Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica

The observed phenomenon of permanent degassing of the volcano Erebus is accompanied by a cyclic variation of gas composition and level of its crater lake that we proposed to model in the assumption that these fluctuations are caused by the arrival of batch of magma originated at shallow depth, ascen...

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Main Author: Molina Polania Aury, Claudia Indira, Molina Polania
Other Authors: Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO), Bureau de Recherches Géologiques et Minières (BRGM) (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), Université d'Orléans, Alain Burgisser
Format: Doctoral or Postdoctoral Thesis
Language:French
Published: HAL CCSD 2012
Subjects:
Online Access:https://theses.hal.science/tel-00772305
https://theses.hal.science/tel-00772305/document
https://theses.hal.science/tel-00772305/file/claudiaindira.molinapolania_2733_vd.pdf
id ftinsu:oai:HAL:tel-00772305v1
record_format openpolar
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language French
topic Magmatic system
Système magmatique
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle Magmatic system
Système magmatique
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Molina Polania Aury, Claudia Indira, Molina Polania
Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
topic_facet Magmatic system
Système magmatique
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description The observed phenomenon of permanent degassing of the volcano Erebus is accompanied by a cyclic variation of gas composition and level of its crater lake that we proposed to model in the assumption that these fluctuations are caused by the arrival of batch of magma originated at shallow depth, ascending in a conduit through which percolates a continuous flow of gas whose origin is deeper. We first showed that the observed effect of convection on the surface could not be explained solely by thermal convection of a liquid-crystals mixture. If a continuous supply of magma and gas in an open system simulates a pulsating behavior of the surface, this contribution must be large enough for the changes in surface velocity thus generated can be appreciated. The conduit diameter should be sufficient large to ensure the sustainability of convection and maintain the magma above its glass transition temperature. The presence of crystals convection accelerates and improves the efficiency of heat transfer between the upper and lower regions of the magmatic system; these crystals settle at the bottom of the chamber to form a layer of high concentration of about ten meters thickness. The introduction of two batches of magma from different depths of nucleation helped to highlight how their composition and the behavior of the lava lake were sensitive to the temperature at which they are generated. On the other hand, a batch will contribute to the degassing budget in proportions consistent with the observations only if a threshold of sufficient buoyancy was achieved. Otherwise, the migration of the amount of magma required for the degassing will only occur in a conduit of very large diameter. The physical parameters of the crust forming as the surface of the lava lake cools down, such as thickness and permeability, affect its ability to deform under pressure and to allow the trapped pressure to degas under an effusive regime. This pressure in turn influences the porosity of the magma at surface and possibly the degree of degassing ...
author2 Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO)
Bureau de Recherches Géologiques et Minières (BRGM) (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)
Université d'Orléans
Alain Burgisser
format Doctoral or Postdoctoral Thesis
author Molina Polania Aury, Claudia Indira, Molina Polania
author_facet Molina Polania Aury, Claudia Indira, Molina Polania
author_sort Molina Polania Aury, Claudia Indira, Molina Polania
title Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
title_short Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
title_full Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
title_fullStr Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
title_full_unstemmed Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica
title_sort convection and degassing of a magmatic system : the case of lava lake at erebus, antarctica
publisher HAL CCSD
publishDate 2012
url https://theses.hal.science/tel-00772305
https://theses.hal.science/tel-00772305/document
https://theses.hal.science/tel-00772305/file/claudiaindira.molinapolania_2733_vd.pdf
long_lat ENVELOPE(-60.667,-60.667,-62.983,-62.983)
ENVELOPE(-128.996,-128.996,55.046,55.046)
geographic Crater Lake
Lava Lake
geographic_facet Crater Lake
Lava Lake
genre Antarc*
Antarctica
Antarctique*
genre_facet Antarc*
Antarctica
Antarctique*
op_source https://theses.hal.science/tel-00772305
Sciences de la Terre. Université d'Orléans, 2012. Français. ⟨NNT : 2012ORLE2026⟩
op_relation NNT: 2012ORLE2026
tel-00772305
https://theses.hal.science/tel-00772305
https://theses.hal.science/tel-00772305/document
https://theses.hal.science/tel-00772305/file/claudiaindira.molinapolania_2733_vd.pdf
op_rights info:eu-repo/semantics/OpenAccess
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spelling ftinsu:oai:HAL:tel-00772305v1 2024-01-14T10:01:37+01:00 Convection and degassing of a magmatic system : the case of lava lake at Erebus, Antarctica Convection et dégazage d'un système magmatique : le cas du lac de lave l'Erebus, Antarctique. Molina Polania Aury, Claudia Indira, Molina Polania Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO) Bureau de Recherches Géologiques et Minières (BRGM) (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) Université d'Orléans Alain Burgisser 2012-09-27 https://theses.hal.science/tel-00772305 https://theses.hal.science/tel-00772305/document https://theses.hal.science/tel-00772305/file/claudiaindira.molinapolania_2733_vd.pdf fr fre HAL CCSD NNT: 2012ORLE2026 tel-00772305 https://theses.hal.science/tel-00772305 https://theses.hal.science/tel-00772305/document https://theses.hal.science/tel-00772305/file/claudiaindira.molinapolania_2733_vd.pdf info:eu-repo/semantics/OpenAccess https://theses.hal.science/tel-00772305 Sciences de la Terre. Université d'Orléans, 2012. Français. ⟨NNT : 2012ORLE2026⟩ Magmatic system Système magmatique [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/doctoralThesis Theses 2012 ftinsu 2023-12-20T17:22:39Z The observed phenomenon of permanent degassing of the volcano Erebus is accompanied by a cyclic variation of gas composition and level of its crater lake that we proposed to model in the assumption that these fluctuations are caused by the arrival of batch of magma originated at shallow depth, ascending in a conduit through which percolates a continuous flow of gas whose origin is deeper. We first showed that the observed effect of convection on the surface could not be explained solely by thermal convection of a liquid-crystals mixture. If a continuous supply of magma and gas in an open system simulates a pulsating behavior of the surface, this contribution must be large enough for the changes in surface velocity thus generated can be appreciated. The conduit diameter should be sufficient large to ensure the sustainability of convection and maintain the magma above its glass transition temperature. The presence of crystals convection accelerates and improves the efficiency of heat transfer between the upper and lower regions of the magmatic system; these crystals settle at the bottom of the chamber to form a layer of high concentration of about ten meters thickness. The introduction of two batches of magma from different depths of nucleation helped to highlight how their composition and the behavior of the lava lake were sensitive to the temperature at which they are generated. On the other hand, a batch will contribute to the degassing budget in proportions consistent with the observations only if a threshold of sufficient buoyancy was achieved. Otherwise, the migration of the amount of magma required for the degassing will only occur in a conduit of very large diameter. The physical parameters of the crust forming as the surface of the lava lake cools down, such as thickness and permeability, affect its ability to deform under pressure and to allow the trapped pressure to degas under an effusive regime. This pressure in turn influences the porosity of the magma at surface and possibly the degree of degassing ... Doctoral or Postdoctoral Thesis Antarc* Antarctica Antarctique* Institut national des sciences de l'Univers: HAL-INSU Crater Lake ENVELOPE(-60.667,-60.667,-62.983,-62.983) Lava Lake ENVELOPE(-128.996,-128.996,55.046,55.046)