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This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and experimental approaches, cross-fertilizations have remained marginal. Going beyond the state of the art, the book provides readers with a global introduction and an up-to-date overview of relevant studies, fully addressing the wide range of disciplines and methods involved. The content builds on the CISM course “Fluid mechanics of planets and stars”, held in April 2018, which was part of the research project FLUDYCO, supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program.
Fluid mechanics. --- Fluids. --- Geophysics. --- Atmospheric sciences. --- Planetary science. --- Engineering Fluid Dynamics. --- Fluid- and Aerodynamics. --- Geophysics/Geodesy. --- Atmospheric Sciences. --- Planetary Sciences.
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This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and experimental approaches, cross-fertilizations have remained marginal. Going beyond the state of the art, the book provides readers with a global introduction and an up-to-date overview of relevant studies, fully addressing the wide range of disciplines and methods involved. The content builds on the CISM course “Fluid mechanics of planets and stars”, held in April 2018, which was part of the research project FLUDYCO, supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program.
Fluid mechanics. --- Fluids. --- Geophysics. --- Atmospheric sciences. --- Planetary science. --- Engineering Fluid Dynamics. --- Fluid- and Aerodynamics. --- Geophysics/Geodesy. --- Atmospheric Sciences. --- Planetary Sciences.
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This state-of-the-art reference work includes over 15 sections dealing with all aspects of exoplanets and exobiology research, including historic aspects, the Solar System as a template, objects at the planet-to-star transition, exoplanet detection and characterization with related instrumentation, technology and software tools, planet and planet-system statistics with recent and planned surveys, their atmosphere and formation and evolution processes, habitability and exobiology implications, and outlooks for future exploration and science development, including visionary contributions. Each section has 10-20 contributions written by the top experts in their subject, including both senior researchers as well as young, smart researchers who represent the future of the discipline. All in all, this handbook comprehensively tackles one of the most challenging and dynamic fields of modern astronomy and astrophysics. .
Observations, Astronomical. --- Astronomy—Observations. --- Astrobiology. --- Planetology. --- Astrophysics. --- Atmospheric sciences. --- Meteorology. --- Astronomy, Observations and Techniques. --- Astrophysics and Astroparticles. --- Atmospheric Sciences.
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This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and experimental approaches, cross-fertilizations have remained marginal. Going beyond the state of the art, the book provides readers with a global introduction and an up-to-date overview of relevant studies, fully addressing the wide range of disciplines and methods involved. The content builds on the CISM course “Fluid mechanics of planets and stars”, held in April 2018, which was part of the research project FLUDYCO, supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program.
Fluid mechanics. --- Fluids. --- Geophysics. --- Atmospheric sciences. --- Planetary science. --- Engineering Fluid Dynamics. --- Fluid- and Aerodynamics. --- Geophysics/Geodesy. --- Atmospheric Sciences. --- Planetary Sciences.
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This book gathers peer-reviewed research articles on recent advances concerning the geology, geophysics, tectonics, geochronology, sedimentology, igneous petrology, paleo-climate and paleo-oceanography of the Andaman and Nicobar Islands of India and the adjoining ocean basins. Accordingly, it contributes significantly to readers’ understanding of the origin and evolution of the Andaman subduction zone and its various components. It also provides much-needed information on the evolution of the South Asian monsoon system since the Eocene and its link to Himalayan weathering and erosion.
Geophysics. --- Structural geology. --- Atmospheric sciences. --- Geophysics/Geodesy. --- Structural Geology. --- Atmospheric Sciences. --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Geotectonics --- Structural geology --- Tectonics (Geology) --- Physical geology --- Geological physics --- Terrestrial physics --- Physics --- Geology. --- Geognosy --- Geoscience --- Natural history
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Atmospheric science --- Weather --- Climatology --- Weather. --- Climatology. --- Atmospheric science. --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Climate --- Climate science --- Climate sciences --- Science of climate --- Meteorology --- atmospheric sciences --- climate dynamics --- meteorology
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The past few decades have witnessed the explosive growth of Earth Sciences in the pursuit of knowledge and understanding the planet Earth. Such a development addresses the challenging endeavour to enrich human lives with bounding Nature as well as to preserve the Planet Earth, the Moon, the other planets, in total the Cosmos, for generations to come. Geodetic Sciences aspires to define and quantify the internal structure, the surface structure, the Oceans and the Atmosphere as well as the exterior - interior structure of the planets. Basic principles of Physics and Astronomy, namely the Static Gravity Field, the time-varying Gravity Field, in short Gravitodynamics, of the Earth and the other planets, the complex rotational motion for rigid bodies as well as deforming bodies of the Earth, The Moon, the Sun, and the planets and their moons and on top the time-varying Topography open a fascination Arena of Geodetic Sciences.
Geophysics. --- Remote sensing. --- Geotechnical engineering. --- Astronomy. --- Astrophysics. --- Atmospheric sciences. --- Geophysics/Geodesy. --- Geophysics and Environmental Physics. --- Remote Sensing/Photogrammetry. --- Geotechnical Engineering & Applied Earth Sciences. --- Astronomy, Astrophysics and Cosmology. --- Atmospheric Sciences.
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Atmospheric science --- Meteorology --- Atmospheric science. --- Meteorology. --- Aerology --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Science de l'atmosphère --- Météorologie --- Meteorology. Climatology
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The book (COST Action Final report) summarises the proceedings from COST Action ES1206. COST Action ES1206, Advanced GNSS Tropospheric Products for Severe Weather Events and Climate (GNSS4SWEC), was a 4-year project, running from 2013 to 2017, which coordinated new and improved capabilities from concurrent developments in GNSS, meteorological and climate communities. For the first time, the synergy of multi-GNSS constellations was used to develop new, more advanced tropospheric products, exploiting the full potential of multi-GNSS on a wide range of temporal and spatial scales - from real-time products monitoring and forecasting severe weather, to the highest quality post-processed products suitable for climate research. The Action also promoted the use of meteorological data as an input to real-time GNSS positioning, navigation, and timing services and has stimulated knowledge and data transfer throughout Europe and beyond. .
Earth System Sciences. --- Atmospheric Sciences. --- Global Positioning System. --- Global Navigation Satellite System --- GNSS (Navigational system) --- GPS (Navigational system) --- Navigation Satellite Timing and Ranging Global Positioning System --- NAVSTAR GPS --- Artificial satellites in navigation --- Mobile geographic information systems --- Physical geography. --- Atmospheric sciences. --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Geography
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This book examines the origins and dynamical characteristics of atmospheric inertia-gravity waves in the Antarctic mesosphere. Gravity waves are relatively small-scale atmospheric waves with a restoring force of buoyancy that can transport momentum upward from the troposphere to the middle atmosphere. In previous studies, the dynamical characteristics of mesospheric gravity waves have not been fully examined using numerical simulations, since performing a numerical simulation with a high resolution and a high model-top requires considerable computational power. However, recent advances in computational capabilities have allowed us to perform numerical simulations using atmospheric general circulation models, which cover the troposphere to the mesosphere with a sufficiently fine horizontal resolution to resolve small-scale gravity waves. The book first describes the simulation of mesospheric gravity waves using a high-resolution non-hydrostatic atmospheric model with a high model top. The accuracy of the numerical results was confirmed by the first Mesosphere-Stratosphere-Troposphere/Incoherent Scattering (MST/IS) radar observation in the Antarctic. It also depicts the origins and propagation processes of mesospheric gravity waves on the basis of the results of the high-resolution numerical model. The behaviors of mesospheric gravity waves can be clearly explained using both fundamental and cutting-edge theories of fluid dynamics.
Geophysics. --- Computer simulation. --- Atmospheric sciences. --- Fluids. --- Geophysics and Environmental Physics. --- Geophysics/Geodesy. --- Simulation and Modeling. --- Atmospheric Sciences. --- Fluid- and Aerodynamics. --- Hydraulics --- Mechanics --- Physics --- Hydrostatics --- Permeability --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Computer modeling --- Computer models --- Modeling, Computer --- Models, Computer --- Simulation, Computer --- Electromechanical analogies --- Mathematical models --- Simulation methods --- Model-integrated computing --- Geological physics --- Terrestrial physics --- Gravity waves. --- Hydrodynamics --- Waves
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