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.

Rapport de mission sur la conférence mondiale sur l'aquaculture, organisée conjointement par la World Aquaculture Society et la European Aquaculture Society. Florence, Italie, 9-13 mai 2006

Ce congrès était organisé conjointement par les deux grandes associations de développement de l'aquaculture dans le monde: la World Aquaculture Society (WAS, 2300 membres) et la European Aquaculture Society (EAS, 550 membres). Le précédent s'était tenu à Nice, en mai 2000. Il a rassemblé pendant 5 jours plus de 3000 chercheurs et responsables institutionnels de 95 nationalités. Environ 600 communications orales étaient réparties sur 67 sessions suivant un système de 11 salles en parallèle. Entre les salles de conférence étaient présentés les panneaux des 460 posters. Sur le site, l'exposition commerciale accueillait 135 entreprises et organismes; elle a reçu la visite d'environ 2000 visiteurs dont la moitié d'Italiens (source: EAS). Le thème général du congrès était le lien entre la tradition et la technologie. L'objectif était de montrer que les technologies, dont l'image est ambivalente, constituent un outil remarquable de développement de l'aquaculture, y compris en tenant compte des contraintes de durabilité. En effet, les attentes du citoyen, comme du consommateur, restent centrées autour des notions de qualité, sécurité alimentaire, bien-être et santé animale. Les travaux portaient sur les disciplines classiques de l'aquaculture (nutrition, physiologie, génétique, etc) et leur relation avec les biotechnologies. Il faut souligner l'émergence de thèmes de plus en plus liés la démonstration que l'aquaculture peut s'intégrer dans détruire (capacité de charge d'un écosystème, animaux échappés, etc) et à la perception de la société (perception du consommateur, aquaculture et société, position des ONG écologistes, etc). L'U.E. était très présente avec 5 représentants et une implication marquée dans de plusieurs sessions. Sous différentes formes, ses représentants ont rappelé la volonté de l'UE de continuer à soutenir l'aquaculture, avec l'objectif de poursuivre le développement de ce secteur (4 % de croissance moyenne par an). L'aquaculture devrait générer 8 à 10 000 emplois nouveaux sur les 15 prochaines années, notamment dans la conchyliculture et la pisciculture marine au large avec comme mot clef l'intégration dans l'environnement, dans le tissu socio-économique côtier et dans l'imaginaire des gens, touristes, consommateurs, élus, etc. Ce congrès à vocation mondiale a attiré des représentants de régions habituellement peu représentées comme le Moyen Orient et la Chine, présente à de nombreuses sessions. Il a été aussi le lieu de multiples réunions satellites impliquant presque toujours des chercheurs français: grands programmes européens en cours comme SeaFood+, ASEM (coop. Europe - Asie) ou Consensus, assemblée générale de l'EAS, groupe de travail de l'UICN, etc. Ce type de réunion confirme l'importance des contacts personnels directs pour 1. Evaluer les grandes tendances mondiales du secteur 2. Etablir des contacts directs avec des chercheurs seniors des grandes équipes de recherche et des décideurs au niveau européen et extra-européen 3. Tester des idées et des projets de collaboration et de partenariat Il constitue un forum exceptionnel de diffusion de connaissances, d'informations et de messages. Il offre un espace de perception et de reconnaissance d'Ifremer par de nombreux acteurs de la communauté de recherche en aquaculture. Grâce à la variété thématique des sessions où des chercheurs d'Ifremer sont actifs, l'institut renforce sa notoriété notamment dans la dimension pluridisciplinaire. Cette capacité d'ensemblier est la qualité la plus demandée dans les conclusions d'ateliers et la plus rare dans les instituts présents. Le congrès révèle bien l'évolution de l'aquaculture mondiale: il y a 10 ans, la production de masse était au Sud et la technologie et les marchés au Nord (USA, Europe, Japon). Aujourd'hui, la progression économique et scientifique rapide des pays du Sud, surtout en Asie, crée des marchés locaux .solvables pour l'aquaculture (Chine, Inde) et fait émerger une capacité de recherche « de masse». Cette situation exige que la recherche occidentale évolue pour rester compétitive. Pour préserver un secteur important, qui concourt à la sécurité alimentaire en protéines de manière croissante (4% par an, record de toutes les productions alimentaires), la recherche européenne en aquaculture doit maintenir son effort afin de garder une longueur d'avance, surtout dans les secteurs qui seront vitaux dans la décennie: relations avec l'environnement naturel (durabilité dont la maîtrise des coûts énergétiques), qualité des produits, sécurité alimentaire, intégration socio-économique dans des espaces de plus en plus convoités, maîtrise de l'image de l'espèce « cultivée» (industrielle mais contrôlée) par rapport à l'image de l'espèce « sauvage» (naturelle mais polluée et surexploitée). En conséquence, l'UE conserve tout son potentiel de développement car l'essentiel de la valeur ajoutée sera de moins en moins dans la production en quantité mais dans sa maîtrise de la qualité. Cette évolution donne toute sa valeur à la recherche menée par Ifremer et ce d'autant plus que l'institut sera capable d'anticiper les besoins et les attentes des entreprises, des consommateurs, des associations comme des organisations internationales. Dans cette vision, réactivité, capacité d'ensemblier et réflexion prospective sont les qualités à développer pour que l'lfremer puisse donner toute sa mesure notamment dans la recherche en aquaculture. Ces enjeux sont à l'échelle internationale et Ifremer fait partie du petit nombre d'instituts capables de les traiter en large partenariat, en accord complet avec la politique souhaitée par l'UE

RELATIONSHIP BETWEEN COLUMN DENSITY AND SURFACE MIXING RATIO FOR O3 AND NO2: IMPLICATIONS FOR SATELLITE OBSERVATIONS AND THE IMPACTS OF VERTICAL MIXING

Satellites have great potential for diagnosis of surface air quality conditions, though reduced sensitivity of satellite instrumentation to the lower troposphere currently impedes their applicability. One objective of the NASA DISCOVER-AQ project is to provide information relevant to improving our ability to relate satellite-observed columns to surface conditions for key trace gases and aerosols. In support of DISCOVER-AQ, this dissertation investigates the degree of correlation between O3 and NO2 column abundance and surface mixing ratio during the four DISCOVER-AQ deployments; characterize the variability of the aircraft in situ and model-simulated O3 and NO2 profiles; and use the WRF-Chem model to further investigate the role of boundary layer mixing in the column-surface connection for the Maryland 2011 deployment, and determine which of the available boundary layer schemes best captures the observations. Simple linear regression analyses suggest that O3 partial column observations from future satellite instruments with sufficient sensitivity to the lower troposphere may be most meaningful for surface air quality under the conditions associated with the Maryland 2011 campaign, which included generally deep, convective boundary layers, the least wind shear of all four deployments, and few geographical influences on local meteorology, with exception of bay breezes. Hierarchical clustering analysis of the in situ O3 and NO2 profiles indicate that the degree of vertical mixing (defined by temperature lapse rate) associated with each cluster exerted an important influence on the shapes of the median cluster profiles for O3, as well as impacted the column vs. surface correlations for many clusters for both O3 and NO2. However, comparisons to the CMAQ model suggest that, among other errors, vertical mixing is overestimated, causing too great a column-surface connection within the model. Finally, the WRF-Chem model, a meteorology model with coupled chemistry, is used to further investigate the impact of vertical mixing on the O3 and NO2 column-surface connection, for an ozone pollution event that occurred on July 26-29, 2011. Five PBL schemes were tested, with no one scheme producing a clear, consistent “best” comparison with the observations for PBLH and pollutant profiles; however, despite improvements, the ACM2 scheme continues to overestimate vertical mixing.

Wave climate in the Arctic 1992-2014: seasonality and trends

Over the past decade, the diminishing Arctic sea ice has impacted the wave field, which depends on the ice-free ocean and wind. This study characterizes the wave climate in the Arctic spanning 1992–2014 from a merged altimeter data set and a wave hindcast that uses CFSR winds and ice concentrations from satellites as input. The model performs well, verified by the altimeters, and is relatively consistent for climate studies. The wave seasonality and extremes are linked to the ice coverage, wind strength, and wind direction, creating distinct features in the wind seas and swells. The altimeters and model show that the reduction of sea ice coverage causes increasing wave heights instead of the wind. However, trends are convoluted by interannual climate oscillations like the North Atlantic Oscillation (NAO) and Pacific Decadal Oscillation. In the Nordic Greenland Sea the NAO influences the decreasing wind speeds and wave heights. Swells are becoming more prevalent and wind-sea steepness is declining. The satellite data show the sea ice minimum occurs later in fall when the wind speeds increase. This creates more favorable conditions for wave development. Therefore we expect the ice freeze-up in fall to be the most critical season in the Arctic and small changes in ice cover, wind speeds, and wave heights can have large impacts to the evolution of the sea ice throughout the year. It is inconclusive how important wave–ice processes are within the climate system, but selected events suggest the importance of waves within the marginal ice zone.