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  • 1
    UID:
    gbv_027303993
    Format: XV, 485 S. , Ill., graph. Darst.
    ISBN: 0387964754 , 3540964754
    Series Statement: Applied mathematical sciences 60
    Note: Literaturverz. S. 453 - 479
    Additional Edition: Online-Ausg. Ghil, Michael Topics in Geophysical Fluid Dynamics: Atmospheric Dynamics, Dynamo Theory, and Climate Dynamics New York, NY : Springer, 1987 ISBN 9781461210528
    Language: English
    Subjects: Physics
    RVK:
    RVK:
    Keywords: Atmosphäre ; Dynamik ; Klima ; Dynamotheorie
    Author information: Ghil, Michael
    Library Location Call Number Volume/Issue/Year Availability
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  • 2
    UID:
    almahu_9947363001002882
    Format: XV, 512 p. , online resource.
    ISBN: 9781461210528
    Series Statement: Applied Mathematical Sciences, 60
    Content: The vigorous stirring of a cup of tea gives rise, as we all know, to interesting fluid dynamical phenomena, some of which are very hard to explain. In this book our "cup of tea" contains the currents of the Earth's atmosphere, oceans, mantle, and fluid core. Our goal is to under­ stand the basic physical processes which are most important in describing what we observe, directly or indirectly, in these complex systems. While in many respects our understanding is measured by the ability to predict, the focus here will be on relatively simple models which can aid our physical intuition by suggesting useful mathematical methods of investiga­ tion. These elementary models can be viewed as part of a hierarchy of models of increasing complexity, moving toward those which might be use­ fully predictive. The discussion in this book will deal primarily with the Earth. Interplanetary probes of Venus, Mars, Jupiter and Saturn have revealed many exciting phenomena which bear on geophysical fluid dynamics. They have also enabled us to see the effect of changing the values of certain parameters, such as gravity and rotation rate, on geophysical flows. On the other hand, satellite observations of our own planet on a daily and hourly basis have turned it into a unique laboratory for the study of fluid motions on a scale never dreamt of before: the motion of cyclones can be observed via satellite just as wing tip vortices are studied in a wind tunnel.
    Note: I. Fundamentals -- 1. Effects of Rotation -- 2. Effects of Shallowness -- 3. The Quase-Geostrophic Approximation -- II. Large-Scale Atmospheric Dynamics -- 4. Effects of Stratification Baroclinic Instability -- 5. Changing Flow Patterns and Successive Bifurcations -- 6. Persistent Anomalies, Blocking and Predictability -- III. Dynamo Theory -- 7. Models of Geomagnetism: A Survey -- 8. Kinematic Dynamo Theory -- 9. The Hydrodynamic Basis of Geomagnetism -- IV. Theoretical Climate Dynamics -- 10. Radiation Balance and Equilibrium Models -- 11. Glaciation Cycles: Phenomenology and Slow Processes -- 12. Climatic Oscillators -- References.
    In: Springer eBooks
    Additional Edition: Printed edition: ISBN 9780387964751
    Language: English
    Library Location Call Number Volume/Issue/Year Availability
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  • 3
    UID:
    b3kat_BV042419727
    Format: 1 Online-Ressource (XV, 512p. 143 illus)
    ISBN: 9781461210528 , 9780387964751
    Series Statement: Applied Mathematical Sciences 60
    Note: The vigorous stirring of a cup of tea gives rise, as we all know, to interesting fluid dynamical phenomena, some of which are very hard to explain. In this book our "cup of tea" contains the currents of the Earth's atmosphere, oceans, mantle, and fluid core. Our goal is to understand the basic physical processes which are most important in describing what we observe, directly or indirectly, in these complex systems. While in many respects our understanding is measured by the ability to predict, the focus here will be on relatively simple models which can aid our physical intuition by suggesting useful mathematical methods of investigation. These elementary models can be viewed as part of a hierarchy of models of increasing complexity, moving toward those which might be usefully predictive. The discussion in this book will deal primarily with the Earth. Interplanetary probes of Venus, Mars, Jupiter and Saturn have revealed many exciting phenomena which bear on geophysical fluid dynamics. They have also enabled us to see the effect of changing the values of certain parameters, such as gravity and rotation rate, on geophysical flows. On the other hand, satellite observations of our own planet on a daily and hourly basis have turned it into a unique laboratory for the study of fluid motions on a scale never dreamt of before: the motion of cyclones can be observed via satellite just as wing tip vortices are studied in a wind tunnel
    Language: English
    Keywords: Dynamik ; Geophysik ; Geophysik ; Strömungsmechanik ; Hydrodynamik ; Geophysik
    Author information: Ghil, Michael
    Library Location Call Number Volume/Issue/Year Availability
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