926 resultados para Saturn-Ring Defects


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The theory of deterministic chaos is used to study the three rings A, B, and C of Saturn and the French and Cassini divisions in between them. The data set comprises Voyager photopolarimeter measurements. The existence of spatially distributed strange attractors is shown, implying that the system is open, dissipative, nonequilibrium, and non-Markovian in character.

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We use a two-dimensional (2D) elastic free energy to calculate the effective interaction between two circular disks immersed in smectic-C films. For strong homeotropic anchoring, the distortion of the director field caused by the disks generates topological defects that induce an effective interaction between the disks. We use finite elements, with adaptive meshing, to minimize the 2D elastic free energy. The method is shown to be accurate and efficient for inhomogeneities on the length scales set by the disks and the defects, that differ by up to 3 orders of magnitude. We compute the effective interaction between two disk-defect pairs in a simple (linear) configuration. For large disk separations, D, the elastic free energy scales as similar to D-2, confirming the dipolar character of the long-range effective interaction. For small D the energy exhibits a pronounced minimum. The lowest energy corresponds to a symmetrical configuration of the disk-defect pairs, with the inner defect at the mid-point between the disks. The disks are separated by a distance that, is twice the distance of the outer defect from the nearest disk. The latter is identical to the equilibrium distance of a defect nucleated by an isolated disk.

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The interaction between two disks immersed in a 2D nernatic is investigated i) analytically using the tenser order parameter formalism for the nematic configuration around isolated disks and ii) numerically using finite-element methods with adaptive meshing to minimize the corresponding Landau-de Gennes free energy. For strong homeotropic anchoring, each disk generates a pair of defects with one-half topological charge responsible for the 2D quadrupolar interaction between the disks at large distances. At short distance, the position of the defects may change, leading to unexpected complex interactions with the quadrupolar repulsive interactions becoming attractive. This short-range attraction in all directions is still anisotropic. As the distance between the disks decreases, their preferred relative orientation with respect to the far-field nernatic director changes from oblique to perpendicular.

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Rolling element bearings are essential components of rotating machinery. The spherical roller bearing (SRB) is one variant seeing increasing use, because it is self-aligning and can support high loads. It is becoming increasingly important to understand how the SRB responds dynamically under a variety of conditions. This doctoral dissertation introduces a computationally efficient, three-degree-of-freedom, SRB model that was developed to predict the transient dynamic behaviors of a rotor-SRB system. In the model, bearing forces and deflections were calculated as a function of contact deformation and bearing geometry parameters according to nonlinear Hertzian contact theory. The results reveal how some of the more important parameters; such as diametral clearance, the number of rollers, and osculation number; influence ultimate bearing performance. Distributed defects, such as the waviness of the inner and outer ring, and localized defects, such as inner and outer ring defects, are taken into consideration in the proposed model. Simulation results were verified with results obtained by applying the formula for the spherical roller bearing radial deflection and the commercial bearing analysis software. Following model verification, a numerical simulation was carried out successfully for a full rotor-bearing system to demonstrate the application of this newly developed SRB model in a typical real world analysis. Accuracy of the model was verified by comparing measured to predicted behaviors for equivalent systems.

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We directly visualize the response of nematic liquid crystal drops of toroidal topology threaded in cellulosic fibers, suspended in air, to an AC electric field and at different temperatures over the N-I transition. This new liquid crystal system can exhibit non-trivial point defects, which can be energetically unstable against expanding into ring defects depending on the fiber constraining geometries. The director anchoring tangentially near the fiber surface and homeotropically at the air interface makes a hybrid shell distribution that in turn causes a ring disclination line around the main axis of the fiber at the center of the droplet. Upon application of an electric field, E, the disclination ring first expands and moves along the fiber main axis, followed by the appearance of a stable "spherical particle" object orbiting around the fiber at the center of the liquid crystal drop. The rotation speed of this particle was found to vary linearly with the applied voltage. This constrained liquid crystal geometry seems to meet the essential requirements in which soliton-like deformations can develop and exhibit stable orbiting in three dimensions upon application of an external electric field. On changing the temperature the system remains stable and allows the study of the defect evolution near the nematic-isotropic transition, showing qualitatively different behaviour on cooling and heating processes. The necklaces of such liquid crystal drops constitute excellent systems for the study of topological defects and their evolution and open new perspectives for application in microelectronics and photonics.

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La vie commence par la fusion des gamètes pour générer un zygote, dans lequel les constituants à la fois de l'ovocyte et des spermatozoïdes sont partagés au sein d'un syncytium. Le syncytium consiste en des cellules ou tissus dans lesquels des cellules nucléées individuelles distinctes partagent un cytoplasme commun. Alors que l’avantage du syncytium durant la fécondation est tout à fait évident, les syncytia se produisent également dans de nombreux contextes de développement différents dans les plantes, les champignons et dans le règne animal, des insectes aux humains, pour des raisons qui ne sont pas immédiatement évidentes. Par exemple, la lignée germinale de nombreuses espèces de vertébrés et d'invertébrés, des insectes aux humains, présente une structure syncytiale, suggérant que les syncytia constituent des phases conservées de développement de la lignée germinale. Malgré la prévalence commune des syncytia, ces derniers ont cependant confondu les scientifiques depuis des décennies avec des questions telles que la façon dont ils sont formés et maintenus en concurrence avec leurs homologues diploïdes, et quels sont les avantages et les inconvénients qu'ils apportent. Cette thèse va décrire l'utilisation de la lignée germinale syncytiale de C. elegans afin d'approfondir notre compréhension de l'architecture, la fonction et le mode de formation des tissus syncytiaux. Les cellules germinales (CGs) dans la lignée germinale de C. elegans sont interconnectées les unes aux autres par l'intermédiaire de structures appelées des anneaux de CG. En utilisant l'imagerie des cellules vivantes, nous avons d'abord analysé l'architecture syncytiale de la lignée germinale au long du développement et démontré que la maturation de l'anneau de CG se produit progressivement au cours de la croissance des larves et que les anneaux de CG sont composés de myosine II, de l'anilline canonique ANI-1, et de la courte isoforme d’anilline ANI-2, qui n'a pas les domaines de liaison à l’actine et à la myosine, depuis le premier stade larvaire, L1. Parmi les composants de l'anneau de CG, ANI-2 est exprimé au cours du développement et exclusivement enrichi entre les deux CGs primordiales (CGPs) au cours de l'embryogenèse de C. elegans, indiquant qu’ANI-2 est un composant bona fide des anneaux de CG. Nous avons en outre montré que les anneaux de CG sont largement absents dans les animaux mutants pour ani-2, montrant que leur maintien repose sur l'activité d'ANI-2. Contrairement à cela, nous avons trouvé que la déplétion d’ANI-1 a augmenté à la fois le diamètre des anneaux de CG et la largeur du rachis. Fait intéressant, la déplétion d’ANI-1 dans les mutants d’ani-2 a sauvé les défauts d'anneaux de CG des gonades déficientes en ani-2, ce qui suggère que l'architecture syncytiale de la lignée germinale de C. elegans repose sur un équilibre de l'activité de ces deux protéines Anilline. En outre, nous avons montré que lors de leur entrée à l'âge adulte, les mutants ani-2 présentent de sévères défauts de multinucléation des CGs qui découlent de l'effondrement des membranes de séparation des CGs individuelles. Cette multinucléation a coïncidé avec le début de la diffusion cytoplasmique, dont le blocage réduit la multinucléation des gonades mutantes pour ani-2, suggérant que les anneaux de CG résistent au stress mécanique associé au processus de diffusion cytoplasmique. En accord avec cela, nous avons trouvé aussi que la gonade peut soutenir la déformation élastique en réponse au stress mécanique et que cette propriété repose sur la malléabilité des anneaux de CGs. Dans une étude séparée afin de comprendre le mécanisme de formation du syncytium, nous avons suivi la dynamique de division de la cellule précurseur de la lignée germinale, P4 en deux CGP dans l’embryon de C. elegans. Nous avons démontré que les CGPs commencent la cytocinèse de manière similaire aux cellules somatiques, en formant un sillon de clivage, qui migre correctement et transforme ainsi l'anneau contractile en anneau de « midbody ring » (MBR), une structure qui relie de manière transitoire les cellules en division. Malgré cela, les CGPs, contrairement à leurs homologues somatiques, ne parviennent pas à accomplir la dernière étape de la cytocinèse, qui est la libération abscission-dépendante du MBR. Au lieu de cela, le MBR persiste à la frontière entre les CGPs en division et subit une réorganisation et une maturation pour se transformer finalement en structures en forme d'anneau qui relient les cellules en division. Nous montrons en outre que les composants du MB/MBR; UNC-59Septin, CYK-7, ZEN-4Mklp1, RHO-1RhoA sont localisés à des anneaux de CG au long du développement de la lignée germinale du stade L1 à l'âge adulte, ce qui suggère que les anneaux de CG sont dérivés des MBR. Bien qu'il reste encore beaucoup à faire pour comprendre pleinement le mécanisme précis de la formation du syncytium, le maintien, ainsi que la fonction du syncytium, nos résultats appuient un modèle dans lequel la stabilisation du MBR et la cytocinèse incomplète pourraient être une option conservée dans l’évolution pour la formation du syncytium. En outre, notre travail démontre que les régulateurs de la contractilité peuvent jouer un rôle dans la maturation et l’élasticité de l'anneau de CG au cours du développement de la lignée germinale, fournissant un ajout précieux pour une plus ample compréhension de la syncytiogenèse et de sa fonction.

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An algorithm is presented for the generation of molecular models of defective graphene fragments, containing a majority of 6-membered rings with a small number of 5- and 7-membered rings as defects. The structures are generated from an initial random array of points in 2D space, which are then subject to Delaunay triangulation. The dual of the triangulation forms a Voronoi tessellation of polygons with a range of ring sizes. An iterative cycle of refinement, involving deletion and addition of points followed by further triangulation, is performed until the user-defined criteria for the number of defects are met. The array of points and connectivities are then converted to a molecular structure and subject to geometry optimization using a standard molecular modeling package to generate final atomic coordinates. On the basis of molecular mechanics with minimization, this automated method can generate structures, which conform to user-supplied criteria and avoid the potential bias associated with the manual building of structures. One application of the algorithm is the generation of structures for the evaluation of the reactivity of different defect sites. Ab initio electronic structure calculations on a representative structure indicate preferential fluorination close to 5-ring defects.

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

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Saturn's F ring, which lies 3,400 km beyond the edge of the main ring system, was discovered by the Pioneer 11 spacecraft(1) in 1979. It is a narrow, eccentric ring which shows an unusual 'braided' appearance in several Voyager 1 images' obtained in 1980, although it appears more regular in images from Voyager 2 obtained nine months later(3). The discovery of the moons Pandora and Prometheus orbiting on either side of the ring provided a partial explanation for some of the observed features(4). Recent observations of Prometheus(5,6) by the Hubble Space Telescope show, surprisingly, that it is lagging behind its expected position by similar to 20 degrees. By modelling the dynamical evolution of the entire Prometheus-F ring-Pandora system, we show here that Prometheus probably encountered the core of the F ring in 1994 and that it may still be entering parts of the ring once per orbit. Collisions with objects in the F ring provide a plausible explanation for the observed lag and imply that the mass of the F ring is probably less than 25% that of Prometheus.

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Image photometry reveals that the F ring is approximately twice as bright during the Cassini tour as it was during the Voyager flybys of 1980 and 1981. It is also three times as wide and has a higher integrated optical depth. We have performed photometric measurements of more than 4800 images of Saturn's F ring taken over a 5-year period with Cassini's Narrow Angle Camera. We show that the ring is not optically thin in many observing geometries and apply a photometric model based on single-scattering in the presence of shadowing and obscuration, deriving a mean effective optical depth tau approximate to 0.033. Stellar occultation data from Voyager PPS and Cassini VIMS validate both the optical depth and the width measurements. In contrast to this decades-scale change, the baseline properties of the F ring have not changed significantly from 2004 to 2009. However, we have investigated one major, bright feature that appeared in the ring in late 2006. This transient feature increased the ring's overall mean brightness by 84% and decayed with a half-life of 91 days. (c) 2012 Elsevier B.V. All rights reserved.

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The strange morphology of the F ring of Saturn is thought to be caused by the perturbing effects of two close satellites, Prometheus and Pandora. The F ring and the satellites also experience periodic close encounters as a result of differential precession arising from Saturn's oblateness. Using the orbits of the F-ring strands derived by Murray et al. (1997, Icarus 129, 304-316) the behaviour of the ring particles at their closest approach to Prometheus is analysed using numerical simulations. The results show that a gap and a wave are formed in the ring at each encounter with the satellite. However, the gap is expected to have a short lifetime due to keplerian shear. © 2000 Elsevier Science Ltd. All rights reserved.

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The endodermis represents the main barrier to extracellular diffusion in plant roots, and it is central to current models of plant nutrient uptake. Despite this, little is known about the genes setting up this endodermal barrier. In this study, we report the identification and characterization of a strong barrier mutant, schengen3 (sgn3). We observe a surprising ability of the mutant to maintain nutrient homeostasis, but demonstrate a major defect in maintaining sufficient levels of the macronutrient potassium. We show that SGN3/GASSHO1 is a receptor-like kinase that is necessary for localizing CASPARIAN STRIP DOMAIN PROTEINS (CASPs)--major players of endodermal differentiation--into an uninterrupted, ring-like domain. SGN3 appears to localize into a broader band, embedding growing CASP microdomains. The discovery of SGN3 strongly advances our ability to interrogate mechanisms of plant nutrient homeostasis and provides a novel actor for localized microdomain formation at the endodermal plasma membrane.

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Particles in Saturn's main rings range in size from dust to kilometer-sized objects. Their size distribution is thought to be a result of competing accretion and fragmentation processes. While growth is naturally limited in tidal environments, frequent collisions among these objects may contribute to both accretion and fragmentation. As ring particles are primarily made of water ice attractive surface forces like adhesion could significantly influence these processes, finally determining the resulting size distribution. Here, we derive analytic expressions for the specific self-energy Q and related specific break-up energy Q(star) of aggregates. These expressions can be used for any aggregate type composed of monomeric constituents. We compare these expressions to numerical experiments where we create aggregates of various types including: regular packings like the face-centered cubic (fcc), Ballistic Particle Cluster Aggregates (BPCA), and modified BPCAs including e.g. different constituent size distributions. We show that accounting for attractive surface forces such as adhesion a simple approach is able to: (a) generally account for the size dependence of the specific break-up energy for fragmentation to occur reported in the literature, namely the division into "strength" and "gravity" regimes and (b) estimate the maximum aggregate size in a collisional ensemble to be on the order of a few tens of meters, consistent with the maximum particle size observed in Saturn's rings of about 10 m. (c) 2012 Elsevier B.V. All rights reserved.

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The aim of this study was to clinically and radiographically evaluate acute bone shortening followed by gradual lengthening in the treatment of large segmental tibia defects induced in seven clinically normal dogs. A circular external fixator was assembled with one proximal 5/8-circle ring, one middle ring and one distal ring connected with three rods. Thirty per cent of the tibia and fibula were removed in the middle and distal parts of the diaphyses, between the middle and distal rings. Acute bone shortening with compression of proximal and distal segments was performed. A subperiosteal osteotomy was performed between the half-ring and middle ring. Bone distraction started 7 days after surgery; after lengthening, the apparatus was left in place for 14 weeks for consolidation of regenerated bone. The frame was removed at the end of this period, and the dogs observed for four more weeks. Functional results were considered excellent in two, good in three and fair in the other two dogs. Bone regeneration within the distraction gap was obtained 14 weeks after neutral fixation period. We concluded that acute bone shortening followed by gradual lengthening by Ilizarov method can be used to treat extensive tibial defects in dogs, although it presents limb temporary abnormal limb shape and unequal length as early disadvantages.