Quand un fluide mouillant visqueux (comme une huile) pénètre un milieu hétérogène tel qu’une fracture, l’interface (entre l’air déplacé et l’huile) développe des corrélations à longue portée menant à une dynamique spatio-temporelle complexe. Dans cette Thèse, nous avons étudié expérimentalement et théoriquement ce processus de transport d’un fluide, appelé imbibition, dans un modèle de fracture ouverte, pertinent dans diverses situations. Notre travail a combiné une étude expérimentale détaillée, avec une analyse précise des données, basées sur des méthodes de physique statistique et non-linéaire. D’abord, la position moyenne de l'interface h(t) est étudiée lors d’expériences de montée capillaire donnant lieu à une nouvelle solution analytique pour h(t). Nous avons ensuite étudié les propriétés d’invariance d’échelle de l’interface et en particulier leur évolution pour des processus d’imbibition forcées, caractérisée par un scénario dit «super-rugueux». Enfin, nous avons étudié et quantifié la dynamique intermittente par avalanches des fronts d’imbibition à partir de l’analyse multi-échelle (spatiales et temporelles) de leurs vitesses. L'ensemble des résultats présentés dans cette Thèse propose une image très générale de la dynamique hors équilibre des fronts d’imbibition se propageant lentement dans des fractures ouvertes. La propagation latérale des fluctuations interfaciales est contrôlée par conservation de la masse locale. L'avancement de l'interface dans la direction de propagation est contrôlé par l’échelle caractéristique du désordre et la vitesse moyenne du front. / The heterogeneous structure of fractured media can lead to complex spatiotemporal fluid invasion dynamics. It thus brings forward challenging fundamental questions in the context of out-of-equilibrium dynamical systems, but also relevant to many processes of interest. The goal of the Thesis is to study the spatio-temporal dynamics of the oil-air interface between displaced air and invading oil, in imbibition through a model open fracture. The research combines exhaustive experimental work with accurate data analysis based on methods of nonlinear statistical physics. The mean postion of the interface h(t) is studied in capillary rise experiments, giving rise to a new analytical solution for h(t). The fluctuations of the interface in forced-flow experiments are analysed in the context of kinetic roughening, characterizing a super-rough scaling scenario. Finally, the burst-like dynamics is studied by analysing the local and global velocities of the front, which are widely distributed and display complex spatio-temporal correlations. We define local and global avalanches whose sizes and durations are also widely distributed, with cutoffs that diverge with the capillary number. Intermittentcy of the global signal is quantified. The ensemble of results presented in this Thesis supports a very general picture of the nonequilibrium dynamics of slowly-driven fronts in open fractures: the lateral propagation of interfacial fluctuations is controlled by local mass conservation, through the lateral correlation length; and the advancement of the interface in the direction of propagation is controlled by the characteristic extent of the disorder d and by the mean front velocity.

Les éruptions solaires sont des tempêtes de rayonnement électromagnétique, de particules relativistes et parfois de masse coronale provoquées par la libération d’énergie magnétique provenant de la couronne solaire. Si ces tempêtes atteignent l'environnement terrestre, elles peuvent poser un danger à la santé des astronautes en hautes orbites et causer des perturbations importantes sur les systèmes GPS. Dans certains cas, elles peuvent même induire des dommages aux infrastructures technologiques, dont les réseaux électriques. La prédiction des éruptions solaires est donc considérée comme un des plus importants défis de la météorologie spatiale. Par contre, à ce jour, aucune méthode présentée dans la littérature n’est capable de produire des prédictions fiables, ce qui met en évidence la nature complexe du déclenchement des éruptions solaires. Nous présentons donc dans ce mémoire une méthode alternative aux techniques statistiques habituelles, basée sur l'assimilation de données couplée avec des modèles rapides en automate cellulaire appelés modèles d'avalanche. Les modèles d'avalanche sont une simplification drastique de la physique du déclenchement des éruptions solaires. Malgré leur simplicité, ils reproduisent assez bien les statistiques à long terme de la taille des éruptions. Nous présentons dans ce mémoire des analyses empiriques de la capacité prédictive de quatre modèles: le modèle de Lu et Hamilton (LH) (Lu & Hamilton, 1991, ApJ, 412, 841-852), deux modèles à forçage déterministes (D) (Strugarek & Charbonneau, 2014, SoPh, 289(8), 2993-3015) et finalement deux modèles maximisant l'énergie libérée, appelées modèles DMC, qui sont fortement inspirés du modèle présenté par Farhang et al. (2018, ApJ, 859(1), 41). Les modèles DMC ont été développés dans le cadre de cette maîtrise et donc un chapitre de ce mémoire est dédié à leur présentation et aux analyses plus détaillées de leurs caractéristiques. Nous montrons que pour les modèles D ainsi que les modèles DMC, une mémoire existe entre les évènements simulés de grandes tailles, malgré la forte stochasticité de chacun de ces modèles. Nous présentons de plus dans ce mémoire un nouveau protocole de prédiction des éruptions solaires, utilisant l'assimilation de données couplée avec les modèles d'avalanches. Notre protocole se base sur une méthode de recuit simulé pour ajuster la condition initiale du modèle jusqu'à ce qu'elle reproduise de façon satisfaisante une série d'évènements observés. Une fois cette condition initiale optimisée produite, la simulation qui en résulte représente notre prédiction. Nous montrons dans ce mémoire le succès de notre protocole à bien assimiler une centaine d'observations synthétiques (produit par les modèles d'avalanche eux-mêmes). / Solar flares are sudden releases of electromagnetic radiation, relativistic particles and occasionally coronal mass, caused by the release of magnetic energy from the solar corona. They pose a danger to astronauts in high orbits and directly impact the Earth, including significant disturbances on GPS systems, and can even cause damage to technological infrastructures, including electrical networks. Predicting solar flares is therefore considered to be one of the most critical challenges in space weather. However, no method presented in the literature can produce reliable predictions, highlighting the complex nature of the triggering of solar flares. We, therefore, present in this thesis an alternative method to the usual statistical forecasting techniques. Our method is based on data assimilation coupled with computationally inexpensive cellular automaton models called avalanche models. Avalanche models are a drastic simplification of the physics underlying the triggering of solar flares. Despite their simplicity, they reproduce reasonably well the long-term statistics of solar flares sizes. In this thesis, we present empirical analyses of the predictive capabilities of four models: the Lu and Hamilton (LH) model (Lu & Hamilton, 1991, ApJ, 412, 841-852), two deterministic-driven (D) models (Strugarek & Charbonneau, 2014, SoPh, 289(8), 2993-3015) and finally two models using the principle of minimum energy during magnetic reconnection, called DMC models, which are strongly inspired by the models presented by Farhang et al. (2018, ApJ, 859(1), 41). The DMC models were developed during this project; therefore, a chapter of this thesis is dedicated to their presentation and more detailed analyses of their characteristics. We show that for D and DMC models, a memory exists between large simulated events, despite the high stochasticity present within each of these models. We finally present in this thesis a new protocol for predicting solar flares, using data assimilation coupled with avalanche models. Our protocol is based on a simulated annealing method to adjust the initial condition of the model until it satisfactorily reproduces a series of observed events. Once this optimal initial condition is found, the resulting simulation produces our prediction. In this thesis, we show our algorithm's success in assimilating hundreds of synthetic observations (produced by the avalanche models themselves).

Although the construction of flexible culverts involves simplicity in comparison to similar concrete structures, the complexity of the beneficial interaction between soil and steel materials requires good understanding for their composite action and performance. Current design methods have certain validity limitations with regard to applicable slopes above the structures. Given the short construction time of flexible culverts, there is an urge to explore the feasibility and the constructability of such as cost-effective structures in sloping terrain, where they may function as an avalanche protection structure for a given road, a culvert under a ski slope, or even as a protection canopy for tunnel entrances. This report compiles the efforts carried out toward gaining knowledge about the different factors that may affect the behaviour of flexible culverts in sloping environment. The report includes an extended summary of the investigation, which is mainly presented in two appended papers. The study involved numerical simulation of three case studies to investigate their performances with regard to soil loading and avalanche loads as well. The height of cover, surface slope intensity, slope stability, soil support conditions, and avalanche proximity, were studied and discussed. The study results allowed realizing the susceptibility of flexible culverts to low heights of soil cover when built in sloping terrain, which is reflected in the deformation response and the incremental change in sectional forces, especially the bending moments. It is also found that increasing the depth of soil cover may feasibly improve the structural performance under asymmetrical soil loading and avalanche loads, where it subsequently help in reducing the bending moments in the wall conduit. The presence of a flexible culvert may affect adversely the soil stability in sloping terrain and thus need to be addressed in design. Furthermore, the flexural response of a flexible culvert is directly influenced by the soil support configuration at the downhill side of the structure. In addition, the report also attempts to highlight some general guidelines about the design aspects of flexible culverts in sloping terrain, and seeks to reflect some of the findings on the design methodology for flexible culverts used in Sweden. / <p>QC 20151130</p>

No description available.

<p> A large gravel pit at East Paris exposed 14m of Pleistocene braided outwash. Large scale longitudinal bars (30 - 400m long) were developed utilising irregular topographic highs (4 - 6m) of the basal gravels as Bar Cores. These bars prograded downstream by means of larce-scale cross-strata, periodically interupted by reactivation surfaces. Contemparaneous upstream addition of material took place by the migr ation of mixed sand and gravel bed-forms on the stoss-side of the bars. The gravel supply to the avalanche face of the major bars took the form of imbricated gravels which passed from the stoss-side, through the Bar Top, onto the Bar Front. Adjacent, sandy side-channels (4 -6m deep) exhibit a fining upward fill of trough cross beds, planar lamination and ripples; and interdigitated with the gravel bars alongside. </p> <p> Aggradation of the flood plain led to the extension of the Bar Top facies over the length of the bars, and then to the development of a Shallow-braided stream facies over the whole system. The latter is recognised by its smaller (less than 1m) bar forms composed of crossbedded gravel supplied by an imbricate gravel, and numerous small, sandy channel forms. </p> <p> At West Paris another large gravel pit exposed 6m of sandier, but stratigraphically equivalent deposits. Large scale side-bar accumulations (200-300m across) of gravel developed from river bank lateral accretion deposits. The downstream progradation was by lobes of cross-stratified and imbricated gravels, alternating with sand drapes of low flow stages. Sandy Side-channels (4m deep) developed between the gravel lobes and the accreting river bank. </p> <p> The concept of braid bar growth from a pre-existing form (bar core or river bank) is in contrast to the classic theory of development from a gravel lag. The differences may be due to depth relationships of the systems, which in this case may be the effect of position on the sandur surface. </p> / Thesis / Master of Science (MSc)

Avalanches kill on average 250 people per year. Fall detection algorithms have been used to detect many different types of falls. In this work, a robust humanoid test rigwas designed and built to investigate the use of proven threshold based fall detection algorithms during skiing. A novel burial detection algorithm is used, to detect whether or not a person has been buried by snow, as this is often lethal. Data acquisition were conducted in the Swedish mountains, as well as computer simulations to further strengthen the results. This thesis shows that an IMU, in conjunction with force sensors around the chest and shoulders are sufficient to detect a fall and burial by snow. The algorithms achieve excellent results based on measurement data gathered by thetest rig. Tests were made to check the algorithm for a person gathering data. This showed that additional evaluation is needed to be applicable to live people, since skiing by the test rig is not completely representative of human skiing. / Laviner dödar i genomsnitt 250 människor per år. Fallavkänningsalgoritmer har använts för att upptäcka många olika typer av fall. I detta arbete har en robust människoliknande testrigg designats och byggts för att undersöka användningen avbevisade gränsvärdebaserade fallavkänningsalgortimer under skidåkning. En ny begravningsavkänningsalgoritm används, för att avkänna om en person har blivit begraven av snö, då det är livshotande. Datainsamling gjordes i de svenska fjällen, samt datorsimuleringar för att vidare stärka resultaten. Denna avhandling visar att en IMU, tillsammans med kraftsensorer runt bröstet och axlar är tillräckligt för att avkänna ett fall och begravning i snö. Algoritmerna producerar förträffliga resultat av baserat på mätdata samlat avtestriggen. Tester gjordes för att granska algoritmen när en person samlar data. Det visade att ytterligare undersökning krävs för applicering på levande människor, då skidåkning av testriggen inte är helt representativt av mänsklig skidåkning.

Vision has always been one of the most important cognitive tools of human beings. In this regard, the development of image sensors opens up the potential to view objects that our eyes cannot see. One of the most promising capability in some image sensors is their single-photon sensitivity that provides information at the ultimate fundamental limit of light. Time-resolved single-photon avalanche diode (SPAD) image sensors bring a new dimension as they measure the arrival time of incident photons with a precision in the order of hundred picoseconds. In addition to this characteristic, they can be fabricated in complementary metal-oxide-semiconductor (CMOS) technology enabling the integration of complex signal processing blocks at the pixel level. These unique features made CMOS SPAD sensors a prime candidate for a broad spectrum of applications. This thesis is dedicated to the optimization and characterization of quantum imagers based on the SPADs as part of the E.U. funded SUPERTWIN project to surpass the fundamental diffraction limit known as the Rayleigh limit by exploiting the spatio-temporal correlation of entangled photons. The first characterized sensor is a 32×32-pixel SPAD array, named “SuperEllen”, with in-pixel time-to-digital converters (TDC) that measure the spatial cross-correlation functions of a flux of entangled photons. Each pixel features 19.48% fill-factor (FF) in 44.64-μm pitch fabricated in a 150-nm CMOS standard technology. The sensor is fully characterized in several electro-optical experiments, in order to be used in quantum imaging measurements. Moreover, the chip is calibrated in terms of coincidence detection achieving the minimal coincidence window determined by the SPAD jitter. The second developed sensor in the context of SUPERTWIN project is a 224×272-pixel SPAD-based array called “SuperAlice”, a multi-functional image sensor fabricated in a 110-nm CMOS image sensor technology. SuperAlice can operate in multiple modes (time-resolving or photon counting or binary imaging mode). Thanks to the digital intrinsic nature of SPAD imagers, they have an inherent capability to achieve a high frame rate. However, running at high frame rate means high I/O power consumption and thus inefficient handling of the generated data, as SPAD arrays are employed for low light applications in which data are very sparse over time and space. Here, we present three zero-suppression mechanisms to increase the frame rate without adversely affecting power consumption. A row-skipping mechanism that is implemented in both SuperEllen and SuperAlice detects the absence of SPAD activity in a row to increase the duty cycle. A current-based mechanism implemented in SuperEllen ignores reading out a full frame when the number of triggered pixels is less than a user-defined value. A different zero-suppression technique is developed in the SuperAlice chip that is based on jumping through the non-zero pixels within one row. The acquisition of TDC-based SPAD imagers can be speeded up further by storing and processing events inside the chip without the need to read out all data. An on-chip histogramming architecture based on analog counters is developed in a 150-nm CMOS standard technology. The test structure is a 16-bin histogram with 9 bit depth for each bin. SPAD technology demonstrates its capability in other applications such as automotive that demands high dynamic range (HDR) imaging. We proposed two methods based on processing photon arrival times to create HDR images. The proposed methods are validated experimentally with SuperEllen obtaining &gt;130 dB dynamic range within 30 ms of integration time and can be further extended by using a timestamping mechanism with a higher resolution.

Phan (2003)等人的研究首先採用網路結構的觀點，來進行在獨占市場下的消費行為分析。本文延伸Phan等人的研究，採用多樣性的不同網路結構，特別是以「無標度網路」(scale-free)作為市場背後的網路結構，藉此來探討網路對於市場需求行為的影響。同時，為了有效地進行量化分析，我們建立了一些數學公式，以便能夠精準地比較不同網路對於需求面的影響程度，其中包含了消費者剩餘、雪崩效果和磁滯效果等。在實驗結果中，我們發現網路結構的確會影響到消費行為的表現，並且當市場規模變大時，仍存在著一些因網路不同而有的差異性。 / The economic implications of network topologies are studied via a monopolist's model of market networks originally proposed by Phan, et al. (2003). By embedding the market into a larger collection of network topologies, in particular, a class of scale-free networks, we extend the early analysis built upon a class of ring networks. To facilitate the study of the impacts of network topologies upon market demand, various measures concerning social welfare (the consumer's surplus), the avalanche effect, and the hysteresis effect, are formally established. Comparisons based on these measures show that network topologies matter, and their implied differences will remain even when the network size becomes large.

In environmental impact assessment (EIA), accident risk should be considered as one impact. However, few studies have compared assessed risk levels with documented accidents. There is thus a need for assessing accuracy of risk assessment methodologies. The aim of this study was to develop and examine a risk assessment guideline based on environmental assessment. The guideline examination was carried out along the railway and the road between Kiruna and Narvik, Northern Scandinavia. The examined hazards were avalanches, debris flows, rock falls, slush flows, torrents, moose and reindeer. Documented accidents were quantified into an accident level. For each hazard type, six sections/sites were assessed. The propensities of these hazards were analysed through environmental assessments, especially by utilising geomorphology. Then, the accident densities along the sections/sites were compared with assessed accident phase indices describing risk and hazard in both spatial and temporal dimensions. The average uncertainty factors for both the risk and the hazard indices were about 5. This implies a fairly good precision. Risk and hazard indices were also rated and compared to the accident density rates. Thereafter, railway and road information was split up as different proposal alternatives in an EIA context. The total risk for each proposal was compared with the total accident density. The risk assessment guideline proved to be cost-efficient, rapid and relatively reliable in comparing accident risk.

In environmental impact assessment (EIA), accident risk should be considered as one impact. However, few studies have compared assessed risk levels with documented accidents. There is thus a need for assessing accuracy of risk assessment methodologies. The aim of this study was to develop and examine a risk assessment guideline based on environmental assessment. The guideline examination was carried out along the railway and the road between Kiruna and Narvik, Northern Scandinavia. The examined hazards were avalanches, debris flows, rock falls, slush flows, torrents, moose and reindeer. Documented accidents were quantified into an accident level. For each hazard type, six sections/sites were assessed. The propensities of these hazards were analysed through environmental assessments, especially by utilising geomorphology. Then, the accident densities along the sections/sites were compared with assessed accident phase indices describing risk and hazard in both spatial and temporal dimensions. The average uncertainty factors for both the risk and the hazard indices were about 5. This implies a fairly good precision. Risk and hazard indices were also rated and compared to the accident density rates. Thereafter, railway and road information was split up as different proposal alternatives in an EIA context. The total risk for each proposal was compared with the total accident density. The risk assessment guideline proved to be cost-efficient, rapid and relatively reliable in comparing accident risk.