Altération de la régénération musculaire dans la maladie pulmonaire obstructive chronique

Altération de la régénération musculaire dans la maladie pulmonaire obstructive chronique. La maladie pulmonaire obstructive chronique (MPOC) est caractérisée par une obstruction bronchique irréversible et progressive. L’atrophie musculaire périphérique y est fréquente et a un impact négatif sur la capacité fonctionnelle et la survie des sujets atteints. Toutefois, on ignore si une altération du processus de régénération musculaire est un processus ayant cours dans l’atrophie musculaire périphérique. Le but de la présente thèse était donc d’étudier les cellules satellites, principales cellules responsables de la régénération musculaire dans les muscles périphériques de patients ayant une MPOC. Dans un premier temps, nous avons évalué l’historique de réplication du tissu musculaire et la sénescence des cellules satellites. Les changements morphologiques ayant lieu dans le muscle au cours de la progression de la maladie rendent le muscle plus susceptible aux dommages, induisant un raccourcissement prématuré des télomères. Un raccourcissement des télomères chez les sujets ayant une MPOC avec atrophie est concomitant avec une augmentation du nombre de cellules satellites sénescentes et de l’épuisement du potentiel de régénération compromettant le maintien de la masse musculaire chez ces sujets. Dans un deuxième et troisième temps, nous avons étudié les étapes amenant une cellule satellite vers une cellule musculaire dans les muscles périphériques et respiratoires de patients ayant une MPOC comparativement à des sujets contrôles. Les cellules satellites sont impliquées dans la réparation du tissu musculaire. Dans les cellules satellites provenant des sujets ayant une MPOC, une altération de la prolifération et de la différentiation a été observée. Ces résultats sont compatibles avec une altération de la régénération musculaire pouvant conduire à l’atrophie musculaire dans la MPOC. Le quatrième volet de ce projet s’intéressait à l’impact d’un entraînement en résistance sur l’activité des cellules satellites et le rôle joué par la myostatine dans ce contexte. La littérature montre que l’exercice en résistance est bien toléré et aide les patients ayant une MPOC à retrouver une meilleure qualité de vie. Cependant, il semble qu’ils n’y répondent pas tous aussi bien que les sujets contrôles. La capacité de réponse des cellules satellites à un entraînement en résistance semble inadéquate, suggérant ainsi un défaut de leur activation. Dans la dernière étude de cette thèse, nous avons voulu évaluer l’impact de l’inflammation systémique en étudiant SAA1, une protéine de phase aiguë et p21, une protéine du cycle cellulaire dans la dégradation des protéines des cellules musculaires. Les liens de causalité entre l’affection primaire et les différentes comorbidités demeurent nébuleux dans la MPOC. SAA1 et p21 sont augmentés dans les muscles squelettiques des patients ayant une MPOC et par ailleurs, SAA1 est capable d’induire la dégradation des protéines musculaires. Cette thèse expose les premiers éléments impliquant l’altération de la régénération musculaire avec la dysfonction musculaire observée chez les patients ayant une MPOC. Ces résultats vont certainement contribuer au développement de nouvelles thérapies et stratégies d’intervention dans le but d’améliorer la qualité de vie des personnes atteintes d’une MPOC. En somme, les travaux effectués dans le cadre de la présente thèse montrent que plusieurs mécanismes agissent de concert avec l’inactivité physique afin d’induire le phénotype dysfonctionnel dans les muscles des patients ayant une MPOC.

O potencial energético do gradiente térmico na plataforma continental do sul do brasil

O crescimento da demanda energética, prevista para a metade do século XXI, com números embasados no crescimento demográfico e de consumo dos países em desenvol- vimento, sugere a busca por fontes energéticas renováveis e de menor impacto ao meio ambiente, conforme os tratados da política internacional. Portanto, o fornecimento de energia suplementar se torna vital nas sociedades modernas e sua extensão até o mar tem se constituído uma recente preocupação do ponto de vista enérgico e ecológico. Várias formas de conversão de energia foram desenvolvidas no decorrer dos anos, com destaque para a energia dos gradientes térmicos. A Plataforma Continental Sul do Bra- sil (PSCB) possui alta variabilidade espacial e temporal nos campos de temperatura, de forma que existe a necessidade de uma análise das regiões de maior potencial energético com respeito ao gradiente vertical de temperatura. Neste estudo, foram utilizados dados do modelo OCCAM com uma grade de resolu- ção horizontal de 0, 25o e resolução vertical de 66 níveis, distribuídos ao longo de um sistema de coordenadas vertical. Foram utilizadas imagens de temperatura superfícial do mar (TSM) obtidas a partir do sensor AVHRR (Advanced Very High Resolution Ra- diometer) de forma a realizar a validação dos dados do modelo OCCAM. A análise da média dos dados do modelo indicou um sítio energético de maior viabilidade devido oC ao padrão médio do gradiente térmico de aproximadamente 0, 17 ao longo da coluna vertical (545 m de profundidade) no oceano. Neste local, foram coletados os dados, e aplicados a um módulo de conversão de energia térmica dos oceanos que vem sendo desenvolvido na Universidade Federal do Rio Grande - FURG. A região de estudo de- monstrou possuir um local com ótimo potencial energético, onde a produção máxima de energia pode alcançar 111, 9MW , associada com um padrão variabilidade tempo- ral dominante de 12 meses. Este sítio energético demonstra maior eficiência durante o período de verão e outono ao longo dos anos e sua média para todo o período é de 94, 3MW . Neste estudo, duas correntes: Corrente do Brasil (CB) e a Contra Corrente Costeira (CCC), com águas de origem tropical e subantártica com aportes continentais, respecti- vamente, tem alta correlação com os valores dos gradientes térmicos e com os significa- tivos eventos de conversão energética. O sítio energético demonstrou alta estabilidade à sazonalidade e à gama de eventos meteorológicos e oceanográficos, de forma que pode ser qualificado como uma fonte suplementar a matriz energética do país para um futuro próximo.

Reduction of the “ngege”, Oreochromis esculentus (Teleostei: Cichlidae) populations, and resultant population genetic status in the Lake Victoria region

Ngege, Oreochromis esculentus, originally formed the mainstay of the Lake Victoria Region (LVR) fisheries. Together with its indigenous congener O. variabilis, it was displaced from Lakes Victoria and Kyoga of LVR and was found to survive as isolated small populations within the peripheral minor lakes and reservoirs around the two lakes. Displacement of the two LVR indigenous tilapiines was thought to be principally driven by changed lake environment and predation by the introduced Nile perch, but also competition and genetic swamping by the closely related introduced and comparatively more ecologically versatile tilapine species. In a study carried out in the LVR between 1993 and 2003, micro satellites and RAPD markers were used to analyse the remnant populations so as to establish the population structure and extant genetic diversity of O. esculentus. Analyses indicated that the surviving O. esculentus retained a high proportion of genetic diversity with high differentiation between units an indication of genetic exchange between indigenous and introduced Nile tilapia where the two forms co-existed. While this heightened concern for genetic swamping of the remnant population units by the introduced tilapiines it was noteworthy that in a few of the satellite lakes where the O. esculentus was dominant evidence for introgression was weak.

Use of satellite observations for operational oceanography: recent achievements and future prospects

The paper gives an overview of the development of satellite oceanography over the past five years focusing on the most relevant issues for operational oceanography. Satellites provide key essential variables to constrain ocean models and/or serve downstream applications. New and improved satellite data sets have been developed and have directly improved the quality of operational products. The status of the satellite constellation for the last five years was, however, not optimal. Review of future missions shows clear progress and new research and development missions with a potentially large impact for operational oceanography should be demonstrated. Improvement of data assimilation techniques and developing synergetic use of high resolution satellite observations are important future priorities.

Fibre components and systems for mid-IR applications

Fibre-optic components and systems are used in a wide variety of industrial, medical and communication applications and can be found in use everywhere in the modern world, from the bottom of the ocean to satellites in orbit. The field of fibre optics has seen rapid growth in the past few decades to become an essential enabling technology. However, much more work is needed to develop components and systems that can work at wavelengths in the short-wavelength infrared (SWIR) / mid-IR part of the spectrum (defined in this work as 1.5 – 4.5.

Commande optimale d'un satellite à propulsion électrique utilisant les perturbations pour l'élimination des débris orbitaux en basse altitude

Depuis le lancement du premier satellite Spoutnik 1 en 1957, l’environnement spatial est de plus en plus utilisé et le nombre de débris orbitaux se multiplie naturellement, soit par des explosions, des collisions ou tout simplement par les opérations normales des satellites. Au-delà d'un certain seuil, la densité des débris orbitaux risque de créer une réaction en chaîne incontrôlée : l’effet Kessler. L’élimination des débris orbitaux en basse altitude permettrait de limiter cette réaction et ainsi de préserver l’environnement spatial afin de pouvoir l’utiliser de façon sécuritaire. L’élimination des débris orbitaux est une opération complexe et coûteuse. Elle consiste à déplacer des objets spatiaux inactifs vers une orbite basse pour mener à leur désintégration dans la basse atmosphère terrestre. En utilisant les perturbations orbitales, il est possible de réduire le coût du carburant requis pour effectuer les manœuvres orbitales nécessaires à l’élimination de ces débris. L'objectif principal de cette étude consiste à développer une procédure et une stratégie de commande autonome afin de modifier l'orbite des satellites non opérationnels (débris) pour mener à leur désintégration naturelle tout en optimisant les facteurs carburant et temps. Pour ce faire, un modèle d’atmosphère basé sur le modèle de Jacchia (1977) est développé. Un modèle de la dynamique du satellite inclut aussi les perturbations principales, soit : traînée atmosphérique, non sphéricité et distribution non uniforme de la masse de la Terre. Ces modèles ainsi qu'un algorithme de commande optimale pour un propulseur électrique sont développés et le tout est validé par simulations numériques sur Matlab/Simulink. Au terme de cette étude, les conditions optimales dans lesquelles il faut laisser un débris afin qu'il se désintègre dans la basse atmosphère de la Terre en quelques semaines seront données (type d'orbite : altitude, inclinaison, etc.) ainsi que le coût en carburant pour une telle mission. Cette étude permettra de prouver qu'il est possible de réaliser des missions d'élimination des débris orbitaux tout en réduisant les coûts associés aux manœuvres orbitales par l'utilisation des perturbations naturelles de l'environnement.

Influence de la rigidité du microenvironnement sur les cellules progénitrices myogéniques du muscle squelettique

La matrice extracellulaire (MEC) subit plusieurs modifications au cours du vieillissement, ce qui altère ses propriétés biomécaniques. Les cellules responsables de la régénération de la portion myogénique du muscle sont les cellules satellites, qui, une fois activées, sont appelées les cellules progénitrices myogéniques (CPM). La rigidité du muscle, influence le devenir des CPM. La capacité régénérative du muscle squelettique diminue lors du vieillissement. Nous avons posé l’hypothèse selon laquelle la rigidité observée dans le tissu âgé pourrait nuire à la capacité régénérative des CPM. Nous avons tout d’abord validé les modifications subies par la MEC suite au vieillissement en les comparant au tissu adulte. Les résultats montrent une augmentation de la quantité de collagènes et de réticulation non enzymatique. En plus, une augmentation de la rigidité du muscle et des fibres individualisées a été observée par microscopie à force atomique (AFM). L’équipe s’est ensuite intéressée à leur activité myogénique dans un modèle de fibres musculaires en culture (ex vivo). Nous avons observé une diminution du nombre de cellules myogéniques sur les fibres de tissus âgés, comparativement aux tissus adultes. Nous avons montré que les proportions de cellules quiescentes sont plus élevées sur des fibres adultes suite à l’isolement et que les proportions de cellules prolifératives et en voie de différenciation sont plus élevées sur les fibres âgées. De plus, sur des fibres endommagées gardées en culture six jours, nous avons observé que les proportions de cellules prolifératives sont plus élevées sur les fibres adultes et que celles des cellules en voie de différenciation sont plus élevées sur les fibres âgées. Enfin, nous avons observé l’activité myogénique des CPM ainsi que l’impact de la rigidité en culture (in vitro). Nous n’avons observé aucune différence des capacités de prolifération et de différenciation des myoblastes adultes et âgés. En terminant, nos recherches ont montré qu’une rigidité de 2.0 kPa favorise un état prolifératif tandis qu’une rigidité de 18 kPa stimule plutôt l’engagement vers la différenciation. Ces résultats suggèrent que la rigidité peut être une cause de la diminution du potentiel régénératif du muscle vieillissant. En résumé, ces travaux soulignent l’importance de l’augmentation de la rigidité du microenvironnement sur les CPM comme cause de la diminution du potentiel de régénération du muscle vieillissant.

Comparison and validation of physical wave parameterizations in spectral wave models

Recent developments in the physical parameterizations available in spectral wave models have already been validated, but there is little information on their relative performance especially with focus on the higher order spectral moments and wave partitions. This study concentrates on documenting their strengths and limitations using satellite measurements, buoy spectra, and a comparison between the different models. It is confirmed that all models perform well in terms of significant wave heights; however higher-order moments have larger errors. The partition wave quantities perform well in terms of direction and frequency but the magnitude and directional spread typically have larger discrepancies. The high-frequency tail is examined through the mean square slope using satellites and buoys. From this analysis it is clear that some models behave better than the others, suggesting their parameterizations match the physical processes reasonably well. However none of the models are entirely satisfactory, pointing to poorly constrained parameterizations or missing physical processes. The major space-time differences between the models are related to the swell field stressing the importance of describing its evolution. An example swell field confirms the wave heights can be notably different between model configurations while the directional distributions remain similar. It is clear that all models have difficulty in describing the directional spread. Therefore, knowledge of the source term directional distributions is paramount in improving the wave model physics in the future.

Low temperature magneto-photoluminescence characterization of high purity gallium arsenide and indium phosphide

Low-temperature magneto-photoluminescence is a very powerful technique to characterize high purity GaAs and InP grown by various epitaxial techniques. These III-V compound semiconductor materials are used in a wide variety of electronic, optoelectronic and microwave devices. The large binding energy differences of acceptors in GaAs and InP make possible the identification of those impurities by low-temperature photoluminescence without the use of any magnetic field. However, the sensitivity and resolution provided by this technique rema1ns inadequate to resolve the minute binding energy differences of donors in GaAs and InP. To achieve higher sensitivity and resolution needed for the identification of donors, a magneto-photoluminescence system 1s installed along with a tunable dye laser, which provides resonant excitation. Donors 1n high purity GaAs are identified from the magnetic splittings of "two-electron" satellites of donor bound exciton transitions 1n a high magnetic field and at liquid helium temperature. This technique 1s successfully used to identify donors 1n n-type GaAs as well as 1n p-type GaAs in which donors cannot be identified by any other technique. The technique is also employed to identify donors in high purity InP. The amphoteric incorporation of Si and Ge impurities as donors and acceptors in (100), (311)A and (3ll)B GaAs grown by molecular beam epitaxy is studied spectroscopically. The hydrogen passivation of C acceptors in high purity GaAs grown by molecular beam epitaxy (MBE) and metalorganic chemical vapor deposition (MOCVD) 1s investigated using photoluminescence. Si acceptors ~n MBE GaAs are also found to be passivated by hydrogenation. The instabilities in the passivation of acceptor impurities are observed for the exposure of those samples to light. Very high purity MOCVD InP samples with extremely high mobility are characterized by both electrical and optical techniques. It is determined that C is not typically incorporated as a residual acceptor ~n high purity MOCVD InP. Finally, GaAs on Si, single quantum well, and multiple quantum well heterostructures, which are fabricated from III-V semiconductors, are also measured by low-temperature photoluminescence.

Probabilistic verification of satellite systems for mission critical applications

In this thesis, we present a quantitative approach using probabilistic verification techniques for the analysis of reliability, availability, maintainability, and safety (RAMS) properties of satellite systems. The subject of our research is satellites used in mission critical industrial applications. A strong case for using probabilistic model checking to support RAMS analysis of satellite systems is made by our verification results. This study is intended to build a foundation to help reliability engineers with a basic background in model checking to apply probabilistic model checking to small satellite systems. We make two major contributions. One of these is the approach of RAMS analysis to satellite systems. In the past, RAMS analysis has been extensively applied to the field of electrical and electronics engineering. It allows system designers and reliability engineers to predict the likelihood of failures from the indication of historical or current operational data. There is a high potential for the application of RAMS analysis in the field of space science and engineering. However, there is a lack of standardisation and suitable procedures for the correct study of RAMS characteristics for satellite systems. This thesis considers the promising application of RAMS analysis to the case of satellite design, use, and maintenance, focusing on its system segments. Data collection and verification procedures are discussed, and a number of considerations are also presented on how to predict the probability of failure. Our second contribution is leveraging the power of probabilistic model checking to analyse satellite systems. We present techniques for analysing satellite systems that differ from the more common quantitative approaches based on traditional simulation and testing. These techniques have not been applied in this context before. We present the use of probabilistic techniques via a suite of detailed examples, together with their analysis. Our presentation is done in an incremental manner: in terms of complexity of application domains and system models, and a detailed PRISM model of each scenario. We also provide results from practical work together with a discussion about future improvements.

Cassini states for black hole binaries

Cassini states correspond to the equilibria of the spin axis of a body when its orbit is perturbed. They were initially described for planetary satellites, but the spin axes of black hole binaries also present this kind of equilibria. In previous works, Cassini states were reported as spin-orbit resonances, but actually the spin of black hole binaries is in circulation and there is no resonant motion. Here we provide a general description of the spin dynamics of black hole binary systems based on a Hamiltonian formalism. In absence of dissipation, the problem is integrable and it is easy to identify all possible trajectories for the spin for a given value of the total angular momentum. As the system collapses due to radiation reaction, the Cassini states are shifted to different positions, which modifies the dynamics around them. This is why the final spin distribution may differ from the initial one. Our method provides a simple way of predicting the distribution of the spin of black hole binaries at the end of the inspiral phase.

Close-in planets around giant stars: lack of hot-Jupiters and prevalence of multiplanetary systems

Extrasolar planets abound in almost any possible configuration. However, until five years ago, there was a lack of planets orbiting closer than 0.5 au to giant or subgiant stars. Since then, recent detections have started to populated this regime by confirming 13 planetary systems. We discuss the properties of these systems in terms of their formation and evolution off the main sequence. Interestingly, we find that 70.0 ± 6.6% of the planets in this regime are inner components of multiplanetary systems. This value is 4.2σ higher than for main-sequence hosts, which we find to be 42.4 ± 0.1%. The properties of the known planets seem to indicate that the closest-in planets (a< 0.06 au) to main-sequence stars are massive (i.e., hot Jupiters) and isolated and that they are subsequently engulfed by their host as it evolves to the red giant branch, leaving only the predominant population of multiplanetary systems in orbits 0.06

The study of correlation between sea surface temperature (SST) by using the NOAA-AVHRR data and compare this data with temperature measurement in the Caspian Sea

The changes in time and location of surface temperature from a water body has an important effect on climate activities, marine biology, sea currents, salinity and other characteristics of the seas and lakes water. Traditional measurement of temperature is costly and time consumer due to its dispersion and instability. In recent years the use of satellite technology and remote sensing sciences for data acquiring and parameter and lysis of climatology and oceanography is well developed. In this research we used the NOAA’s Satellite images from its AVHRR system to compare the field surface temperature data with the satellite images information. Ten satellite images were used in this project. These images were calibrated with the field data at the exact time of satellite pass above the area. The result was a significant relation between surface temperatures from satellite data with the field work. As the relative error less than %40 between these two data is acceptable, therefore in our observation the maximum error is %21.2 that can be considered it as acceptable. In all stations the result of satellite measurements is usually less than field data that cores ponds with the global result too. As this sea has a vast latitude, therefore the different in the temperature is natural. But we know this factor is not the only cause for surface currents. The information of all satellites were images extracted by ERDAS software, and the “Surfer” software is used to plot the isotherm lines.

Multiwavelength observations of the blazar 1ES 1011+496 in Spring 2008

The BL Lac object 1ES 1011+496 was discovered at Very High Energy (VHE, E>100GeV) γ-rays by MAGIC in spring 2007. Before that the source was little studied in different wavelengths. Therefore a multi-wavelength (MWL) campaign was organized in spring 2008. Along MAGIC, the MWL campaign included the Mets¨ahovi radio observatory, Bell and KVA optical telescopes and the Swift and AGILE satellites. MAGIC observations span from March to May, 2008 for a total of 27.9 hours, of which 19.4 hours remained after quality cuts. The light curve showed no significant variability yielding an integral flux above 200 GeV of (1.3 ± 0.3) × 10^(−11) photons cm^(−2) s^( −1) . The differential VHE spectrum could be described with a power-law function with a spectral index of 3.3 ± 0.4. Both results were similar to those obtained during the discovery. Swift XRT observations revealed an X-ray flare, characterized by a harder-when-brighter trend, as is typical for high synchrotron peak BL Lac objects (HBL). Strong optical variability was found during the campaign, but no conclusion on the connection between the optical and VHE γ-ray bands could be drawn. The contemporaneous SED shows a synchrotron dominated source, unlike concluded in previous work based on non-simultaneous data, and is well described by a standard one–zone synchrotron self–Compton model. We also performed a study on the source classification. While the optical and X-ray data taken during our campaign show typical characteristics of an HBL, we suggest, based on archival data, that 1ES 1011+496 is actually a borderline case between intermediate and high synchrotron peak frequency BL Lac objects.