La microporosité représente jusqu'à 95% de la porosité totale des réservoirs à hydrocarbures et des aquifères dans les calcaires crétacés du Moyen-Orient. Dans ces sédiments microporeux, la porosité est modérée à excellente (jusqu'à 35%), tandis que la perméabilité est faible à modérée (jusqu'à 190mD). A l'inverse, mes faciès microporeux peuvent former des niveaux denses, avec de très faibles porosité et perméabilité (respectivement 2–8% et 0,01–2mD). Dans ce travail, les échantillons proviennent essentiellement de la Formation Mishrif (Cénomanien), mais aussi de la Formation Habshan (Berriasien/Valanginien), afin d'examiner les grandes différences verticales et latérales des propriétés pétrophysiques. Le MEB a été utilisé pour étudier deux contrôles potentiels des qualités réservoir : (1) la morphologie des particules micritiques (forme et contacts intercristallins), et (2) la cristallométrie des micrites, définie comme la taille médiane des particules mesurées sur les clichés MEB. Les données morphométriques ont été comparées avec trois paramètres pétrophysiques (porosité, perméabilité, distribution des rayons de seuil de pore). Les résultats montrent que les matrices micritiques peuvent être subdivisées en trois classes pétrophysiques. La Classe C (micrites strictement microporeuses avec des cristaux grossiers ayant des contacts punctiques à partiellement coalescents) est composée de particules grossières (>2µm), polyhédrales à arrondies. Elle présente des porosités bonnes à excellentes (8-28%), des perméabilités faibles à modérées (0,2-190mD), et des rayons de seuils de pores (PTR) moyens supérieurs à 0,5µm. Cette Classe C est généralement observée dans les shoals bioclastiques riches en rudistes, où de nombreux facteurs sédimentaires (hydrodynamisme…) peuvent défavoriser le dépôt des particules les plus fines. L'étude diagénétique montre que ces micrites grossières peuvent aussi être expliquées par une dissolution précoce des fines particules d'aragonite et de HMC dans des fluides météoriques oxydants, permettant la formation in-situ de surcroissances sur les particules de LMC au sommet de la nappe phréatique météorique. Ces processus induisent une augmentation de la taille des particules micritiques, une lithification précoce de la boue carbonatée, et donc une stabilisation minéralogique précoce des micrites grossières de la Classe C. La Classe F (micrites strictement microporeuses avec des cristaux fins ayant des contacts punctiques à partiellement coalescents, est composée de particules fines (<2µm), polyhédrales à arrondies. Elle présente des porosités bonnes à excellentes (3-35%), mais des valeurs de perméabilité souvent inférieures à 10mD, et des PTR inférieurs à 0,5µm. Cette Classe F est souvent observée dans les sédiments déposés en domaine de plate-forme interne boueuse. La formation de ces micrites fines est aussi expliquée par une stabilisation minéralogique précoce des particules micritiques dans des eaux météoriques confinées, favorisant les processus de néomorphisme, pouvant continuer au cours de l'enfouissement. Plus tard, au cours de l'enfouissement de la série, les qualités réservoirs des Classes C et F sont localement améliorées par de la dissolution mésogénétique (probablement liée à des acides organiques) affectant la matrice micritique durant la mise en charge des réservoirs. La Classe D est formée par des matrices micritiques denses, composées de cristaux anhédraux ou subhédraux avec des contacts fusionnés. Elle présente de très faibles données de porosité et de perméabilité. Ces micrites sont uniquement observées dans les niveaux de plate-forme interne et forment des intervalles inter-réservoirs, généralement en association avec des stylolites et un contenu argileux important, pouvant dépasser 10%. Quelque soit leur mode de formation, ces trois classes peuvent être incorporées dans les futures études de rock-typing portant sur les réservoirs carbonatés microporeux du Moyen-Orient / Microporosity may account for as much as 95% of the total porosity of hydrocarbon and water reservoirs in Cretaceous limestones of the Arabian Gulf. In these microporous facies porosity is moderate to excellent (up to 35%) while permeability is poor to moderate (up to 190mD). Conversely, microporous facies may form dense inter-reservoir or cap rock layers with very low porosity and permeability values (2–8% and 0.01–2mD, respectively). For this study, samples were mainly collected from the Cenomanian Mishrif Formation, but also from the Berriasian-Valanginian Habshan Formation, so as to examine the wide vertical and lateral discrepancies in their petrophysical parameters. Scanning Electron Microscopy was used to investigate two potential controls of reservoir properties: (1) micrite particle morphology (shape and inter-crystal contacts); and (2) micrite crystallometry, defined as the median size of micrite particles measured on SEM photomicrographs. The morphometric data are compared with three petrophysical parameters (porosity, permeability and pore threshold radius distribution). Results reveal that micrite matrixes can be subdivided into three petrophysical classes each with its own distinctive crystallometry, morphology and reservoir properties. Class C (strictly microporous limestones with coarse punctic-to-partially coalescent micrites) is made up of coarse (>2µm) polyhedral to rounded micritic crystals, it has good to excellent porosity (8–28%), poor to moderate permeability (0.2–190mD) and a mean pore threshold radius of more than 0.5µm. The class C is usually observed in rudist-rich bioclastic shoal facies where several sedimentary factors (hydrodynamism, bioproduction …) would disfavour deposition of the finer micritic crystals. Diagenetic study shows that the development of coarse micrites (Class C) must also be explained by the early dissolution of fine aragonite and high magnesium calcite particles in oxygenated meteoric fluids leading to a simultaneous in-situ overgrowth on LMC particles at the top of the meteoric phreatic lens. These processes induce an increase of the crystallometry of micritic particles, an early lithification of the carbonate mud, and so the mineralogical stabilization of coarse Class C micrites. Class F (strictly microporous limestones with fine punctic-to-partially coalescent micrites) is composed of fine (<2µm) polyhedral to rounded micrites with poor to excellent porosity (3–35%), but permeability values of less than 10mD and a mean pore threshold radius of less than 0.5µm. It is mostly observed in sediments deposited in a low energy muddy inner platform setting. The formation of fine micrites (Class F) is also explained by an early mineralogical stabilization of micritic particles in confined meteoric waters, favoring neomorphism processes, which may proceeds during burial. Later, during burial, reservoir properties of classes C and D strictly microporous samples where locally enhanced by mesogenetic dissolution (probably due to organic acids) affecting the microporous matrix during the oil emplacement. Class D (strictly microporous mud-dominated facies with compact anhedral to fused dense micrites) comprises subhedral to anhedral crystals with sutured to fused contacts forming a dense matrix. It has very low porosity and permeability. Class D is only found in low energy muddy inner platform facies and forms inter-reservoir or caps rock layers usually in association with stylolites and clay contents that exceed 10%. Regardless of how they formed, though, the three classes can be usefully incorporated into future rock-typing of the microporous carbonate reservoirs of the Middle East

The Precambrian-Cambrian Athel Silicilyte is an enigmatic chert unit of up to 390 m thick found as slabs (each slab typically 2 × 6 km across) entrapped within salt domes at a depth of 4-5 km in the South Oman Salt Basin. This formation is a prolific self-charged reservoir with high porosity (up to 34 %) and high oil saturation (80 %). Despite its economic value, the origin and the variability of this formation are not fully understood. This study therefore aims to investigate the variability and the origin (silica source and precipitation mechanism) of the Athel Silicilyte. Data obtained from core, wireline log and petrographical analysis were employed to establish the vertical and the lateral variability and, with the assistance of geochemical data, the likely source and precipitation mechanism of silica was determined.The Athel Silicilyte is only present in the deepest parts of the South Oman Salt Basin within the fault-bounded Athel Basin, bounded by two silt-rich mudstone units. Six lithofacies were recognised in the Athel Silicilyte that reflect variability in detrital material contents (three silica-rich facies), sediment remobilisation (slumped and brecciated lithofacies) and diagenetic modification (carbonate-bearing lithofacies), with the silica-rich facies being the most abundant (> 97 % of the total thickness). The Athel Silicilyte exhibits wavy discontinuous lamination and it is predominately (silica-rich facies average = 80 wt. %) composed of connected-networks of microcrystalline quartz (1-5 µm). Other constituent components are detrital quartz (3 wt. %), illite (10 wt. %), pyrite (4 wt. %) and organic carbon (TOC = 3 wt. %). The detrital contents increase towards the Upper Athel Silicilyte and towards the basin margins (ranging from 3 to 30 wt. %). The wavy laminations are interpreted to have a microbial origin. The homogeneity, loose packing of detrital grains and preservation of 390 m thick laminated fabric suggest that the Athel Silicilyte precipitated syndepositionally in microbial layers during low detrital input. The intense detrital input during bounding mudstones sedimentation inhibited Athel Silicilyte precipitation as a result of the rapid burial of microbial layers. The Athel Silicilyte shows strong enrichments of redox-sensitive elements (U, V and Mo), Mn-depletion, positive Ce anomalies, and small framboidal pyrites (3.6-4.0 µm), suggesting that the water column was euxinic during precipitation.Based on the petrographical evidence for the Athel Silicilyte forming as a syndepositional precipitate alongside seawater-like rare earth element (REE) characteristics, silica is interpreted to have been sourced directly from seawater. Mass balance calculations support this interpretation, indicating that silica-rich Precambrian seawater provided the significant silica mass in the Athel Silicilyte. The ability of dissolved silica to form hydrogen bonds with the functional groups (e.g. carboxyl and hydroxyl) in microbial layers was the key for Athel Silicilyte precipitation. The formation of hydrogen bonds was made possible under euxinic conditions, where the pH values were probably lower (< 7) than for the normal seawater as a result of HS- and H+ production by sulphate reducing bacteria and HS- oxidation at the redox boundary by sulphur oxidising bacteria. Consequently, dissolved silica was concentrated in microbial layer microenvironemnts, resulting in silica nucleation and polymerisation.

Le stockage géologique du CO2 et/ou la récupération assistée de pétrole par injection de CO2 dans des réservoirs pétroliers, pourraient permettre de limiter le CO2 atmosphérique. Cependant, le CO2 peut être associé à de l’oxygène. Prédire l’évolution des hydrocarbures dans ces conditions, implique d’étudier les mécanismes de l’oxydation. Des expériences d’oxydation et des modélisations cinétiques détaillées ont été réalisées avec des composés modèles purs ou en mélange. La comparaison des résultats expérimentaux et de modélisation a permis la construction d’un mécanisme d’oxydation d’hydrocarbures, et a souligné les paramètres influençant l’apparition d’une auto-inflammation. La bonne cohérence des expérimentations et des modélisations, est prometteuse pour le développement d’un outil de prédiction afin de déterminer la limite d’auto-inflammation ainsi que l’évolution de la composition des hydrocarbures, pour estimer la stabilité d’un système pétrolier en contexte d’injection de CO2 / The geological storage of CO2 (CO2 Capture-Storage – CCS) and the Enhanced Oil Recovery (EOR) by CO2 injection into petroleum reservoirs could limit CO2 atmospheric accumulation. However, CO2 can be associated with oxygen. To predict the hydrocarbon evolution under these conditions involves the study of oxidation mechanisms. Oxidation experiment and kinetic detailed modeling were carried out with pure compounds. The comparison between experimental and modeling results led to the construction of a hydrocarbon oxidation kinetic model and emphasized the parameters leading to auto ignition. The good agreement between our experiments and modeling are promising for the development of a tool predicting the critical temperature leading to auto-ignition and the evolution of hydrocarbon composition, to estimate the stability of a petroleum system in CO2 injection context

Les microbialites, dépôts lithifiés d’origine microbienne, sont des structures organosédimentaires documentées depuis plus de 3,5 milliards d’années. La compréhension de ces structures, des conditions et des modalités de leur mise en place, nous apporte des informations précieuses sur l’origine de la vie sur Terre. Cette thématique de recherche est également en plein essor du fait de ses implications économiques majeures concernant les hydrocarbures. La reconstitution des environnements associés aux structures microbiennes fossiles reste incertaine, notamment entre milieux de dépôts marins ou continentaux. Ces deux environnements contrastés ont été étudiés à travers deux exemples modernes, Cayo Coco (Cuba) en domaine marin lagunaire et le Grand Lac Salé (Utah, USA) en domaine lacustre continental dans le but d’identifier des critères diagnostiques pour discriminer ces environnements dans le registre fossile.La formation des microbialites résulte de la minéralisation et de la lithification d’un tapis microbien sous l’influence d’une composante métabolique (intrinsèque) liée à l’activité du tapis microbien, et d’une composante environnementale (extrinsèque). L’objectif de ce travail était de replacer à différentes échelles les dépôts microbiens dans leur contexte environnemental et de comprendre les influences directes des paramètres extrinsèques sur : (1) les processus de minéralisation des tapis microbiens et la formation de microbialites, (2) la morphologie des structures microbiennes, (3) la distribution spatio-temporelle des microbialites et des sédiments associés, et enfin (4) les relations entre les tapis microbiens et microbialites et leur environnement. / Lithified microbial deposits, considered as microbialites, are organosedimentary structures observed since 3.5 billion years. Understanding the mechanisms and environmental conditions leading to their formation may provide valuable information about the origin of life on Earth. Our interest on this research topic has increased owing to the economic implications of these deposits, especially concerning the hydrocarbons. The reconstruction of the environments associated with microbial structures remains uncertain in the fossil record, especially between marine and continental domains. These two contrasting environments were studied through two modern examples: (1) a marine-fed lagoon area in Cayo Coco (Cuba), and the continental lake of the Great Salt Lake (Utah, USA) in order to identify diagnostic criteria allowing to distinguish both environments in the fossil record.Microbialite result from mineralization and lithification of microbial mats under the influence of metabolic chemical reactions (intrinsic) related to the activity of the microbial biomass and environmental (extrinsic) conditions. The objective of this PhD is to replace microbial deposits, at different scales, in their context of formation to highlight the significance of extrinsic parameters on: (1) the mineralization processes and the formation of microbialites, (2) the morphologies of observed microbial structures, (3) their spatial distribution, and (4) the relationship between microbial mats and microbialite and their environment.

Ce travail de thèse s’est inséré dans la problématique du stockage de déchets radioactifs en formation argileuse profonde. Il porte en particulier sur l’étude de la fissuration hydrique induite par la désaturation et resaturation de la roche en paroi des galeries de la station expérimentale de Tournemire (Averyon, France). Cette étude a visé à identifier les déterminismes microstructuraux et minéralogiques de la fissuration hydrique des argilites de Tournemire, en couplant au laboratoire la Corrélation d’Images Numériques (CIN) et la Microscopie Electronique à Balayage (MEB). Deux échantillons d’argilite de Tournemire ont été soumis à des variations d’humidités différentes par chocs et par paliers progressifs. La CIN a permis de mettre en évidence l’influence de l’humidité et de la teneur en eau sur l’amplitude de l’ouverture des fissures et des déformations à différentes échelles. Cette étude a également permis de mettre en lumière l’influence du chargement hydrique sur l’organisation des réseaux de fractures. Une cartographie minéralogique sur un champ plurimillimétrique en haute résolution a été également mise en œuvre au MEB sur ces deux échantillons d’argilites. Cette cartographie a permis d’apporter des données qualitatives et quantitatives sur l’anisotropie microstructurale et minéralogique de la roche argileuse et de proposer une estimation de la surface élémentaire représentative du système grain/matrice pour des zones à tendance argileuse.Le couplage de la CIN avec le MEB a révélé l’importance des hétérogénéités microstructurales relatives à la proportion, taille, élongation et orientation moyennes des inclusions rigides présentes dans la matrice argileuse de la roche, sur la localisation des fissures hydriques. / This study is included in the issues of a nuclear waste storage in deep geological clay formations. It concerns the cracking phenomenon due to desaturation and saturation processes of the argillaceous medium on gallery walls of the Underground Laboratory of Tournemire (Aveyron, France). The work presented here aims to identify in laboratory the different mineralogical factors which control the cracking generated by humidity variations, coupling two methods: the Digital Image Correlation (DIC) and the Scanning Electron Microscopy (SEM).Two clay rock samples were submitted to swelling/shrinkage processes by fast bumps or gradual humidity variations. The DIC method enabled to reveal the influence of humidity and water content on crack widths and deformations intensity to different scales. This study highlighted the part of humidity variations on evolution and width of crack networks while comparing the results obtained by different conditions of humidity variations.A mineralogical map was investigated on a millimeter field with high resolution on two clay rock samples. It allowed to: quantify the microstructural anisotropy of the rock, and estimate the size of a representative elementary surface of a microstructural system composed of coarse grains and clay matrix, for argillaceous areas.The DIC-SEM approach has shown the closed relation between the location of microstructural heterogeneities such as local proportion of coarse grains and clay matrix, medium size, length ratio and orientation of coarse grains, with the position of the hydric cracks.

No description available.

Les péridotites, roches du manteau terrestre, sont instables en présence d'eau et peuvent se transformer en un minéral hydraté la serpentine, qui a la capacité remarquable de générer de l'hydrogène H2; cette réaction s'appelle la serpentinisation. Au niveau des dorsales médio-océaniques, la circulation d'eau dans ces roches conduit à la formation de larges systèmes hydrothermaux. Ils montrent différentes conditions de température et de pH des fluides, bien qu'ils conduisent tous à la formation abiotique d'H2, de méthane CH4 et possiblement d'autres hydrocarbures légers.Cette thèse est dédiée à l'étude du rôle de la composition chimique du fluide hydrothermal sur la cinétique et les mécanismes de serpentinisation des roches ultrabasiques à différentes conditions de P-T. L'interaction entre l'olivine et/ou l'orthopyroxène a été analysée avec une solution aqueuse simulant une eau de mer enrichie en aluminium et/ou en ions bicarbonates, à différents pH. Une première série d'expériences a été réalisée à 200, 340 °C et 200 MPa en lp-DAC à l'ESRF en France. Elle a permis de quantifier les paramètres cinétiques de réaction, de déterminer un effet opposé de l'aluminium sur la cinétique de ces deux minéraux et l'accélération de la réaction en conditions alcalins. Autres expériences ont été réalisée à Pamb et 80 °C en flacons de verre. Elles ont conduit, pour la première fois, à la formation de serpentine ainsi qu'à la formation d'H2 et de CH4. Ces résultats montrent qu'une chimie plus complexe du fluide hydrothermal peut avoir un impact majeur sur la cinétique de la serpentinisation pour l'accélérer et la rendre plus accessible à une échelle de temps industrielle / Peridotites, Earth's mantle rocks, are unstable in the presence of water and can be transformed into a hydrated mineral, serpentine, which has the remarkable ability to generate hydrogen H2; this reaction is called serpentinization. At the mid-ocean ridges, the circulation of water in these rocks leads to the formation of large hydrothermal systems. They show great variability of temperature and fluids’pH conditions, although they all lead to the abiotic formation of H2, methane CH4 and eventually other light hydrocarbons. This PhD thesis is dedicated to the study of the chemical composition role of the hydrothermal fluid on the kinetics and mechanisms of serpentinization of ultramafic rocks to different conditions of P-T. The interaction between olivine and/or orthopyroxene was analyzed with an aqueous solution to simulate sea water which is rich in aluminum and/or bicarbonate ions, with different pH values. A first series of experiments was carried out at 200, 340 °C and 200 MPa in lp-DAC at the ESRF in France. It was used to quantify the kinetic parameters of the reaction, to determine an opposite effect of aluminum on the kinetics these two minerals and the acceleration of the reaction under alkaline conditions. Other experiments were performed in glass bottles at Pamb and 80 °C. They led, for the first time, to the formation of serpentine, as well as to the formation of H2 and CH4. These results show that the slightly more complex chemistry of the hydrothermal fluid can have a major impact on the kinetics of serpentinization to speed and make it more accessible to industrial time scale

MSc (Applied Mathematics) / Department of Mathematics and Applied Mathematics / In this study, we develop a multiscale model of soil transmitted helminths in humans with a special reference to hookworm infection. Firstly, we develop a single scale model that comprises of five between host scale populations namely; susceptible humans, infected humans, eggs in the physical environment, noninfective worms in the physical environment and infective worms in the physical environment. Secondly, we extend the single scale model to incorporate within-host scales namely; infective larvae within-host, immature worms in small intestine, mature worm population and within-host egg population which resulted to a multiscale model. The models are analysed both numerically and analytically. The models are epidemiologically and mathematically well posed. Numerical simulation results show that there is a bidirectional relationship between the between-host and within-host scales. This is in agreement with the sensitivity analysis results, we noted that the same parameters that reduce reproductive number R0 are the same parameters that reduce the infective worms endemic equilibrium point. From the comparative effectiveness of hookworm interventions analysis results, we notice that any intervention combination that include wearing shoes controls and reduces the spread of the infection. The modelling framework developed in this study is vigorous to be applicable to other soil transmitted helminths infections / NRF

The Malaysian granitoids form the backbone of the Malay Peninsula and have long been recognized as composed of two distinct granitic provinces separated by the Bentong-Raub suture zone: <table><ol><li>Early Permian to Late Triassic Eastern Province (Indochina – East Malaya) with mainly “I-type” hornblende-bearing granitoids, associated with Cu-Au deposits, and subordinate hornblende-free pluton roof-zones hosting limited Sn-W deposits; and</li> <li>Late Triassic Main Range Province, western Malaysia (Sibumasu) with mainly “S-type” hornblende-free granitoids, associated with Sn-W deposits, and subordinate hornblende-bearing granitoids.</li></ol></table> Field observations and new geochemical data suggested that the division of the Eastern Province and Main Range granitoids using Chappell and White’s (1974) I-S classification could be problematic, as there is a large degree of overlap between the two granitic provinces in terms of lithology, mineralogy and metallogenic affinity. The Main Range granitoids are more fractionated than the hornblende-bearing Eastern Province. Although the two granitic provinces were emplaced into different continental terranes, both granitic provinces exhibit common trace element geochemistry in the enrichment of high field strength elements (HFSE) and rare earth elements (REE) compared to typical Cordilleran I-S granites. Such enrichment is interpreted as an inheritance signature from the protoliths. The Kontum massif (an analogue of Indochina lower continental crust) comprises intraplate ortho-amphibolites and para-gneisses, which could serve as two hypothetical source end-members for the Malaysian granitoids. The model suggests that the geneses of the parental magmas of the Eastern Province and the Main Range Province were related to hybridization of melts derived from protoliths, geochemically and isotopically similar to these two source end-members, but in differing proportions. The fact that the granites from the two granitic provinces are so similar compositionally and metallogenically, suggests that similar protoliths were involved in their source. The incorporation of sedimentary-sourced melt makes the Main Range granitoids transitional I/S-type in nature, but this is unlikely to be true for the less evolved Eastern Province fractionated I-type granitoids. The hybridization of igneous- and sedimentary-sourced melts, and granite fractionation promotes Sn metallogenesis in the Main Range granitic province. Previous ages were obtained using whole rock Rb-Sr and biotite K-Ar geochronology in the 1970s and 1980s, dating methods that almost certainly do not accurately represent the crystallization age of granites. New ion microprobe U-Pb zircon ages are presented that provide new temporal constraints for the Malaysian granitic magmatism. Eastern Province granitoids have U-Pb zircon ages that range from 289 to 220 Ma, while Main Range Province magmatism is constrained between 227 and 201 Ma. A progressive westward younging trend is apparent across the Eastern Province, but becomes less obvious in the Main Range Province. In addition, the U-Pb zircon analysis of the Malaysian granitoids suggests that both granitic provinces have Cambro-Ordovician and Mesoproterozoic inheritance signatures, which match the ages of the Kontum intraplate ortho-amphibolites and para-gneisses, the two source end-members of the suspected Indochina basement. Two different tectonic models have been suggested to explain the formation and the emplacement of the Malaysian granitoids. Both models involve an east-dipping subduction zone during the Early and Mid-Triassic with Palaeo-Tethys lithosphere rolling back along the Bentong-Raub suture zone to produce westward younging ages in the Eastern Province granitoids. The first model (modified after Searle et al. 2012) suggests the younger Main Range granitoids were produced by another Late Triassic – Cretaceous east-dipping (Neo-Tethyan) subduction to the west of Sibumasu, after the Sibumasu – East Malaya collision. The transitional I/S-type geochemistry of the Main Range granitoids was caused by the partial melting of the more heterogeneous Sibumasu basement. The second model (Oliver et al. 2014) suggests the younger Main Range granitoids were produced by the westward underthrusting of Indochina crust of East Malaya beneath Sibumasu along the Bentong-Raub suture zone after the continental collision. In this model, the source of the Main Range granitoids was the pre-collision I-type Eastern Province granitoids. The second model is less likely, as no geological evidence for such underthrust is found in the Malay Peninsula.

The Tibetan plateau is a vast, elevated region located in central Asia, which is underlain by the thickest crust known on Earth (up to 90 km). An outstanding question of importance to many fields within geology is how and why did the Tibetan plateau form? Models attribute the growth of the plateau to a consequence of the ongoing India-Asia continental collision, but differ in the details of how the crustal thickening was accommodated: was it by underplating of Indian lower crust or by homogeneous shortening? High-grade metamorphic rocks sampled from the region potentially hold the key to answering this question, as they contain a record of past tectonic events that can discriminate between the various proposed models. This record can be decoded by integrating field, thermobarometric and geochronological techniques, to elucidate a detailed thermotectonic understanding of a region. This methodology was applied to three case studies, each of which targeted rare tectonic windows into the mid-crust of the plateau. These regions comprise Danba in eastern Tibet, Basong Tso in south-eastern Tibet and the Western Nyainqentanglha in southern Tibet. Each case study documents previously unreported metamorphic events that have allowed original interpretations to be made regarding tectonic evolution: in Danba, all metamorphism is shown to be early Jurassic; in Basong Tso, two metamorphic belts are documented that reveal a late Triassic--early Jurassic orogenic event; and in the Western Nyainqengtanglha, Cretaceous--Neogene magmatism is shown to overprint late Triassic metamorphism. Integration of the results has enabled commentary on the large scale evolution of the Tibetan plateau from the Permian until the present day, and even hinted at its future. The results indicate that the closure of the Paleotethys played an important role in the construction of the Tibetan plateau, and suggest that homogeneous crustal thickening is not a viable model for the documented exposure levels.