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  • 1
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 12 (2000), S. 609-617 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: In this study we present results from three-dimensional numerical experiments on thermal convection in a volumetrically heated, infinite Prandtl number fluid cooled from above. At high Rayleigh number, a thin thermal boundary layer forms adjacent to the cold top boundary. On the basis of our numerical results we study the thermal structure and dynamics of this boundary layer and the population of plumes that it creates. Cold thermal plumes that develop by boundary layer instability form continuous nearly vertical columns that migrate horizontally sweeping off the unstable boundary layer. A plume usually persists until it coalesces with another plume. The average spacing of plumes, inferred from the variation of the observed number of plumes with Rayleigh number, is proportional to (δd)1/2, where δ and d are the thermal boundary layer and fluid layer thicknesses, respectively. Based on a "kinetic theory" of plume populations, we show that this is consistent with an equilibrium plume population in which the creation of plumes by boundary layer instability and their disappearance by coalescing with other plumes are balanced. This scaling of average plume spacing is a consequence of the width of velocity plumes in a very viscous (infinite Prandtl number) fluid comparable to the fluid layer depth. For finite Prandtl number, the same analysis but with temperature and velocity plumes of comparable width predicts a plume spacing proportional to the boundary layer thickness. © 2000 American Institute of Physics.
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  • 2
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 116 (1994), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The structure and time dependence of 3-D thermal convection in a volumetrically heated, infinite Prandtl number fluid is examined for high values of the Rayleigh number. The methods employed allow the numerical experiments to proceed for long-enough times to derive good estimates of mean and fluctuating parts of the structure. An iterative multirigid method to solve for the buoyant, incompressible viscous flow at each time step of the energy equation is a novel aspect of the methodology. A simple explicit time step of the energy equation is utilized that vectorizes well on serial computers and which is ideally suited to massively parallel computers. Numerical experiments were carried out for Rayleigh numbers from 3 × 106 to 3 × 107 in a cartesian region with a prescribed temperature at the top boundary and an adiabatic bottom boundary. Over this complete range of Rayleigh number, the flow structure consists dominantly of cold, nearly axisymmetric plumes that migrate horizontally sweeping off the cold thermal-boundary layer that forms at the top of the convecting fluid. Plumes disappear by coalescing with other plumes; new plumes are created by thermal-boundary-layer instability. Sheet plumes form only occasionally and do not penetrate to significant depths in the fluid. Plumes have sizes comparable to the thickness of the thermal-boundary layer and an average spacing comparable to the fluid depth. No persistent large-scale motion in the fluid can be identified. Its absence may reflect the large subadiabatic stratification that develops beneath the thermal-boundary layer as cold plumes penetrate to the bottom boundary without thermally equilibrating with surrounding fluid. We consider the possible implications for convection in planetary mantles and for the existence of plate tectonics.
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  • 3
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 112 (1993), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: Buoyant flow beneath oceanic spreading centres can be driven by density gradients due to thermal expansion and compositional gradients arising from the extraction of melt. Numerical experiments are used to examine the pattern of mantle flow and melting produced by these two sources of buoyancy. Compositional buoyancy leads to three-dimensional flow beneath the spreading axis with along-axis variations in upwelling and melt production. Thermal buoyancy drives axis-parallel circulation and convective rolls aligned perpendicular to the spreading axis that originate at a distance off-axis controlled by the spreading rate and mantle viscosity. Hie distance from the axis to the onset of observed sea-floor gravity lineations may show a similar dependence on spreading rate. Compositional density stratification suppresses the formation of thermally driven rolls near the axis, and when it is large causes the thermal rolls to become unstable, leading to time-dependent behaviour. the amount of crust produced is less sensitive to spreading rate than in passive flow models, however it has a maximum at intermediate spreading rates, due to the presence of thermally driven upwelling in the melting region. Along-axis variations in upwelling and melt production suggest that buoyant flow may have an important effect on the segmentation of spreading centres, particularly at slow spreading rates.
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  • 4
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 96 (1989), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: We examine the extensional deformation of oceanic plates at mid-ocean ridges, especially within an axial yield zone where pervasive faulting occurs. Thermal models of ridges are developed which include the effects of lithospheric thickening on the mantle flow, the heat of magmatic crustal accretion at the ridge axis, and the hydrothermal cooling due to seawater circulation in the crust. When hydrothermal circulation occurs, the brittle lithospheric plate at slow-spreading ridges could be as thick as 8-9 km, thicker than the crust; while the plate at fast-spreading ridges is only 1-2 km. For a typical slow-spreading ridge, several kilometres of plate thickening are expected within a distance of 15 km from the ridge axis.When subjected to the extensional force due to horizontal stretching, shear failure by normal faulting will occur pervasively in an axial zone, where the lithospheric plate is the thinnest. Adopting perfectly plastic rheology as a continuum description of deformation on the distributed faults, we obtain approximate solutions for the stress distribution in the yield zone. Within this yield zone, sea-floor topography increases significantly away from the ridge axis so that the resulting gravity sliding force balances the differential horizontal extensional force due to the thickening of the lithospheric plate. Basal stresses induced by the viscously deforming asthenosphere could significantly influence the stresses inside the lithospheric plate only if the mantle viscosity beneath the ridge is on the order of 1020 Pa s, significantly higher than generally accepted values of 1018 Pa s. Model calculations reveal that although the sea floor topography at the Mid-Atlantic Ridge at 13-15 d̀N is regionally compensated, it is locally supported by stresses in the lithospheric plate. The deviation of the lithospheric plate from its thermal isostatic equilibrium position can be explained by necking due to plastic stretching in the axial yield zone and elastic deflection of strong plates outside the yield zone. The best fit models require the yield zones to have a half width of 10-15 km.We find systematic variations in the gravity and topography of the East Pacific Rise, which indicate strong influence of plate spreading rate on the ridge thermal and mechanical structure. At the 16-17 d̀N area, where the half-spreading rate is 4.3 cm yr-1, a prominent axial topographic high and an axial mantle Bouguer gravity low exist, implying a crustal or sub-crustal low density body. The gravity low disappears at the 20-21 d̀N area, where the half-spreading rate is 3.6 cm yr1. As the plate spreading rate decreases from 4.3 cm yr1 at the 16-17 d̀N area to 2.7 cm yr1 at the 22-23 d̀N area, axial ridge topography changes from higher than the thermal isostatic equilibrium position to lower than the isostatic position. The low axial topography at the 22-23 d̀N area can be explained by the existence of a low amplitude median valley.
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 295 (1982), S. 290-293 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] GANYMEDE, Jupiter's largest moon, is the largest known icy object in the Solar System. Voyager images of its surface show a complex and unique geology with widespread evidence for tectonic activity1'2. For silicate bodies on which significant lateral motion of the lithosphère does not occur, global ...
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  • 6
    Electronic Resource
    Electronic Resource
    Oxford, UK; Malden, USA : Blackwell Science Ltd
    Journal of fish biology 66 (2005), S. 0 
    ISSN: 1095-8649
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: At hatching (15 h post fertilization), Brycon moorei possesses no skeletal structure. Thereafter, development is very rapid. The first oral teeth appear no later than 3 h post-hatching, but they remain covered with epithelium until c. 45 h. At 7 h, the trabecular bars and part of the cartilaginous visceral arches are visible and at 15 h, the dentaries and premaxillaries are present. At 25 h, i.e. the onset of piscivory and cannibalism (the yolk sac is only fully resorbed after 36 h), the oral teeth are fully developed, the first pharyngeal teeth are formed, and some head movements already appear synchronized, but the mouth cavity is not completely isolated from the neurocranium by bony structures. Thereafter, no new buccal or pharyngeal bony structure is visible until 45 h, when the maxilla and opercula appear, along with a new type of cannibalistic behaviour. Cartilage resorptions also start at 45 h, but with no concomitant replacement by formation of calcified structures. Later, development gradually becomes similar to that of many previously studied teleosts. The developmental pattern of B. moorei is thus extremely rapid in comparison with other teleosts, i.e. it prioritizes feeding structures that permit the expression of piscivory at a very early age. The uniqueness of this pattern is discussed in relation to ecological constraints on early feeding and fast growth.
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  • 7
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Journal of fish biology 58 (2001), S. 0 
    ISSN: 1095-8649
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: Carapid species are characterized by so-called otophysical structures (sonic muscles, broad first apophyses covering the anterior part of the swimbladder, etc.) The family includes pelagic (Pyramodon and Snyderidia) and benthic (Echiodon) species and ones that are either commensal with (Onuxodon, Carapus) or parasites of (Encheliophis) invertebrates (sea cucumbers, etc). The aim of the present work was to seek possible relationships between the structures of the inner ear (particularly the sagitta) on the one hand and otophysical structures and lifestyles within the Carapidae family. In the eight species studied, the otic cavity is wide, the saccular otosac and its sagitta are particularly developed. The sacculi touch each other on the median line. A comparison of the inner ear structures reveals notably that the species with the most developed sagitta and sacculus are those with the largest parapophyses and have a commensal or parasitic lifestyle.
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  • 8
    Electronic Resource
    Electronic Resource
    Oxford, UK; Malden , USA : Blackwell Publishing Ltd/Inc
    Journal of fish biology 64 (2004), S. 0 
    ISSN: 1095-8649
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: Body shortening was observed in the pearlfish Carapus homei during metamorphosis. The tenuis larva at first possessed a suite of osseous vertebral bodies of similar length. The reduction in both the number and size of vertebrae followed increasing decalcification, degeneration of organic tissue and shortening. This involved a complete degradation and disappearance of the caudal tip vertebrae, and there was a reduction in the size of most of the remaining vertebrae. The further development of the vertebrae began with ossification of the neural and haemal arches before that of the vertebral body. This second part of the development followed a gradient: a gradual decreases towards the caudal tip in the size of the vertebrae and their completeness.
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  • 9
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Journal of fish biology 55 (1999), S. 0 
    ISSN: 1095-8649
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: The inception and development of the cartilaginous cephalis skeleton of Chrysichthys auratus is described from hatching to about 18 days post-hatching. At hatching, no skeletal structure is present. Not until day 3 do clearly delimited cranial primordia become apparent. As in many siluriforms, the neurocranium is platybasic from the start, the suspensorium constitutes, with Meckel's cartilage and the hyoid bar, a single cartilaginous element, and the junction between the front and rear of the neurocranium is complete on day 4. By day 8 the quadratomandibular joint has formed and the tectum posterius has appeared. Cartilage reduction first affects the trabecular bars, then, markedly, the visceral arches. By day 18 the braincase floor has almost disappeared.
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  • 10
    ISSN: 1432-234X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract  Onuxodon fowleri and Encheliophis dubius are two Carapidae species that live in bivalve hosts and their diet is made of the same type of prey. The aim of this study is to compare their cephalic morphology to see whether: (1) the head anatomy of both species is related to the constraints of their way of life and (2) there are differences between these species and commensal carapids that shelter in other invertebrates. The components of their skeletons and muscles are similar, but differ in size and are arranged differently. In O. fowleri, the buccal cavity is smaller than in E. dubius, the jaws (bearing very large anterior teeth) are larger, the quadrato- mandibular joint lies further to the rear and the fibres of muscle bundles A3α, A2α and A2β are more vertical and insert higher on the neurocranium. The buccal system of O. fowleri appears better suited for ingesting food by biting and grasping. That of E. dubius seems better adapted to a feeding mechanism where sucking would have a more important role. The E. dubius head morphology is more similar to the cephalic anatomy of non-bivalve commensal species than to O. fowleri features. Diet constraints may have greater influence than the different host constraints on the head construction. A simulated backwards rotation of the posterior part of the E. dubius suspensorium around the posterior joint between the hyomandibular and the neurocranium brings the jaws and the cheeks to coincide with those of O. fowleri. This model could be indicative of how structure modifications and their influences on annex pieces could in part have a role in the biodiversity.
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