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  • 1
    Monograph available for loan
    Monograph available for loan
    Berlin [u.a.] : Springer
    Associated volumes
    Call number: MOP 46441 / Mitte
    In: Physics and chemistry in space
    Type of Medium: Monograph available for loan
    Pages: IX, 205 S. : graph. Darst.
    ISBN: 3540135103 , 0-387-13510-3
    Series Statement: Physics and chemistry in space 11
    Location: MOP - must be ordered
    Branch Library: GFZ Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    Braunschweig [u.a.] : Vieweg
    Associated volumes
    Call number: AWI A15-98-0097
    In: Sammlung Vieweg
    Type of Medium: Monograph available for loan
    Pages: 232 S.
    Series Statement: Sammlung Vieweg 127
    Branch Library: AWI Library
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  • 3
    Monograph available for loan
    Monograph available for loan
    Dordrecht [u.a.] : Kluwer
    Call number: M 93.1059 ; AWI A6-92-0298 ; M 93.1094
    Description / Table of Contents: Atmospheric Tidal and Planetary Waves is written for workers in the fields of meteorology, climatology, aeronomy and space physics, and deals in a unified way with global scale dynamical processes within the lower, middle, and upper atmosphere. lrregular ultralong planetary waves with periods ranging from a few days to a few years are considered, as well as regular large-scale waves with basic periods of one (solar or lunar) day and one year, and the climatic mean flow (lumped together as tidal waves). The basic concept is the separation of the atmospheric flow into eigenmodes on a sphere (Hough functions). The sources and the meridional and vertical structure of these modes are discussed in detail, and Observations of tidal and planetary waves within the lower, middle, and upper atmosphere are interpreted in terms of Hough modes. The effects of nonlinear wave-wave interactions are outlined.
    Type of Medium: Monograph available for loan
    Pages: X, 348 S. , graph. Darst.
    ISBN: 9027726302
    Series Statement: Atmospheric sciences library 12
    Classification:
    Geodynamics
    Language: English
    Note: Table of Contents: Preface. - Chapter 1. lntroduction. - Chapter 2. Basic Equations. - 2.1. Hydrodynamic and Thermodynamic Equations. - 2.2. Equations of the Mean Flow. - 2.3. Equations of the Eddies. - 2.4. Energy Balance. - 2.5. Vorticity and Divergence. - 2.6. Linearization. - 2.7. Eliassen-Palm Flux. - 2.8. Ertel Potential Vorticity. - 2.9. Diffusive Separation of Atmospheric Constituents. - 2.10. Spherical Harmonics. - 2.11. Hermite Functions. - Chapter 3. External Energy Sources. - 3.1. Solar Irradiance. - 3.2. Solar Heat Input into Upper Atmosphere. - 3.3. Solar Heat Input into Lower and Middle Atmosphere. - 3.4. Lunar Gravitational Tidal Energy. - 3.5. Solar Wind Energy. - Chapter 4. Internal Energy Sources and Sinks. - 4.1. Eddy Viscosity. - 4.2. Eddy Heat Conduction. - 4.3. Latent Heat. - 4.4. Newtonian Cooling. - 4.5. Rayleigh Friction. - 4.6. Ion Drag. - 4.7. Feedback between Large-Scale Eddies and Mean Flow. - Chapter 5. Horizontal Modal Structure. - 5.1. Separation of Variables. - 5.2. Eigenvalues of Laplace's Equations. - 5.3. Gravity Waves. - 5.4. Rossby- Haurwitz Waves. - 5.5. Kelvin Waves and Yanai Waves. - 5.6. Low Frequency Waves with Positive Eigenvalues. - 5.7. Class Il Waves of Wavenumber m = 0. - 5.8. Diurnal Tides. - 5.9. Dynamo Action of Tidal Winds. - 5.10. Rossby Waves Migrating within Mean Zonal Flow. - 5.11. Influence of Zonal Mean Flow on Rossby-Haurwitz Waves. - 5.12. Salutions of Inhomogeneous Laplace Equations. - Chapter 6. Vertical Modal Structure. - 6.1. Characteristic Waves. - 6.2. Vertical Wavenumber. - 6.3. Particular Salutions. - 6.4. Boundary Conditions. - 6.5. Normal Modes. - 6.6. Height Structure of External Waves. - 6.7. Directly Driven Circulation Cells. - 6.8. Indirectly Driven Circulation Cells. - 6.9. Height Structure of Internal Waves. - 6.10. Impulsive Heat Input. - 6.11. Ray Tracing of Rossby Waves. - 6.12. Mode Conversion. - 6.13. Baroclinic Instability. - Chapter 7. Nonlinear Wave Propagation. - 7.1. Nonlinear Coupling between Rossby- Haurwitz Waves. - 7.2. Analytic Salutions for Weak Coupling of Rossby-Haurwitz Waves. - 7.3. Rossby- Haurwitz Wave Coupling in Realistic Mean Flow. - 7.4. Homogeneous and Isotropic Turbulence. - 7.5. Space-Time Analysis. - 7.6. Nonlinear Normal Mode Initialization. - 7.7. Lorenz Attractor. - 7.8. Logistic Difference Equation. - 7.9. Multiple Equilibria. - Chapter 8. Tidal Waves. - 8.1. Seasonal Tides within Lower and Middle Atmosphere (m = 0). - 8.2. Quasi-Stationary Seasonal Waves (m 〉 0). - 8.3. Climatic Mean Flow. - 8.4. Seasonal Tides within Upper Atmosphere. - 8.5. Migrating Solar Diurnal Tides within Lower and Middle Atmosphere. - 8.6. Migrating Solar Diurnal Tides within Upper Atmosphere. - 8.7. Nonmigrating Solar Diurnal Tides. - 8.8. Lunar Tides. - 8.9. Electromagnetic Effects of Tidal Waves. - 8.10. Energy and Momentum Deposition of Solar Diurnal Tides. - Chapter 9. Planetary Waves. - 9.1. Extratropical Transients. - 9.2. Southern Oscillation. - 9.3. Forty-Day Oscillations. - 9.4. Transients in the Tropical Middle Atmosphere. - 9.5. Fluctuations of Atmospheric Angular Momentum. - 9.6. Sudden Stratospheric Warnings. - 9.7. Thermospheric Response to Solar EUV Fluctuations. - 9.8. Thermospheric Storms. - 9.9. Solar Activity Effects within Middle and Lower Atmosphere. - Chapter 10. Epilogue. - References. - Subject Index.
    Location: Upper compact magazine
    Location: AWI Reading room
    Location: Upper compact magazine
    Branch Library: GFZ Library
    Branch Library: AWI Library
    Branch Library: GFZ Library
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Naturwissenschaften 76 (1989), S. 305-309 
    ISSN: 1432-1904
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Chemistry and Pharmacology , Natural Sciences in General
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Surveys in geophysics 17 (1996), S. 101-144 
    ISSN: 1573-0956
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The theoretical aspects of the transfer of angular momentum between atmosphere and Earth are treated with particular emphasis on analytical solutions. This is made possible by the consequent usage of spherical harmonics of low degree and by the development of large-scale atmospheric dynamics in terms of orthogonal wave modes as solutions of Laplace's tidal equations. An outline of the theory of atmospheric ultralong planetary waves is given leading to analytical expressions for the meridional and height structure of such waves. The properties of the atmospheric boundary layer, where the exchange of atmospheric angular momentum with the solid Earth takes place, are briefly reviewed. The characteristic coupling time is the Ekman spin-down time of about one week. The axial component of the atmospheric angular momentum (AAM), consisting of a pressure loading component and a zonal wind component, can be described by only two spherical functions of latitude ϕ: the zonal harmonicP 2 0 (ϕ), responsible for pressure loading, and the spherical functionP 1 1 (ϕ) simulating supperrotation of the zonal wind. All other wind and pressure components merely redistributeAAM internally such that their contributions toAAM disappear if averaged over the globe. It is shown that both spherical harmonics belong to the meridional structure functions of the gravest symmetric Rossby-Haurwitz wave (0, −1)*. This wave describes retrograde rotation of the atmosphere within the tropics (the tropical easterlies), while the gravest symmetric external wave mode (0, −2) is responsible for the westerlies at midlatitudes. Applying appropriate lower boundary conditions and assuming that secular angular momentum exchange between solid Earth and atmosphere disappears, the sum of both waves leads to an analytical solution of the zonal mean flow which roughly simulates the observed zonal wind structure as a function of latitude and height. This formalism is used as a basis for a quantitative discussion of the seasonal variations of theAAM within the troposphere and middle atmosphere. Atmospheric excitation of polar motion is due to pressure loading configurations, which contain the antisymmetric functionP 2 1 (ϕ) exp(iλ) of zonal wavenumberm=1, while the winds must have a superrotation component in a coordinate system with the polar axis within the equator. The Rossby-Haurwitz wave (1, −3)* can simulate well the atmospheric excitation of the observed polar motion of all periods from the Chandler wobble down to normal modes with periods of about 10 days. Its superrotation component disappears so that only pressure loading contributes to polar motion. The solar gravitational semidiurnal tidal force acting on the thermally driven atmospheric solar semidiurnal tidal wave can accelerate the rotation rat of the Earth by about 0.2 ms per century. It is speculated that the viscous-like friction of the geomagnetic field at the boundary between magnetosphere and solar wind may be responsible for the westward drift of the dipole component of the internal geomagnetic field. Electromagnetic or mechanical coupling between outer core and mantle may then contribute to a decrease of the Earth's rotation rate.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 34 (1983), S. 327-335 
    ISSN: 1572-9672
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The ionospheric storm process at F layer heights is reviewed and an explanation in terms of wind-induced diffusion of atomic oxygen is given.
    Type of Medium: Electronic Resource
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  • 7
    Publication Date: 1983-03-01
    Print ISSN: 0038-6308
    Electronic ISSN: 1572-9672
    Topics: Physics
    Published by Springer
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  • 8
    Publication Date: 1969-01-01
    Print ISSN: 0148-0227
    Electronic ISSN: 2156-2202
    Topics: Geosciences
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  • 9
    Publication Date: 1978-01-01
    Print ISSN: 0148-0227
    Electronic ISSN: 2156-2202
    Topics: Geosciences
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  • 10
    Publication Date: 1982-03-01
    Print ISSN: 0048-6604
    Electronic ISSN: 1944-799X
    Topics: Geosciences , Physics
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