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  • 1
    Monograph available for loan
    Monograph available for loan
    Moskva
    Call number: MOP 43464 / Mitte
    Type of Medium: Monograph available for loan
    Pages: 436 S.
    Location: MOP - must be ordered
    Branch Library: GFZ Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    Leningrad : Gidrometeoizdat
    Call number: MOP 26583
    Type of Medium: Monograph available for loan
    Pages: 171 S.
    Uniform Title: The physics of the stratosphere
    Language: Russian
    Location: MOP - must be ordered
    Branch Library: GFZ Library
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  • 3
    Monograph available for loan
    Monograph available for loan
    New York [u.a.] : Oxford Univ. Press
    Call number: AWI A10-92-0279 ; MOP 47991
    Type of Medium: Monograph available for loan
    Pages: XIII, 519 S : graph. Darst. , 24 cm
    Edition: 2nd ed.
    ISBN: 0195051343
    Note: CONTENTS: 1. INTRODUCTION. - 1.1 The nature of the problem. - 1.2 The thermal structure of the atmosphere. - 1.3 The chemical composition of the atmosphere. - Bibliography. - 2. THEORY OF RADIATIVE TRANSFER. - 2.1 Definitions. - 2.1.1 Intensity, flux, energy density. - 2.1.2 Extinction and emission. - 2.1.3 Simple scattering. - 2.2 Thermal emission. - 2.2.1 Thermodynamic equilibrium. - 2.2.2 Breakdown of thermodynamic equilibrium. - 2.2.3 The interaction between matter and radiation. - 2.2.4 Discussion of the source function. - 2.2.5 Transitions between more than two levels. - 2.3 The integral equations. - 2.3.1 Introduction. - 2.3.2 The general solution. - 2.3.3 Thermal radiation in a stratified atmosphere. - 2.3.4 Solar radiation in a stratified atmosphere. - 2.4 Approximate methods for thermal radiation. - 2.4.1 The atmospheric problem. - 2.4.2 Transparent and opaque approximations. - 2.4.3 Approximate forms for the absorption coefficient. - 2.4.4 The method of moments in three dimensions. - 2.4.5 Approximations for a stratified atmosphere. - Bibliography. - 3. VIBRATION-ROTATION SPECTRA OF GASEOUS MOLECULES. - 3.1 Introduction. - 3.2 Vibration-rotation spectra. - 3.2.1 The Hamiltonian for a semirigid molecule. - 3.2.2 The states of the harmonic-oscillator, rigid-rotator model. - 3.2.3 Selection rules and line intensities. - 3.2.4 Interactions. - 3.3 The shape of a spectral line. - 3.3.1 Introduction. - 3.3.2 The Michelson-Lorentz theory. - 3.3.3 An adiabatic model. - 3.3.4 The Anderson-Tsao-Curnutte theory. - 3.3.5 The far wings of pressure-broadened lines. - 3.3.6 Doppler effects. - 3.4 Collision-induced and polymer spectra. - 3.5 Overview. - Bibliography. - 4. BAND MODELS. - 4.1 Introduction. - 4.2 Isolated lines. - 4.2.1 Single line of Lorentz shape. - 4.2.2 Single line with a Voigt profile. - 4.3 Distributed line intensities. - 4.3.1 Distribution functions. - 4.3.2 Application to the Lorentz profile. - 4.3.3 Application to the Doppler and Voigt profiles. - 4.4 The effect of overlap. - 4.4.1 Schnaidt's model. - 4.4.2 The method of Matossi, Meyer, and Rauscher. - 4.5 Regular models. - 4.5.1 The Elsasser model for Lorentz lines. - 4.5.2 The Curtis model. - 4.5.3 The Elsasser model for the Voigt profile. - 4.6 Random models. - 4.6.1 Introduction. - 4.6.2 Constant line intensity. - 4.6.3 The general random model. - 4.6.4 Verification of the theory. - 4.7 Generalized transmission functions. - 4.7.1 Superimposed regular and random bands. - 4.7.2 Deviations from the Voigt profile. - 4.7.3 Background continuum. - 4.8 k distributions. - 4.8.1 Band models and spectral representations. - 4.8.2 Calculations of k distributions. - 4.8.3 Overlapping bands. - 4.9 Models of complete bands. - 4.9.1 Band absorption areas. - 4.9.2 Empirical models. - 4.9.3 Exponential band contour. - 4.9.4 Semiempirical treatment. - Bibliography. - 5. ABSORPTION BY ATMOSPHERIC GASES. - 5.1 Introduction. - 5.2 Nitrogen. - 5.3 Oxygen. - 5.3.1 Ultraviolet, molecular absorptions. - 5.3.2 Forbidden bands in the vibration-rotation spectrum. - 5.3.3 The "atmospheric" bands. - 5.3.4 The collision-induced spectrum. - 5.3.5 Atomic oxygen. - 5.4 Water vapor. - 5.4.1 The vibration-rotation spectrum. - 5.4.2 Listed data. - 5.4.3 Continuum absorption. - 5.5 Carbon dioxide. - 5.5.1 The vibration-rotation spectrum. - 5.5.2 Listed data. - 5.5.3 The collision-induced rotation spectrum. - 5.6 Ozone. - 5.6.1 Electronic bands. - 5.6.2 The vibration-rotation spectrum. - 5.7 Nitrous oxide, carbon monoxide, and methane. - 5.7.1 Nitrous oxide. - 5.7.2 Carbon monoxide. - 5.7.3 Methane. - Bibliography. - 6. RADIATION CALCULATIONS IN A CLEAR ATMOSPHERE. - 6.1 Introduction. - 6.1.1 Line-by-line calculations. - 6.1.2 The angular integration. - 6.1.3 The frequency integration. - 6.2 Transmission through a nonhomogeneous atmosphere. - 6.2.1 Exact solutions for constant mixing ratio. - 6.2.2 Scaling approximations. - 6.2.3 The H-C-G approximation. - 6.2.4 Correlated k. - 6.3 Topics concerning heating rates. - 6.3.1 The Chapman layer. - 6.3.2 The Curtis matrix. - 6.3.3 Calculations for the middle atmosphere. - 6.4 Approximate methods. - 6.4.1 Exchange of radiation with the boundaries. - 6.4.2 Use of emissivities. - 6.4.3 Radiation charts. - 6.5 The inverse problem for thermal radiation. - 6.5.1 The Kernel functions. - 6.5.2 A "physical" approach to retrieval. - 6.5.3 Linear analysis. - Bibliography. - 7. EXTINCTION BY MOLECULES AND DROPLETS. - 7.1 The problem in terms of the electromagnetic theory. - 7.2 Scattering functions. - 7.3 Rayleigh's solution for small particles. - 7.4 Large particles as |m̃| → 1,300. - 7.5 Geometric optics. - 7.6 The Mie theory. - 7.7 Nonspherical particles. - Bibliography. - 8. RADIATIVE TRANSFER IN A SCATTERING ATMOSPHERE. - 8.1 Introduction. - 8.2 Integrodifferential equation. - 8.2.1 Fourier series expansion. - 8.2.2 Discrete ordinates. - 8.2.3 Feautrier method. - 8.3 Interaction principle. - 8.3.1 Adding two layers. - 8.3.2 The star semigroup. - 8.3.3 Doubling and adding. - 8.3.4 Invariant imbedding. - 8.3.5 X, Y, and H functions. - 8.4 Miscellaneous methods. - 8.4.1 Successive orders of scattering. - 8.4.2 The integral equation. - 8.4.3 Monte Carlo. - 8.4.4 Distribution of path lengths. - 8.4.5 Low-order approximations for anisotropic scattering. - 8.5 Numerical results. - 8.5.1 The diffusion exponent. - 8.5.2 X, Y, and H functions. - 8.5.3 Internal radiation field. - 8.5.4 Scattering by haze. - 8.5.5 Convergence of successive scatterings. - 8.5.6 The accuracy of low-order approximations. - 8.6 Applications. - 8.6.1 Solar and thermal fluxes in stratocumulus clouds. - 8.6.2 Polarization of light reflected from Venus. - 8.6.3 Scattered light in the stratosphere. - 8.6.4 Scattered light in clear water. - 8.6.5 CO2 lines in the reflection spectrum of Venus. - 8.6.6 The color and polarization of skylight. - Bibliography. - 9. ATMOSPHERES IN RADIATIVE EQUILIBRIUM. - 9.1 Introduction. - 9.2 An elementary solution. - 9.2.1 Without solar absorption. - 9.2.2 Absorption of solar radiation. - 9.3 Nongrey atmospheres. - 9.3.1 Models without pressure broadening. - 9.3.2 Pressure broadening. - 9.3.3 Numerical methods. - 9.4 The troposphere and the stratosphere. - 9.4.1 Introductio. - 9.4.2 The troposphere and the stratosphere. - 9.4.3 Convective models. - 9.4.4 Nonlocal dissipation. - 9.4.5 Semiconvection. - 9.5 The runaway greenhouse. - 9.5.1 History of ideas. - 9.5.2 Simpson's paradox. - 9.5.3 An evolving atmosphere. - 9.5.4 Influence of the tropospheric lapse rate. - Bibliography. - 10. EVOLUTION OF A THERMAL DISTURBANCE. - 10.1 Introduction. - 10.2 The radiation eigenvalue problem. - 10.2.1 The integral equation. - 10.2.2 Spiegel's solution. - 10.2.3 Two-stream solution for a scattering atmosphere. - 10.2.4 Effect of boundaries. - 10.3 Numerical results. - 10.3.1 Ni(∞) for atmospheric bands. - 10.3.2 Special absorption laws. - 10.3.3 Radiative relaxation for earth and Mars. - 10.3.4 Nonequilibrium source functions. - 10.4 Planetary-scale relaxation. - 10.4.1 The planetary relaxation rate. - 10.4.2 The temperature of a nonrotating atmosphere. - 10.5 The Newtonian cooling approximation. - 10.5.1 Transparent and boundary-exchange approximations. - 10.5.2 Internal gravity waves. - 10.6 Solar radiation in the middle atmosphere. - Bibliography. - Appendix 1. Physical constants. - Appendix 2. Spectroscopic units. - Appendix 3. A model atmosphere. - Appendix 4. Properties of water vapor. - Appendix 5. The Planck function. - Appendix 6. The exponential integrals. - Appendix 7. The Ladenburg and Reiche function. - Appendix 8. The Elsasser function. - Appendix 9. The physical state of the sun. - 9.1 The quiet sun. - 9.2 The solar spectrum. - 9.3 The intensity of solar radiation. -
    Location: AWI Reading room
    Location: MOP - must be ordered
    Branch Library: AWI Library
    Branch Library: GFZ Library
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  • 4
    Electronic Resource
    Electronic Resource
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Environment and Resources 27 (2002), S. 1-20 
    ISSN: 1056-3466
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Energy, Environment Protection, Nuclear Power Engineering
    Notes: FAUST: Ich fuhl's, vergebens hab' ich alle Schatze Des Menschengeists auf mich herbeigerafft, Und wenn ich mich am Ende niedersetze, Quilt innerlich doch keine neue Kraft; Ich bin nicht um ein Haar breit hoher, Bin dem Unendlichen nicht naher. Goethe's Faust, Part I, lines 1810-15. 1 A dedication to research in the physical sciences together with the circumstances of World War II, led me into theoretical and observational studies of the global physical climate. For all practical purposes, I was on my own when working in Cambridge and London, England, and I went whereever my interests led me. I organized three atmospheric observatories (two in England). I have also worked at many astronomical observatories. As time progressed, I became increasingly involved in studies of atmospheric radiation as a controlling factor for the Earth's climate. I am often taken to be a specialist in atmospheric radiation, but I have never regarded it as more than an important element in climate studies. But radiative transfer and global questions did not become important for climate science until later, and in the 1950s and 1960s I found myself drawn to studies of planetary atmospheres as an arena in which my skills were of central importance. Mars and Venus were the focus of my work for many years, and I was partly responsible for launching the Pioneer Venus mission, which placed probes into the Venus atmosphere in 1978. Much later, the experience I gained in space instrumentation and in the structure of atmospheres led me back to climate science, where I started. Then my interest was in observing the climate and testing the credibility of climate predictions. I still maintain some activity in this field. Outside these research activities, I created a Center for Earth and Planetary Physics at Harvard University to take over the activities of the Blue Hill Observatory, when that Observatory ceased to be a viable facility. The purpose of the Center was to teach earth science in the context of the discipline of physical science. The Center had some notable achievements but eventually had to give way to requirements for environmental sciences in the University, a change that I regret. During my active life in the United States, I invested a great deal of effort in support of the work of the National Research Council (NRC), including many years spent on report review. I am increasingly troubled by the postmodern view of science that appears to dominate these activities. But that may be no more than a biased rosy view of the past with its exciting early experiences and hopes.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Naturwissenschaften 57 (1970), S. 10-16 
    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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  • 6
    Publication Date: 1996-01-01
    Print ISSN: 0035-9009
    Electronic ISSN: 1477-870X
    Topics: Geography , Physics
    Published by Wiley on behalf of Royal Meteorological Society.
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  • 7
    Publication Date: 1967-12-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
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  • 8
    Publication Date: 1968-05-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
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  • 9
    Publication Date: 1967-10-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
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  • 10
    Publication Date: 1976-02-01
    Print ISSN: 0032-0633
    Electronic ISSN: 1873-5088
    Topics: Geosciences , Physics
    Published by Elsevier
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