNT : 2015SACLS178⟩
op_relation NNT: 2015SACLS178
tel-01328824
https://theses.hal.science/tel-01328824
https://theses.hal.science/tel-01328824/document
https://theses.hal.science/tel-01328824/file/72780_ANDRIEU_2015_diffusion.pdf
op_rights info:eu-repo/semantics/OpenAccess
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