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<dc:title xml:lang="fr">Étude des anomalies magnétiques dans les domaines de manteau exhumé : apport sur les processus de l’océanisation</dc:title>
<dcterms:alternative xml:lang="en">Exhumed mantle at ultra-slow spreading ridges and magma-poor rifted margins : what can we learn from marine magnetic anomalies ?</dcterms:alternative>
<dc:subject xml:lang="fr">Anomalie magnétique</dc:subject>
<dc:subject xml:lang="fr">Péridotite serpentinisée</dc:subject>
<dc:subject xml:lang="fr">Dorsale océanique</dc:subject>
<dc:subject xml:lang="fr">Marge passive</dc:subject>
<dc:subject xml:lang="en">Magnetic anomaly</dc:subject>
<dc:subject xml:lang="en">Serpentinized peridotite</dc:subject>
<dc:subject xml:lang="en">Mid-oceanic ridge</dc:subject>
<dc:subject xml:lang="en">Rifted margin</dc:subject>
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<tef:elementdEntree autoriteExterne="027842371" autoriteSource="Sudoc">Terre -- Manteau</tef:elementdEntree>
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<tef:elementdEntree autoriteExterne="032180721" autoriteSource="Sudoc">Croûte océanique</tef:elementdEntree>
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<dcterms:abstract xml:lang="fr">L’objectif de cette thèse est de comprendre (1) si l’exhumation des roches mantelliques aux dorsales océaniques est compatible avec l’enregistrement des inversions de polarité du champ magnétique terrestre, (2) quels sont les processus associés aux anomalies magnétiques observées à l’aplomb des transitions océan-continent et (3) quelles sont les conséquences de ces processus sur les mécanismes de l’océanisation. Afin de travailler avec des données de résolution maximum, une méthode de calibration et d’interprétation des données magnétiques acquises proches du fond est développée dans le premier chapitre. Dans le deuxième chapitre, cette méthode est appliquée aux données magnétiques acquises à l’aplomb des domaines de manteau exhumé de la dorsale Sud-Ouest Indienne (SWIR). Il est ensuite montré que l’exhumation des roches mantelliques est associée à un signal magnétique de faible amplitude et de faible continuité spatiale rendant impossible l’identification des anomalies magnétiques d’accrétion océanique. De fait, il est proposé que contrairement aux basaltes, les roches mantelliques exhumées de la SWIR ne portent pas une aimantation rémanente suffisamment stable pour fossiliser la direction du champ magnétique terrestre. Dans le dernier chapitre, il est démontré que l’anomalie « J », antérieurement interprétée comme la première isochrone associée à la partie distale des marges Ibérie/Terre-Neuve, est en fait identifiée à l’aplomb d’une structure crustale particulière caractérisée par un haut topographique et un épaississement crustal. Par conséquent, il est proposé qu’un évènement magmatique majeur est à l’origine de la création de cette structure crustale et que cet événement est le déclencheur de la mise en place de la première dorsale océanique.</dcterms:abstract>
<dcterms:abstract xml:lang="en">The aim of this work is to constrain (1) whether exhumation of mantle rocks at mid oceanic ridges is compatible with the record of polarity reversals of the Earth magnetic field, (2) what is the origin and the processes responsible for the magnetic anomalies observed at magma-poor rifted margins and (3) what are the consequences of these processes on continental breakup. In a first part, in order to work with high-resolution data, we develop a method for calibration and interpretation of deep-tow three component magnetic data. In a second part, we apply these methods to the data acquired above the large exhumed mantle domains of the ultraslow-spreading Southwest Indian Ridge. We show that, in these areas, neither the magnetic properties of the dredge samples nor the deep-tow magnetic data are consistent with the seafloor-spreading magnetic pattern commonly observed at mid oceanic ridges. We further suggest that in contrast to mid oceanic ridges basalts the exhumed serpentinized mantle rocks do not carry a sufficiently stable remanant magnetization to produce marine magnetic anomalies. In the last part, we show that the “J” anomaly, previously interpreted as the first seafloor-spreading anomaly of the Iberia and Newfoundland passive margins, is associated with locally high topography and thickened crust. We propose that this peculiar crustal structure results from voluminous magma both erupted at the surface and added beneath the exhumed mantle domain. We therefore propose that the J anomaly did not form during seafloor spreading but instead represents a pulse of magmatism that have triggered continental breakup.</dcterms:abstract>
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