Tomography of the Indian Ocean by waveform inversion

The arrival of some plumes and the birth of hotspots at the Earth surface is more likely the cause of the break up of the Pangea ~200 Ma ago, during the jurassic era. The Gondwana was formed by many continental masses like Africa, Australia, India and Antarctic. The late cretaceous was affected by a...

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Main Author: Dongmo Wamba, Mathurin
Other Authors: 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), Université Paris Cité, Jean-Paul Montagner, Barbara Romanowicz
Format: Doctoral or Postdoctoral Thesis
Language:French
Published: HAL CCSD 2020
Subjects:
Online Access:https://theses.hal.science/tel-03216584
https://theses.hal.science/tel-03216584/document
https://theses.hal.science/tel-03216584/file/DONGMO_WAMBA_Mathurin_va.pdf
id ftinsu:oai:HAL:tel-03216584v1
record_format openpolar
spelling ftinsu:oai:HAL:tel-03216584v1 2023-05-15T13:40:33+02:00 Tomography of the Indian Ocean by waveform inversion Tomographie de l'Océan Indien par inversion de forme d'onde Dongmo Wamba, Mathurin 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) Université Paris Cité Jean-Paul Montagner Barbara Romanowicz 2020-07-08 https://theses.hal.science/tel-03216584 https://theses.hal.science/tel-03216584/document https://theses.hal.science/tel-03216584/file/DONGMO_WAMBA_Mathurin_va.pdf fr fre HAL CCSD NNT: 2020UNIP7077 tel-03216584 https://theses.hal.science/tel-03216584 https://theses.hal.science/tel-03216584/document https://theses.hal.science/tel-03216584/file/DONGMO_WAMBA_Mathurin_va.pdf info:eu-repo/semantics/OpenAccess https://theses.hal.science/tel-03216584 Sciences de la Terre. Université Paris Cité, 2020. Français. ⟨NNT : 2020UNIP7077⟩ Hotspot Mantle plume Narrow conduit Source of the hotspot Point chaud Panache mantellique Conduit étroit Source du point chaud [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/doctoralThesis Theses 2020 ftinsu 2022-12-07T17:25:38Z The arrival of some plumes and the birth of hotspots at the Earth surface is more likely the cause of the break up of the Pangea ~200 Ma ago, during the jurassic era. The Gondwana was formed by many continental masses like Africa, Australia, India and Antarctic. The late cretaceous was affected by a biological crisis caused by a volcanic and/or asteroid cataclysm which provoke the disappearance of 90% of life on the Earth including dinosaurs, and produced India Deccan trapps with an area of 2 millions km^2 and thickness of 2.5-3 km. This volcanic disaster was associated with the birth of la Réunion hotspot ~65 Ma years ago, from there the india plate entered into the northward migration with a velocity of about 18-20 cm/year, and the closure of the Tethys ocean in front of the indian plate started; in the meantime the raising of basaltic lava from the indian ridges formed a new ocean floor behind the indian plate: this was the birth of indian ocean. In 1953 the Canadian researcher Tuzo Wilson suggested that such an intra-plate volcano may be due to a fixed hotspot in the mantle capable to create successive volcano on the surface; later in 1971 Jason Morgan suggested that the hotspot is fed by a mantle plume rising from the core-mantle boundary due to thermal instabilies. The goal of this thesis is to investigate the actual state of the plume in the entire indian ocean, responsible of many volcanic islands such as Maldives, Maurice and Réunion. By applying waveform inversion we are able to image the earth structure down to the lower mantle; we use Rhum-Rum data and also data collected from FDSN (Federation of Digital Seismograph Networks) data center to perfom our inversion. We perform the forward modelling with the spectral element method. For this regional case we use RegSEM (regional spectral element method) to compute synthetic seismograms that were compared to real seismograms later on. We divided the waveform into several wavepackets, each wavepacket corresponds to a specific mode. We inverted for two ... Doctoral or Postdoctoral Thesis Antarc* Antarctic Institut national des sciences de l'Univers: HAL-INSU Antarctic Indian Maurice ENVELOPE(-55.817,-55.817,-63.133,-63.133)
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language French
topic Hotspot
Mantle plume
Narrow conduit
Source of the hotspot
Point chaud
Panache mantellique
Conduit étroit
Source du point chaud
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle Hotspot
Mantle plume
Narrow conduit
Source of the hotspot
Point chaud
Panache mantellique
Conduit étroit
Source du point chaud
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Dongmo Wamba, Mathurin
Tomography of the Indian Ocean by waveform inversion
topic_facet Hotspot
Mantle plume
Narrow conduit
Source of the hotspot
Point chaud
Panache mantellique
Conduit étroit
Source du point chaud
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description The arrival of some plumes and the birth of hotspots at the Earth surface is more likely the cause of the break up of the Pangea ~200 Ma ago, during the jurassic era. The Gondwana was formed by many continental masses like Africa, Australia, India and Antarctic. The late cretaceous was affected by a biological crisis caused by a volcanic and/or asteroid cataclysm which provoke the disappearance of 90% of life on the Earth including dinosaurs, and produced India Deccan trapps with an area of 2 millions km^2 and thickness of 2.5-3 km. This volcanic disaster was associated with the birth of la Réunion hotspot ~65 Ma years ago, from there the india plate entered into the northward migration with a velocity of about 18-20 cm/year, and the closure of the Tethys ocean in front of the indian plate started; in the meantime the raising of basaltic lava from the indian ridges formed a new ocean floor behind the indian plate: this was the birth of indian ocean. In 1953 the Canadian researcher Tuzo Wilson suggested that such an intra-plate volcano may be due to a fixed hotspot in the mantle capable to create successive volcano on the surface; later in 1971 Jason Morgan suggested that the hotspot is fed by a mantle plume rising from the core-mantle boundary due to thermal instabilies. The goal of this thesis is to investigate the actual state of the plume in the entire indian ocean, responsible of many volcanic islands such as Maldives, Maurice and Réunion. By applying waveform inversion we are able to image the earth structure down to the lower mantle; we use Rhum-Rum data and also data collected from FDSN (Federation of Digital Seismograph Networks) data center to perfom our inversion. We perform the forward modelling with the spectral element method. For this regional case we use RegSEM (regional spectral element method) to compute synthetic seismograms that were compared to real seismograms later on. We divided the waveform into several wavepackets, each wavepacket corresponds to a specific mode. We inverted for two ...
author2 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)
Université Paris Cité
Jean-Paul Montagner
Barbara Romanowicz
format Doctoral or Postdoctoral Thesis
author Dongmo Wamba, Mathurin
author_facet Dongmo Wamba, Mathurin
author_sort Dongmo Wamba, Mathurin
title Tomography of the Indian Ocean by waveform inversion
title_short Tomography of the Indian Ocean by waveform inversion
title_full Tomography of the Indian Ocean by waveform inversion
title_fullStr Tomography of the Indian Ocean by waveform inversion
title_full_unstemmed Tomography of the Indian Ocean by waveform inversion
title_sort tomography of the indian ocean by waveform inversion
publisher HAL CCSD
publishDate 2020
url https://theses.hal.science/tel-03216584
https://theses.hal.science/tel-03216584/document
https://theses.hal.science/tel-03216584/file/DONGMO_WAMBA_Mathurin_va.pdf
long_lat ENVELOPE(-55.817,-55.817,-63.133,-63.133)
geographic Antarctic
Indian
Maurice
geographic_facet Antarctic
Indian
Maurice
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source https://theses.hal.science/tel-03216584
Sciences de la Terre. Université Paris Cité, 2020. Français. ⟨NNT : 2020UNIP7077⟩
op_relation NNT: 2020UNIP7077
tel-03216584
https://theses.hal.science/tel-03216584
https://theses.hal.science/tel-03216584/document
https://theses.hal.science/tel-03216584/file/DONGMO_WAMBA_Mathurin_va.pdf
op_rights info:eu-repo/semantics/OpenAccess
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