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  • 1
    Electronic Resource
    Electronic Resource
    Evolution of the upper ocean layer during daytime heating (1992)
    Springer
    Physical oceanography 3 (1992), S. 277-291 
    Details
    ISSN: 0928-5105
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract A one-dimensional model for the evolution of a near-surface layer during daytime heating is suggested. The paper considers how upward thermal fluxes and the Coriolis force affect the heated layer's vertical structure. Experiments have shown that atmospheric heat and impulse are localized in the heated layer, and that the earth's rotation causes deviation of the surface current velocity and reduction of its amplitudinal variations which do not seem to be controlled by the wind speed and depend on the layer's heat budget. Experimental data provide good agreement with model calculations.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF02197304
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    On some characteristics of insolation changes in the past and the future (1990)
    Springer
    Climatic change 5 (1990), S. 237-244 
    Details
    ISSN: 1573-1480
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Variations in terrestrial insolation, induced by perturbations of the earth's orbital parameters, are calculated for different geographical latitudes for ±100000 yr and in detail for the modern period between A.D. 1800–2100. The calculations show that short-period insolation variations occur against a background of secular variation, with an amplitude which can be comparable in magnitude to that of the 300-yr secular trend. For comparison we calculate the secular trends of insolation for Milankovich's caloric half-years for the period ±100000 yr with high time resolution. The nature of secular and short-term insolation changes is discussed for different latitudinal circles during future centuries. We conclude that orbitally-induced variations of insolation with periods of 18.6, 11.9, 5.9, 4.0, and 2.7 yr will perturb the radiation regime at the upper atmospheric boundary.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00140182
    Library Location Call Number Volume/Issue/Year Availability
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    Paper (German National Licenses)
    Fulltext
  • 3
    Electronic Resource
    Electronic Resource
    On some characteristics of insolation changes in the past and the future (1983)
    Springer
    Climatic change 5 (1983), S. 237-244 
    Details
    ISSN: 1573-1480
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Variations in terrestrial insolation, induced by perturbations of the earth's orbital parameters, are calculated for different geographical latitudes for ±100000 yr and in detail for the modern period between A.D. 1800–2100. The calculations show that short-period insolation variations occur against a background of secular variation, with an amplitude which can be comparable in magnitude to that of the 300-yr secular trend. For comparison we calculate the secular trends of insolation for Milankovich's caloric half-years for the period ±100000 yr with high time resolution. The nature of secular and short-term insolation changes is discussed for different latitudinal circles during future centuries. We conclude that orbitally-induced variations of insolation with periods of 18.6, 11.9, 5.9, 4.0, and 2.7 yr will perturb the radiation regime at the upper atmospheric boundary.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF02423520
    Library Location Call Number Volume/Issue/Year Availability
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    Paper (German National Licenses)
    Fulltext
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