This study shows that remote sensing and GIS are powerful tools in identifying geologically induced lineaments from digitally enhanced ETM+ satellite imageries and the digital elevation model (DEM) in remote areas such as the Makran accretionary prism, southeast Iran. The presence of the conjugate shear fractures in the eastern part, along with the extensional, and the presence of reidal sets associated with the subsidiary fractures of the Minab-Zendal fault system in the western part, suggests that the structural pattern changes from pure shear to simple shear from east to the west across the prism. Moreover, the gradual increase in the value of the angle between the two conjugate shear fractures, from south (coastal Makran) to north across the prism, and the presence of high-angle north-dipping reverse faults, with few south-dipping normal faults, suggest that deformation changes from brittle, in the south, to ductile in the northern part of the prism.

Large-scale accretionary and collisional crustal orogenic architecture is studied combining structural geology, lithostratigraphy, geochronology and magmatic petrology with gravity, magnetic and seismic data. This multidisciplinary approach allows characterizing the structure and composition of the orogenic crust in two accretionary-collisional systems. The Central Asian Orogenic Belt (CAOB) constituting one third of the Asia continent and the Bohemian Massif are two Palaeozoic orogens formed by accretion followed by collision. It is proposed that the CAOB formed by successive Paleozoic accretion of oceanic and continental fragments followed by a late Palaeozoic to early Mesozoic N-S convergence of North Chinese and Siberian Cratons. The comparison between the potential fields and the geological data reveals an incorrect compartmentalization into different lithostratigraphic terranes. In contrast to geology the geophysical approach allows the analysis of the crustal structures on a complete thickness of crustal column. This thesis presents a compilation of geological data combined with unique gravity and magnetic results which are integrated into a preliminary model for the architecture of the continental crust. Conversely, an important collection of complementary data is available for the Bohemian Massif, allow more precise 3D geophysical forward modeling. In this area, geophysical data reveal the occurrence of an allochtonous lower crustal layer with a felsic composition. This indicates that the Variscan orogenic crust actually resulted from the accretion of contrasted crustal fragments.

No description available.

La transition d’un comportement séismique/instable à un comportement aséismique/stable est observée dans la partie en aval des zones sismogéniques (12-15 km de profondeur). Cette transition est supposée être contrôlée par l’activation de la plasticité de basse température du quartz à ~350°C. À cause de la grande profondeur à laquelle cette transition a lieu, le seul moyen pour étudier les processus physiques qui agissent en ces contestés, est l’étude des anciens prismes d’accrétion exhumés actuellement dans des chaines de montagnes. Le mélange tectonique de Hyuga et l’unité de Morotsuka appartiennent au prisme fossile de Shimanto et sont des unités metasédimentaires déformées à des températures peu inférieures ou égales à la limite fragile/ductile (~250 et ~340°C respectivement). Les résultats des observations de microstructures en microscopie optique et en microscopie électronique à balayage (diffraction des électrons rétrodiffusés) confirment que 1) la pression dissolution et une intense microfracturation sont les mécanismes de déformation principaux du quartz dans le mélange de Hyuga et localement l’activation de la plasticité du quartz est aussi observée; 2) dans l’unité de Morotsuka la recristallisation dynamique du quartz est pleinement active. Ces considérations indiquent que la température n’est pas le seul paramètre qui control l’activation de la plasticité du quartz, et laisse supposer la participation de l’effet adoucissant de l’eau. Avec le but de mieux comprendre le rôle de l’eau sur la rhéologie quartz, des expériences en Presse Griggs ont été menées, le matériel du départ étant de porphyroclasts de quartz (immergés dans une matrice sec) à la fois très riches en eau (provenant du mélange tectonique de Hyuga) et secs (quartz du Brésil). Ces expériences montrent l’effet très adoucissant de l’eau, qui à parité de conditions de déformation, favorise la migration de joint des grains dans le quartz de Hyuga tandis que le quartz du Brésil reste indéformé à exceptions de ses bordures extérieures. L’eau « en excès » est expulsée dans la matrice pour le quartz de Hyuga et stockée dans des bandes de cisaillement C’; l’eau incorporée par le quartz de Brésil n’est pas suffisantes pour favoriser la recristallisation dynamique. / The trasition from instable seismic to stable aseismic behaviour is observed in at the lower limit of the seismogenic zones in subduction zones (12-15 km). This transition is supposed to be controlled by the onset of quartz low grade plasticity at about 350°C. Due to inaccessibility of these geodynamic contests, the only way to study the physical processes acting at these depth are exhumed accretionary prisms exposed in mountain chains. The Hyuga tectonic mélange and the Foliated Morotsuka are metasedimentary units constituting the Shimanto accretionary prism (Japan). They were deformed at temperatures of ~250°C and ~340°C respectively, so slightly lower or equal to the temperature transition. Results by optical microscopy and EBSD reveal that 1) quartz deformation mechanisms active in Hyuga Tectonic Mélange are pressure solution and microfracturation accompanied by local quartz low grade plasticity; 2) dynamic recrystallization is totally active in quartz of the Foliated Morotsuka. These considerations allow to consider the role of water in triggering quartz plasticity especially in such water-rich contest as subduction zones. With the aim to better understand the role played by water on quartz rheology, we deformed high hydrated (from Hyuga unit) and dry (classic Brazil) quartz porphyroclasts within a quartz matrix, with the Griggs apparatus. These experiments show the weakening water effect on quartz strength. At the same deformation conditions, the high hydrated Hyuga quartz show recrystallization by grain boundary migration while the dry Brazil porphyroclasts are mostly undeformed, at exception of the outer recrystallized rims. The exceeding water expulsed from Hyuga quartz is stored in C’ shear bands in the matrix; water absorbed by dry Brazil porphyroclasts is not enough to promote dynamic recrystallization.

La mer Ionienne est une zone à la géodynamique active en raison de la convergence entre les plaques Nubie et Eurasie. Elle correspond aux derniers stades de vie d’un océan, la Téthys. De ce fait, la tectonique et la sédimentation y sont très réduites ; et les faibles flux sédimentaires permettent ainsi d’enregistrer une multiplicité de processus sédimentaires.Néanmoins, c’est une zone encore peu étudiée d’un point de vue sédimentaire, notamment sur les échelles de temps de l’ordre de la centaine de milliers d’années. Ce travail est basé sur une étude sédimentologique d’archives marines complétée par des données acoustiques (bathymétrie et multi-faisceau) issue de campagnes océanographiques du SHOM. L’analyse détaillée des faciès et des séquences sédimentaire a permis, dans un premier temps, d’établir un calendrier des risques naturels (séismes, tsunamis, volcanisme), leurs sources et leurs processus de dépôt dans le bassin pour les derniers 330 000 ans. Puis, dans un second temps, de retracer l’évolution sur les derniers 400 000 ans de la circulation et de l’oxygénation des eaux de fond dans le bassin ionien et l’influence du détroit de Sicile, et notamment de la plate-forme de Malte, sur les échanges entre les bassins occidental et oriental. L’intégration des données sédimentologiques dans un modèle géoacoustique développé par le SHOM a finalement permis de déterminer l’impact des variations sédimentaires (distribution spatiale, lithologie, stratification) sur la propagation des ondes acoustique pour différentes gammes de fréquences (300 Hz - 3000 Hz) et d’angle d’incidence (0 -90°) et d’établir une cartographie de la réponse sédimentaire du le signal acoustique. / The Ionian Sea is an active geodynamic area because of the convergence between theNubia and the Eurasia plate. It corresponds to the last stage of the Tethys ocean life. Therefore,the tectonics and the sedimentation are much reduced; and the low sedimentary supply enables torecord a multiplicity of sedimentary processes. Nevertheless, this area still poorly studied from asedimentary point of view, in particular on timescales on the order of hundred thousand years.This work is based on a sedimentological study of marine archives supplemented by acoustic data(bathymetry and multibeam imagery) recovered during oceanographic campaign leaded by theSHOM. The detailed sedimentary analysis of facies and sequences allows, at first, to established acalendar of the natural hazard (earthquakes, tsunamis, volcanism), their origins and theirdepositional processes into the basin over the last 330 000 years. Then, secondly, to reconstructthe evolution over the last 400 000 years of the circulation and the oxygenation of bottom waterthrough the Ionian basin and the influence of the strait of Sicily, in particular of the Malta Plateau,on the exchanges between the western and the eastern basins. The integration of thesedimentological data in a geoacoustic modelling developed by the SHOM finally allowed todetermine the impact of the sedimentary variability (special distribution, lithology, stratification)on the acoustic waves propagation for various frequency bands (300 Hz - 3000 Hz) and incidentangle (0 - 90°) and to established a mapping of the sedimentary answer of the acoustic signal.

L’architecture crustale d’orogènes d’accrétion et de collision à grande échelle est étudiée en combinant géologie structurale, litho-stratigraphie, géochronologie et pétrologie magmatique avec les données gravimétriques, magnétiques et sismiques. Cette approche pluridisciplinaire permet de caractériser la structure et la composition de la croûte orogénique dans deux systèmes d’accrétion-collision : la Ceinture Orogénique d’Asie Centrale (CAOC) et le Massif de Bohême. La CAOC représente près d’un tiers du continent asiatique actuel. Ce système orogénique s’est construit par une accrétion continue de matériel depuis le Paléozoïque jusqu’au début du Mésozoïque, suivie par une collision durant le Mésozoïque. La comparaison des champs de potentiels avec les données géologiques met en évidence une compartimentation erronée de l’orogène en unités litho-stratigraphiques. Par rapport à la géologie, la géophysique permet une analyse directe des structures de la croûte orogénique sur toute son épaisseur. Le travail de thèse présente une compilation de données géologiques et de traitements gravimétriques et magnétiques inédits, dont la modélisation préliminaire pour contraindre l’architecture de la croûte continentale est proposée. Le Massif de Bohême possède quant à lui un catalogue de données complémentaires plus conséquent, ce qui permet une modélisation géophysique 3D plus précise. Dans cette zone, les données géophysiques mettent en évidence l’existence d’une croûte inférieure allochtone de composition felsique. Ceci indique que la croûte orogénique hercynienne est également le résultat d’une accrétion de portions crustales contrastées. / Large-scale accretionary and collisional crustal orogenic architecture is studied combining structural geology, lithostratigraphy, geochronology and magmatic petrology with gravity, magnetic and seismic data. This multidisciplinary approach allows characterizing the structure and composition of the orogenic crust in two accretionary-collisional systems. The Central Asian Orogenic Belt (CAOB) constituting one third of the Asia continent and the Bohemian Massif are two Palaeozoic orogens formed by accretion followed by collision. It is proposed that the CAOB formed by successive Paleozoic accretion of oceanic and continental fragments followed by a late Palaeozoic to early Mesozoic N-S convergence of North Chinese and Siberian Cratons. The comparison between the potential fields and the geological data reveals an incorrect compartmentalization into different lithostratigraphic terranes. In contrast to geology the geophysical approach allows the analysis of the crustal structures on a complete thickness of crustal column. This thesis presents a compilation of geological data combined with unique gravity and magnetic results which are integrated into a preliminary model for the architecture of the continental crust. Conversely, an important collection of complementary data is available for the Bohemian Massif, allow more precise 3D geophysical forward modeling. In this area, geophysical data reveal the occurrence of an allochtonous lower crustal layer with a felsic composition. This indicates that the Variscan orogenic crust actually resulted from the accretion of contrasted crustal fragments.

Impaktite des Chicxulubkraters wurden petrographisch (Polarisationsmikroskopie, REM, KL) und chemisch (RFA, TRFA, PGE, EMS) untersucht, um das Verhalten von Ejekta während des atmosphärischen Transports zu erforschen. Die proximalen Impaktite der UNAM-7 Bohrung bestehen aus einer suevitischen Brekzie (222.2 bis 384.4 m) und einer basalen, polymikten Brekzie mit geringem Silikatschmelzanteil. Letztere beinhaltet Evaporit-Megablöcke und Karbonatschmelzpartikel; Zersetzung von Kalzit und Anhydrit ist durch Entgasungsbläschen indiziert. An der distalen Kreide-Paläogen Grenze von El Guayal (520 km SW vom Kraterzentrum) beinhaltet eine 10 m mächtige suevitische Abfolge in einer oberen Untereinheit akkretionäre Lapilli und darüber eine Toneinheit. Das Auftreten von Karbonatschmelzen mit der PGE-angereicherten Impaktorkomponente in der Toneinheit belegt den Zusammenhang der K-P Grenze mit dem Chicxulub-Impakt. Die folgenden Stadien können für die Ablagerung und Alteration der Ejekta unterschieden werden: (1) Ein Hochgeschwindigkeitsauswurf beschleunigte Zersetzungsprodukte und initiierte einen Gasstrom. (2) Karbonatschmelzen wurden mit Anhydrit-Megablöcken ausgeworfen und initiierten einen lateral ausbreitenden Ejektavorhang. Kalzitrückreaktionen erhitzte das Material während des Transports. (3) Die Ejektionswolke kollabierte teilweise, wobei der zurückfallende Suevit vom Impaktormaterial, das in die Stratosphäre verteilt wurde, fraktioniert wurde. Die Kombination von Silikatschmelze mit Kalzit initiierte einen heißen, gas-angetriebenen Strom. In einer oberen, moderat temperierten, turbulenten Aschewolke kondensierte Wasserdampf, und durch Akkretion von Asche entstanden akkretionäre Lapilli. (4) Die Impaktorkomponente wurde mit den feinsten Ejektamassen für Wochen bis Jahre abgelagert. (5) Der Transport von Ejekta in der heißen Ejektionswolke induzierte Alterationsprozesse in den Ablagerungen. Es kann geschlussfolgert werden, dass ein gewisser Anteil des CO2 zu Kalzit zurückreagierte, währenddessen SOX Gase vollständig in die Atmosphäre freigesetzt wurden. Diese Beobachtungen inklusive des Auftretens von Karbonatschmelzen unterstützen die Aussage, dass der freigesetzte Anteil von CO2 in die Atmosphäre in der Vergangenheit überbewertet wurde. / Impactites of the Chicxulub crater were studied petrographically (polarisation microscopy, SEM, CL) and chemically (XRF, TXRF, PGE, EMPA) to investigate the evolution of ejecta during transit through the atmosphere. At the proximal UNAM-7 borehole, the sequence of impactites consists of a suevitic breccia (222.2 to 348.4 m) on top of a polymict silicate melt-poor breccia. The latter is intercalated with evaporite megablocks representing an analogue to the Bunte Breccia of the Nördlinger Ries crater. It contains carbonate melt particles; calcite and anhydrite decomposition is indicated by degassing vesicles. At the distal Cretaceous-Palaeogene site of El Guayal (~520 km SW of the crater centre), a ~10 m thick suevitic succession contains at its upper subunit accretionary lapilli and on top a clay unit. Intermixing of calcite with hot silicate melt resulted in recrystallisation and decomposition of calcite. In the clay unit, the presence of carbonate melt spheroids together with the PGE-enriched impactor component links the Chicxulub impact with the K-P boundary. The following stages can be distinguished for the deposition and alteration of the ejecta: (1) Jetting accelerated decomposition products and initiated a vapour flow. (2) Carbonate melts were excavated with anhydrite megablocks and initiated a lateral extending ejecta curtain. Calcite reformations heated the material during transport. (3) The expanding ejecta plume partially collapsed separating the falling suevite from impactor material that had been lifted into the stratosphere. The combination of silicate melt with calcite initiated a hot, gas-driven, basal flow. In an upper, moderately tempered, turbulent ash cloud, steam condensed and accretion of ash-sized material formed accretionary lapilli. (4) The impactor component was deposited with the finest ejecta for weeks to years. (5) The prolonged transport of ejecta in the hot ejecta plume induced alteration processes observed in the deposits. It can be concluded that a certain amount of CO2 has back-reacted to calcite, whereas SOX gases were completely liberated. These observations including the abundant presence of carbonate melts support that the amount of CO2 released to the atmosphere during the Chicxulub impact was overestimated previously.

The steep forearc slope along the northern sector of the obliquely convergent Hikurangi subduction zone is characteristic of non-accretionary and tectonically eroding continental margins, with reduced sediment supply in the trench relative to further south, and the presence of seamount relief on the Hikurangi Plateau. These seamounts influence the subduction process and the structurally-driven geomorphic development of the over-riding margin of the Australian Plate frontal wedge. The Poverty Indentation represents an unusual, especially challenging and therefore exciting location to investigate the tectonic and eustatic effects on this sedimentary system because of: (i) the geometry and obliquity of the subducting seamounts; (ii) the influence of multiple repeated seamount impacts; (iii) the effects of structurally-driven over-steeping and associated widespread occurrence of gravitational collapse and mass movements; and (iv) the development of a large canyon system down the axis of the indentation. High quality bathymetric and backscatter images of the Poverty Indentation submarine re-entrant across the northern part of the Hikurangi margin were obtained by scientists from the National Institute of Water and Atmospheric Research (NIWA) (Lewis, 2001) using a SIMRAD EM300 multibeam swath-mapping system, hull-mounted on NIWA’s research vessel Tangaroa. The entire accretionary slope of the re-entrant was mapped, at depths ranging from 100 to 3500 metres. The level of seafloor morphologic resolution is comparable with some of the most detailed Digital Elevation Maps (DEM) onshore. The detailed digital swath images are complemented by the availability of excellent high-quality processed multi-channel seismic reflection data, single channel high-resolution 3.5 kHz seismic reflection data, as well as core samples. Combined, these data support this study of the complex interactions of tectonic deformation with slope sedimentary processes and slope submarine geomorphic evolution at a convergent margin. The origin of the Poverty Indentation, on the inboard trench-slope at the transition from the northern to central sectors of the Hikurangi margin, is attributed to multiple seamount impacts over the last c. 2 Myr period. This has been accompanied by canyon incision, thrust fault propagation into the trench fill, and numerous large-scale gravitational collapse structures with multiple debris flow and avalanche deposits ranging in down-slope length from a few hundred metres to more than 40 km. The indentation is directly offshore of the Waipaoa River which is currently estimated to have a high sediment yield into the marine system. The indentation is recognised as the “Sink” for sediments derived from the Waipaoa River catchment, one of two target river systems chosen for the US National Science Foundation (NSF)-funded MARGINS “Source-to-Sink” initiative. The Poverty Canyon stretches 70 km from the continental shelf edge directly offshore from the Waipaoa to the trench floor, incising into the axis of the indentation. The sediment delivered to the margin from the Waipaoa catchment and elsewhere during sea-level high-stands, including the Holocene, has remained largely trapped in a large depocentre on the Poverty shelf, while during low-stand cycles, sediment bypassed the shelf to develop a prograding clinoform sequence out onto the upper slope. The formation of the indentation and the development of the upper branches of the Poverty Canyon system have led to the progressive removal of a substantial part of this prograding wedge by mass movements and gully incision. Sediment has also accumulated in the head of the Poverty Canyon and episodic mass flows contribute significantly to continued modification of the indentation by driving canyon incision and triggering instability in the adjacent slopes. Prograding clinoforms lying seaward of active faults beneath the shelf, and overlying a buried inactive thrust system beneath the upper slope, reveal a history of deformation accompanied by the creation of accommodation space. There is some more recent activity on shelf faults (i.e. Lachlan Fault) and at the transition into the lower margin, but reduced (~2 %) or no evidence of recent deformation for the majority of the upper to mid-slope. This is in contrast to current activity (approximately 24 to 47% shortening) across the lower slope and frontal wedge regions of the indentation. The middle to lower Poverty Canyon represents a structural transition zone within the indentation coincident with the indentation axis. The lower to mid-slope south of the canyon conforms more closely to a classic accretionary slope deformation style with a series of east-facing thrust-propagated asymmetric anticlines separated by early-stage slope basins. North of the canyon system, sediment starvation and seamount impact has resulted in frontal tectonic erosion associated with the development of an over-steepened lower to mid-slope margin, fault reactivation and structural inversion and over-printing. Evidence points to at least three main seamount subduction events within the Poverty Indentation, each with different margin responses: i) older substantial seamount impact that drove the first-order perturbation in the margin, since approximately ~1-2 Ma ii) subducted seamount(s) now beneath Pantin and Paritu Ridge complexes, initially impacting on the margin approximately ~0.5 Ma, and iii) incipient seamount subduction of the Puke Seamount at the current deformation front. The overall geometry and geomorphology of the wider indentation appears to conform to the geometry accompanying the structure observed in sandbox models after the seamount has passed completely through the deformation front. The main morphological features correlating with sandbox models include: i) the axial re-entrant down which the Poverty Canyon now incises; ii) the re-establishment of an accretionary wedge to the south of the indentation axis, accompanied by out-stepping, deformation front propagation into the trench fill sequence, particularly towards the mouth of the canyon; iii) the linear north margin of the indentation with respect to the more arcuate shape of the southern accretionary wedge; and, iv) the set of faults cutting obliquely across the deformation front near the mouth of the canyon. Many of the observed structural and geomorphic features of the Poverty Indentation also correlate well both with other sediment-rich convergent margins where seamount subduction is prevalent particularly the Nankai and Sumatra margins, and the sediment-starved Costa Rican margin. While submarine canyon systems are certainly present on other convergent margins undergoing seamount subduction there appears to be no other documented shelf to trench extending canyon system developing in the axis of such a re-entrant, as is dominating the Poverty Indentation. Ongoing modification of the Indentation appears to be driven by: i) continued smaller seamount impacts at the deformation front, and currently subducting beneath the mid-lower slope, ii) low and high sea-level stands accompanied by variations on sediment flux from the continental shelf, iii) over-steepening of the deformation front and mass movement, particularly from the shelf edge and upper slope.