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  • 1
    Call number: ZSP-690-5
    In: Research report of IHAS
    Type of Medium: Series available for loan
    Pages: 22 S. : Ill., graph. Darst.
    Series Statement: Research report of IHAS 5
    Branch Library: GFZ Library
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  • 2
    Keywords: Sun-Earth system ; space weather ; solar cycles ; solar wind ; solar activity ; sunspot ; ozone ; troposphere ; stratosphere ; Quasi-Biennial Oscillation (QBO)
    Description / Table of Contents: Early Japanese contributions to space weather research—1945-1960— / A. Nishida / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 1-22 --- Hydrodynamics, magnetohydrodynamics, and astrophysical plasmas / E. N. Parker / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 23-40 --- The 1960s—A decade of remarkable advances in middle atmosphere research / M. A. Geller / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 41-62 --- Hinode "a new solar observatory in space" / S. Tsuneta, L. K. Harra, and S. Masuda / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 63-75 --- Coronal mass ejections and space weather / N. Gopalswamy / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 77-120 / © TERRAPUB, Tokyo, 2009. No claim is made to original U.S. Government works. / [Full text] (PDF 3.9 MB) --- Magnetotail after Geotail, Interball and Cluster: Thin current sheets, fine structure, force balance and stability / L. Zelenyi, H. Malova, A. Artemyev, V. Popov, A. Petrukovich, D. Delcourt, and A. Bykov / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 121-170 --- Simulating solar 'climate' / M. Dikpati / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 171-199 --- Evidence for solar forcing: Some selected aspects / J. Beer and K. McCracken / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 201-216 --- Total solar irradiance variability: What have we learned about its variability from the record of the last three solar cycles? / C. Fröhlich / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 217-230 --- Mechanisms for solar influence on the Earth's climate / J. D. Haigh / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 231-256 --- Variability in the stratosphere: The sun and the QBO / K. Labitzke and M. Kunze / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 257-278 --- Gravity wave coupling from below: A review / R. A. Vincent / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 279-293 --- What we have learnt from CPEA (Coupling Processes in the Equatorial Atmosphere): A review / S. Fukao / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 295-336 --- Vertical coupling by the semidiurnal tide in Earth's atmosphere / J. M. Forbes / Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, / pp. 337-348
    Pages: Online-Ressource (VII, 351 Seiten)
    ISBN: 9784887041479
    Language: English
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Pure and applied geophysics 130 (1989), S. 263-275 
    ISSN: 1420-9136
    Keywords: Ozone ; planetary waves ; interhemispheric variations ; Southern Hemisphere behavior
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Four years of SBUV ozone data and NOAA/NMC temperature data are analyzed for the relations between the annual total ozone behaviour in the Northern and Southern Hemispheres and the transport of ozone by planetary waves. It is found that the interhemispheric differences in the annual variation of total ozone are well explained by the interhemispheric differences in the planetary waves and the resulting ozone transports. The annual variation of the ozone transports by the stationary waves is found to control the ozone behavior in both hemispheres. Both the day-to-day and the interannual variation in total ozone are found to be strongly related to the corresponding variability of the planetary waves.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 332 (1988), S. 584-585 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] THERE is no more controversial topic in meteorology than that of whether solar activity exerts a significant control on weather and climate. Karin Labitzke of the Free University of Berlin and Harry van Loon of the National Center for Atmospheric Research show in a provoca-tive paper1 published ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 342 (1989), S. 15-16 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] ATMOSPHERIC conditions can vary over a vast spectrum of timescales á€" extending up to the Milankovic cycles operating over millenia and forced by variations in the Earth's orbit. But James and James warn on page 53 of this issue1 against reading too much into correlations between ...
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 34 (1983), S. 359-375 
    ISSN: 1572-9672
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract It is demonstrated by means of model calculations that while the general configuration of middle atmosphere dynamics (i.e., winter westerlies and summer easterlies) is determined by differential solar heating, the deviations of the zonally-averaged temperature field from radiative equilibrium and the closure of the jet structures with increasing altitude result from the action of zonal mean momentum dissipation processes. The apparent heating and acceleration of the mean zonal state by planetary wave heat and momentum fluxes are examined using an Eulerian framework, and it is demonstrated that these are overestimates of their net effect. It is argued that since decelerations of the mean zonal flow are required in both winter and summer, and planetary waves are known to be very weak in the summer middle atmosphere, gravity waves are probably responsible for most of the middle atmosphere momentum dissipation as a result of their attenuation with height above their wave breaking altitude. Radar observations of middle atmosphere dynamics together with some theoretical work indicates that the effects of breaking gravity waves should be included in the thermodynamic equation as well as the momentum equation.
    Type of Medium: Electronic Resource
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  • 7
    Publication Date: 2002-12-26
    Print ISSN: 0148-0227
    Electronic ISSN: 2156-2202
    Topics: Geosciences
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  • 8
    Publication Date: 2016-02-01
    Description: A high–Reynolds number direct numerical simulation (DNS) is employed to explore the instability and turbulence dynamics accompanying an idealized multiscale flow that approximates such environments observed throughout the atmosphere. The DNS describes the superposition of a stable gravity wave (GW) and a stable, oscillatory, finescale shear flow that together yield significant wave–wave interactions, GW breaking, Kelvin–Helmholtz instabilities (KHI), fluid intrusions, and turbulence. Larger-scale GW breaking and KHI events account for the strongest turbulence intensities, with intrusions competing with KHI and GW breaking at smaller spatial scales and later times. These dynamics drive a series of sheet-and-layer structures in the velocity, stability, and dissipation fields that persist for many buoyancy periods. Measures of local turbulence intensities include energy dissipation rates, Ozmidov and Thorpe scales (LO and LT, respectively), and a buoyancy Reynolds number sufficient to ensure sustained, strong turbulence events. These exhibit significant variability between and within instability events of different types. The Ozmidov and Thorpe scales for individual events are employed to assess variations of their ratio, C = LO/LT, with time. The value of C is highly variable with event type and time but typically increases with time because significant fluid overturning most often precedes turbulence. The value of C determined for the entire domain varies from 0 prior to instability to approximately 2 or larger at late times, with minima (maxima) prior to (following) significant instability and turbulence events. This appears to preclude an assumption that C is constant in stratified flows, except perhaps as an event average that may depend on event type.
    Print ISSN: 0022-4928
    Electronic ISSN: 1520-0469
    Topics: Geography , Geosciences , Physics
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  • 9
    Publication Date: 1987-08-01
    Print ISSN: 0031-8949
    Electronic ISSN: 1402-4896
    Topics: Physics
    Published by Institute of Physics
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  • 10
    Publication Date: 1972-09-01
    Print ISSN: 0148-0227
    Electronic ISSN: 2156-2202
    Topics: Geosciences
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