The sixth volume of the series "Physics and Evolution of the Earth's Interior" focuses on the mature evolution of the Earth's interior. Three closely coupled branches of Earth sciences are presented. These are: paleomagnetism, plate tectonics and mantle convection theory. Their mutual connections are described and the mantle stresses driving the evolution processes are discussed. Paleomagnetism not just provides crucial data confirming the plate tectonics. In a similar way, plate tectonics gives the best evidence of the mantle convection process. Mantle convection is a leading subject of the book. Both the observational and theoretical approach to mantle convection are presented. The observational approach includes the paleomagnetism backing the plate tectonics theory, methods of interpretation of the gravity data and seismic tomography. The motion of the lithospheric plates described by plate tectonics is a surface manifestation of the convective flow. The gravity data, after some assumptions, could be a source of information about the density distribution in the mantle. This is of special value because the density distribution is included directly in the equation of motion for fluid. The seismic tomography provides the data about distribution of seismic wave velocities and seismic anisotropy. Wave velocities data can be interpreted in terms of density distribution whereas seismic anisotropy data indicate the direction of convective flow. Theoretical approach to the mantle convection includes the equations of fluid dynamics, mathematical methods for its handling and a review of the various convection models. The mantle convector is also a source of stresses in the lithosphere. This subject and coupled phenomena are also discussed in the volume. The other extensively discussed subjects are plate tectonics and paleomagnetism. Another way of investigation of Earth's evolution is offered by thermodynamics of the irreversible processes. It is the subject of Chapter 7.
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Hardcover. Condición: Good. Oversized cloth hardcover, xiii + 469 pages, NOT ex-library. Shipping weight over 1kg. Page edges affected by extensive age-spotting; erased pencil number on the rear endpaper. Else little wear. Book is clean and bright with unmarked text, free of inscriptions and stamps, firmly bound; contents are not tanned. Dust jacket with two short tears, a bit of edgewear, faint shelfwear. -- This volume offers an integrated and scientifically rigorous examination of the Earth's dynamic evolution, concentrating on its internal structure, energy flow and tectonic behaviour from a geophysical and thermodynamic perspective. It begins with an updated overview of plate tectonics, reviewing the evolution of the theory from early continental drift models to the present consensus on lithospheric plate motion, spreading, collision and subduction. Through detailed paleomagnetic data and reconstructions, the authors trace the trajectories of continents across geological time, establishing a foundation for modelling crustal deformation and intraplate stresses. A major portion of the volume is dedicated to the structure and dynamics of the mantle, with emphasis on large-scale convection. Drawing on seismic tomography and gravity field analysis, the authors differentiate upper and lower mantle processes, discuss the layered nature of mantle convection and consider the implications of these flows for surface tectonics and thermal evolution. The existence of deep mantle plumes, the potential for whole-mantle versus layered convection and the mechanical coupling between lithosphere and asthenosphere are all examined with reference to observational datasets and numerical models. Another key theme is the stress field of the lithosphere. The book analyses stress using three independent approaches: theoretical modelling based on mechanical and thermal structure; inference from surface observables such as gravity and topography; and inversion of seismic moment tensors. These methodologies converge to reveal a complex picture of stress propagation from mantle convection to crustal deformation, highlighting the interconnection of deep processes with observable tectonic phenomena like rifting, subduction and orogenic compression. Thermodynamic principles are used to address irreversible processes such as mantle differentiation, core formation and secular cooling. The authors explore how non-equilibrium thermodynamics and entropy production models can be applied to long-term geological processes, particularly to explain self-organisation, internal ordering and the emergence of structured heterogeneities in the Earth's interior. Core-mantle interactions and the role of chemical stratification in the lower mantle are also addressed through both theoretical and empirical lenses. Later chapters return to the observational record, using paleomagnetic and geomagnetic data to track Earth's field reversals, secular variation and the geodynamo process. This links outer core dynamics to observable magnetic signatures, offering a valuable window into deep-Earth processes. The study also includes comparisons with other terrestrial bodies, such as the Moon and Mars, highlighting differences in thermal history, tectonic activity and interior evolution that inform our understanding of Earth's uniqueness in the solar system. Throughout, the volume maintains a focus on integrating geophysical, thermodynamic and geochemical data with advanced computational methods. Its broad scope makes it highly relevant for geoscientists working on mantle dynamics, tectonic modelling, planetary geology and Earth system science. Appendices provide detailed data on tectonic plate motion, stress tensors, gravity anomalies and heat flow, making the work a useful reference for both researchers and graduate students. The book synthesises decades of research to offer a coherent model of the Earth's long-term evolution, linking deep interior processes with surface dynamics and planetary context. Nº de ref. del artículo: 011284
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