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  • 1
    Online Resource
    Online Resource
    Cambridge :Cambridge University Press,
    Keywords: Geodynamics. ; Electronic books.
    Description / Table of Contents: Geophysical Continua presents a systematic treatment of deformation in the Earth and demonstrates the linkages between different aspects of the Earth's interior that are often treated separately.This textbook is designed for graduate-level courses in geophysics and geodynamics. It is also a useful reference for practising Earth scientists.
    Type of Medium: Online Resource
    Pages: 1 online resource (446 pages)
    Edition: 1st ed.
    ISBN: 9780511408090
    DDC: 551.11
    Language: English
    Note: Cover -- Half-title -- Title -- Copyright -- Contents -- Preface -- Acknowledgements -- 1 Introduction -- 1.1 Continuum properties -- 1.1.1 Deformation and strain -- 1.1.2 The stress field -- 1.1.3 Constitutive relations -- 1.2 Earth processes -- 1.3 Elements of Earth structure -- 1.3.1 Mantle -- 1.3.2 Core -- 1.4 The state of the Earth -- Deformation regimes and Earth dynamics -- Lithosphere: -- Asthenosphere: -- Transition zone: -- Lower mantle -- Core-mantle Boundary zone - D": -- Outer core: -- Inner core: -- Part I: CONTINUUM MECHANICS IN GEOPHYSICS -- 2 Description of Deformation -- 2.1 Geometry of deformation -- 2.1.1 Deformation of a vector element -- 2.1.2 Successive deformations -- 2.1.3 Deformation of an element of volume -- 2.1.4 Deformation of an element of area -- 2.1.5 Homogeneous deformation -- 2.2 Strain -- 2.2.1 Stretch -- 2.2.2 Principal fibres and principal stretches -- 2.2.3 The decomposition theorem -- 2.2.4 Pure rotation -- 2.2.5 Tensor measures of strain -- 2.3 Plane deformation -- Shear -- 2.4 Motion -- 2.5 The continuity equation -- Material derivative of a volume integral -- Appendix: Properties of the determinant of the deformation gradient -- 3 The Stress-Field Concept -- 3.1 Traction and stress -- Tensor character of stress -- 3.2 Local equations of linear motion -- 3.2.1 Symmetry of the stress tensor -- 3.2.2 Stress jumps (continuity conditions) -- 3.3 Principal basis for stress -- Stress circle -- 3.4 Virtual work rate principle -- Converse principle -- 3.5 Stress from a Lagrangian viewpoint -- 4 Constitutive Relations -- 4.1 Constitutive relation requirements -- 4.1.1 Simple materials -- 4.1.2 Material symmetry -- 4.1.3 Functional dependence -- 4.2 Energy balance -- Neglect of thermal effects -- 4.3 Elastic materials -- Material symmetry -- 4.4 Isotropic elastic material -- 4.4.1 Effect of rotation. , 4.4.2 Coaxiality of the Cauchy stress tensor and the Eulerian triad -- 4.4.3 Principal stresses -- 4.4.4 Some isotropic work functions -- 4.5 Fluids -- 4.6 Viscoelasticity -- Models of viscoelastic behaviour -- 4.7 Plasticity and flow -- 5 Linearised Elasticity and Viscoelasticity -- 5.1 Linearisation of deformation -- 5.2 The elastic constitutive relation -- 5.2.1 Isotropic response -- 5.2.2 Nature of moduli -- 5.2.3 Interrelations between moduli -- 5.2.4 An example of linearisation -- 5.2.5 Elastic constants -- 5.2.6 The uniqueness theorem -- Kirchhoff's Theorem -- 5.3 Integral representations -- 5.3.1 The reciprocal theorem -- 5.3.2 The representation theorem -- 5.4 Elastic waves -- 5.4.1 Isotropic media -- 5.4.2 Green's tensor for isotropic media -- 5.4.3 Interfaces -- 5.5 Linear viscoelasticity -- Creep and relaxation -- 5.6 Viscoelastic behaviour -- Isotropic linear viscoelasticity -- 5.7 Damping of harmonic oscillations -- 6 Continua under Pressure -- 6.1 Effect of radial stratification -- 6.1.1 Hydrostatic pressure -- 6.1.2 Thermodynamic relations -- 6.2 Finite strain deformation -- 6.3 Expansion of Helmholtz free energy and equations of state -- 6.4 Incremental stress and strain -- 6.4.1 Perturbations in stress -- 6.4.2 Perturbations in boundary conditions -- 6.5 Elasticity under pressure -- Seismic wavespeeds -- 7 Fluid Flow -- 7.1 The Navier-Stokes equation -- 7.1.1 Heat flow -- 7.1.2 The Prandtl number -- 7.2 Non-dimensional quantities -- 7.2.1 The Reynolds number -- 7.2.2 Stokes Flow -- 7.2.3 Compressibility -- 7.3 Rectilinear shear flow -- 7.4 Plane two-dimensional flow -- Viscous flow model of glacial rebound -- 7.5 Thermal convection -- 7.5.1 The Rayleigh and Nusselt numbers -- 7.5.2 The Boussinesq approximation -- 7.5.3 Onset of convection -- 7.5.4 Styles of convection -- 7.6 The effects of rotation -- 7.6.1 Rapid rotation. , 7.6.2 The Rossby and Ekman numbers -- 7.6.3 Geostrophic flow -- 7.6.4 The Taylor-Proudman theorem -- 7.6.5 Ekman layers -- 8 Continuum Equations and Boundary Conditions -- 8.1 Conservation equations -- 8.1.1 Conservation of mass -- 8.1.2 Conservation of momentum -- 8.3 Continuum electrodynamics -- 8.3.1 Maxwell's equations -- 8.3.2 Electromagnetic constitutive equations -- 8.3.3 Electromagnetic continuity conditions -- 8.3.4 Energy equation for the electromagnetic field -- 8.3.5 Electromagnetic disturbances -- 8.3.6 Magnetic fluid dynamics -- 8.4 Diffusion and heat flow -- 8.4.1 Equilibrium heat flow -- 8.4.2 Time-varying problems -- Part II: EARTH DEFORMATION -- 9 From the Atomic Scale to the Continuum -- 9.1 Transport properties and material defects -- 9.1.1 Grains and crystal defects -- 9.1.2 General transport properties -- 9.1.3 Atomic diffusion -- 9.2 Lattice vibrations -- Lattice specific heat -- 9.3 Creep and rheology -- 9.3.1 Crystal elasticity -- 9.3.2 Deformation behaviour -- 9.4 Material properties at high temperatures and pressures -- 9.4.1 Shock-wave techniques -- 9.4.2 Pressure concentration by reduction of area -- 9.5 Computational methods -- 9.5.1 Electronic structure calculations -- 9.5.2 Atomistic simulations -- 9.5.3 Simulation of crystal structures -- 9.5.4 Finite temperature -- 9.5.5 Influence of defects -- 10 Geological Deformation -- 10.1 Microfabrics -- 10.1.1 Crystal defects -- 10.1.2 Development of microstructure -- 10.1.3 Formation of crystallographically preferred orientations -- 10.2 Macroscopic structures -- 10.2.1 Multiple phases of deformation -- 10.2.2 Folding and boudinage -- 10.2.3 Fractures and faulting -- 10.2.4 Development of thrust complexes -- 11 Seismology and Earth Structure -- 11.1 Seismic waves -- 11.1.1 Reflection and refraction -- 11.1.2 Attenuation effects -- 11.2 Seismic sources. , 11.3 Building the response of the Earth to a source -- 11.3.1 Displacements as a normal mode sum -- 11.3.2 Free oscillations of the Earth -- 11.4 Probing the Earth -- 11.4.1 Seismic phases -- Branches of core phases -- 11.4.2 Normal mode frequencies -- Observations of modal eigenfrequencies -- 11.4.3 Comparison with observations -- 11.4.4 Imaging three-dimensional structure -- 11.5 Earthquakes and faulting -- 12 Lithospheric Deformation -- 12.1 Definitions of the lithosphere -- 12.2 Thermal and mechanical structure -- 12.2.1 Thermal conduction in the oceanic lithosphere -- 12.2.2 Mechanical deformation -- 12.2.3 Estimates of the elastic thickness of the lithosphere -- 12.2.4 Strength envelopes and failure criteria -- Oceanic lithosphere -- Continental lithosphere -- 12.3 Plate boundaries and force systems -- 12.3.1 Nature of plate boundaries -- 12.3.2 Plate boundary forces -- 12.4 Measures of stress and strain -- 12.4.1 Stress measurements -- 12.4.2 Strain measurements -- 12.5 Glacial rebound -- 12.6 Extension and convergence -- 12.6.1 Extension -- 12.6.2 Convergence -- 13 The Influence of Rheology: Asthenosphere to the Deep Mantle -- 13.1 Lithosphere and asthenosphere -- 13.1.1 Seismic imaging -- 13.1.2 Seismic attenuation -- 13.1.3 Seismic anisotropy -- Surface wave anisotropy -- 13.1.4 Asthenospheric flow -- 13.1.5 The influence of a low-viscosity zone -- 13.2 Subduction zones and their surroundings -- 13.2.1 Configuration of subduction zones -- 13.2.2 Flow around the slab -- 13.2.3 Temperatures in and around the subducting slab -- 13.2.4 Subduction and orogeny -- 13.3 The influence of phase transitions -- Impact of phase transitions on subduction -- 13.4 The deeper mantle -- 13.4.1 Viscosity variations in the mantle and the geoid -- Dynamic compensation -- Spectral representation -- 13.4.2 Material properties -- 13.4.3 The lower boundary layer. , 14 Mantle Convection -- 14.1 Convective forces -- 14.1.1 Boundary layer theory -- 14.1.2 Basic equations -- 14.1.3 Boundary conditions -- 14.1.4 Non-dimensional treatment -- 14.1.5 Computational convection -- 14.2 Convective planform -- 14.3 Thermal structure and heat budget -- 14.3.1 Thermal boundary layers and the geotherm -- Adiabatic gradient -- Heat sources -- Subadiabaticity -- 14.3.2 Plates -- Heat transport -- Influence on mantle flow -- 14.3.3 Hot spots and plumes -- Hot spot swells -- Hot Spot reference frame -- Plume excess temperature and global mantle heat budget -- 14.4 Circulation of the mantle -- 14.4.1 Present-day and past plate motion models -- 14.4.2 Implications of plate motion models for mantle circulation -- 14.4.3 Mantle circulation models -- Heterogeneity pattern -- Adjoint mantle circulation models -- 14.5 Mantle rheology -- 14.5.1 Temperature dependence -- 14.5.2 Strain dependence -- 14.6 Coupled lithosphere-mantle convection models -- 14.7 Thermochemical convection -- 15 The Core and the Earth's Dynamo -- 15.1 The magnetic field at the surface and at the top of the core -- 15.2 Convection and dynamo action -- 15.2.1 Basic equations -- Reference state -- 15.2.2 Boundary conditions -- 15.2.3 Interaction of the flow with the magnetic field -- 15.2.4 Deviations from the reference state -- 15.2.5 Non-dimensional treatment -- Induction equation -- Geostrophy and Taylor Columns -- 15.3 Numerical dynamos -- 15.4 Evolution of the Earth's core -- 15.4.1 Energy balance -- 15.4.2 Thermal and compositional effects -- 15.4.3 Inner core growth in a well-mixed core -- Appendix: Table of Notation -- Stress and Strain -- Solids and Fluids -- Waves -- Thermodynamic Quantities -- Non-dimensional Quantities for Fluids -- Electromagnetic -- Quantum/Atomic -- Deformation -- Seismology -- Core dynamics -- Mathematical -- Bibliography. , Reference Texts.
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  • 2
    Publication Date: 2017-07-24
    Description: TOPO-EUROPE addresses the 4-D topographic evolution of the orogens and intra-plate regions of Europe through a multidisciplinary approach linking geology, geophysics, geodesy and geotechnology. TOPO-EUROPE integrates monitoring, imaging, reconstruction and modelling of the interplay between processes controlling continental topography and related natural hazards. Until now, research on neotectonics and related topography development of orogens and intra-plate regions has received little attention. TOPO-EUROPE initiates a number of novel studies on the quantification of rates of vertical motions, related tectonically controlled river evolution and land subsidence in carefully selected natural laboratories in Europe. From orogen through platform to continental margin, these natural laboratories include the Alps/Carpathians–Pannonian Basin System, the West and Central European Platform, the Apennines–Aegean–Anatolian region, the Iberian Peninsula, the Scandinavian Continental Margin, the East-European Platform, and the Caucasus–Levant area. TOPO-EUROPE integrates European research facilities and know-how essential to advance the understanding of the role of topography in Environmental Earth System Dynamics. The principal objective of the network is twofold. Namely, to integrate national research programs into a common European network and, furthermore, to integrate activities among TOPO-EUROPE institutes and participants. Key objectives are to provide an interdisciplinary forum to share knowledge and information in the field of the neotectonic and topographic evolution of Europe, to promote and encourage multidisciplinary research on a truly European scale, to increase mobility of scientists and to train young scientists. This paper provides an overview of the state-of-the-art of continental topography research, and of the challenges to TOPO-EUROPE researchers in the targeted natural laboratories
    Type: Article , PeerReviewed
    Format: text
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  • 3
    Publication Date: 2013-01-11
    Description: Plane-layer geometry convection models remain a useful tool for investigating planetary mantle dynamics but yield significantly warmer geotherms than spherical-shell systems. Comparisons of uniform property plane-layer and spherical-shell models have provided insight into the role of geometry on temperature in convecting systems but the inclusion of first-order terrestrial characteristics is needed to quantitatively assess the influence of system geometry on more relevant mantle models. Here, we analyse the mean temperatures of over 160 spherical-shell and plane-layer convection models featuring a uniform upper-mantle viscosity and a lower mantle that increases in viscosity by a factor of 30 or 100. With the imposition of the stratified viscosity, an effective Rayleigh number, $Ra_{\overline{\eta }}$ , is defined based on the average viscosity of the mantle. We derive equations for the relationship between the mean temperature, , $Ra_{\overline{\eta }}$ and the non-dimensional internal heating rate, H , for both convection in a spherical shell with Earth-like mantle geometry and plane-layer solution domains. These equations predict the mean temperatures in the corresponding systems to an accuracy of a few percent or better. Our equations can be combined to derive the appropriate heating rate for a plane-layer convection model to emulate the temperatures in a mixed heating mode spherical-shell convection model with effective Rayleigh number comparable to the Earth's value, or greater. When comparing cases with the same internal heating rate and effective Rayleigh number, we find that the increased lower mantle viscosity amplifies the mean temperature ratio of the plane-layer and spherical-shell systems relative to isoviscous convection. These findings imply that the disagreement between spherical-shell mantle convection and plane-layer geometry mantle convection thermal structure must be particularly accounted for in plane-layer geometry models featuring variable viscosities.
    Print ISSN: 0956-540X
    Electronic ISSN: 1365-246X
    Topics: Geosciences
    Published by Oxford University Press on behalf of The Deutsche Geophysikalische Gesellschaft (DGG) and the Royal Astronomical Society (RAS).
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