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  • 1
    Monograph available for loan
    Monograph available for loan
    Berlin [u.a.] : Springer
    Call number: 12/M 00.0587 ; PIK N 300-02-0401 ; PIK N 300-08-0280
    Description / Table of Contents: Contents: 1. Brief Introduction.- 2. Astronomy.- 3. Spectral Analysis.- 4. Climate proxies.- 5. Time scale and timing.- 6. Mechanisms, models and theories.- 7. Accretion climate models.- 8. Evidence.- 9. Status of our understanding.- Appendix 1. Bispectral analysis.- Appendix 2. Matlab programs.- Appendix 3. Maximum entropy plots.- Appendix 4. Websites for data.
    Type of Medium: Monograph available for loan
    Pages: ix, 318 S.
    ISBN: 185233634X , 3-540-43779-7
    Series Statement: Springer-Praxis books in environmental sciences
    Classification:
    Historical Geology
    Location: Reading room
    Location: A 18 - must be ordered
    Location: A 18 - must be ordered
    Branch Library: GFZ Library
    Branch Library: PIK Library
    Branch Library: PIK Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    Cambridge : Cambridge Univ. Press
    Call number: O 3197
    Type of Medium: Monograph available for loan
    Pages: xix, 323 S.
    Series Statement: Cambridge monographs on mechanics and applied mathematics
    Location: Upper compact magazine
    Branch Library: GFZ Library
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  • 3
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 118 (1965), S. 0 
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 377 (1995), S. 107-108 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SIR á- According to the Milankovitch theory, the 100-kyr glacial cycle is caused by changes in insolation (solar heating) brought about by variations in the eccentricity of the Earth's orbit. There are serious difficulties with this theory: the insolation variations appear to be too small to ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Macmillan Magazines Ltd.
    Nature 389 (1997), S. 777-777 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SirIn Kyoto in December, the Framework Convention on Climate Change (FCCC) is expected to be strengthened. Negotiations have focused on commitments to cut carbon dioxide (CO2), methane and nitrous oxide, the three main contributors to global warming. Two other ...
    Type of Medium: Electronic Resource
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  • 6
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    Unknown
    New York : Periodicals Archive Online (PAO)
    Journal of policy analysis and management. 7:3 (1988:Spring) 425 
    ISSN: 0276-8739
    Topics: Political Science , Economics
    Notes: Getting Warmer - Should We Worry?
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 2 (1963), S. 473-557 
    ISSN: 1572-9672
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The internal structures of the moon, Mars, Venus, and Mercury are examined in the light of what is known about the constitution of the earth. The gravitational figure of the earth as obtained from orbits of artificial satellites is used to estimate the possible deviations from hydrostatic equilibrium on other planets. Observations of the orbital and rotational motion of the moon are consistent with the hypothesis that the interior of the moon supports density inhomogeneities of the same order as those supported by the earth. The available data on the moon are insufficient to determine whether or not the moon is differentiated. The orbits of Phobos and Deimos yield an adequate value for the moment of inertia of Mars. The moment of inertia and the mass are consistent with a metallic core containing about 10 per cent of the mass of Mars. The observations of the possible magnetic field of Mars would be of importance both to the understanding of planetary magnetic fields and elucidating the internal structure of that planet. Seismic investigations on the earth yield an equation of state for silicates to pressures of about 1 × 106 bars. This equation of state is used in determining density variation within Mars. The surface heat flow for the earth is consistent with the hypothesis that the concentration of radioactive elements is the same as that in chondritic meteorites. The observed ratio of potassium to uranium in surface and near-surface rocks is not consonant with the chondritic hypothesis. The moon can be of chondritic composition only if it is differentiated with the radioactivity concentrated in the upper few hundred kilometers. A chondritic composition for Mars would require a differentiation in excess of that consistent with its mass and moment of inertia. It is concluded that a chondritic composition is not a satisfactory chemical model for the inner planets.
    Type of Medium: Electronic Resource
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  • 8
    ISSN: 1432-0878
    Keywords: Key words: Adrenal cortex ; Apoptosis ; DNA fragmentation ; DNA 3′-end labeling ; Adrenocorticotropic hormone ; Hypophysectomy ; Rat (Sprague Dawley)
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract. Adrenocortical cell apoptosis was studied by using an established in vivo model, the hypophysectomized rat, and an in vitro model, viz., rat adrenal glands in short-term organ culture. In vivo, apoptosis (biochemical autoradiographic analysis of internucleosomal DNA cleavage) was weak and not apparent until 12–24 h after hypophysectomy. In situ histochemical localization of 3′-end DNA strand breaks revealed that apoptosis in vivo occurred nearly exclusively in subpopulations of zona reticularis cells. Adrenocorticotropic hormone (ACTH) maintenance completely blocked these indices of apoptosis. By contrast, apoptosis (DNA fragmentation) in cultured rat adrenal glands without ACTH was extensive and relatively rapid, being apparent after 1 h and increasing with the duration of incubation. ACTH attenuated (by 44%) but did not completely block apoptosis in vitro. Thus, ACTH appears to be the sole pituitary hormone that forestalls apoptosis of terminally differentiated adrenocortical (zona reticularis) cells. However, the discrepancy between in vitro and in vivo models in terms of the magnitude and rate of DNA fragmentation suggests that, in vivo, other factors finely regulate the magnitude of adrenocortical apoptotic cell death.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Climatic change 16 (1990), S. 247-281 
    ISSN: 1573-1480
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Methane clathrates are stable at depths greater than about 200 m in permafrost regions and in ocean sediments at water depths greater than about 250 m, provided bottom waters are sufficiently cold. The thickness of the clathrate stability zone depends on surface temperature and geothermal gradient. Average stability zone thickness is about 400 m in cold regions where average surface temperatures are below freezing, 500 m in ocean sediments, and up to 1,500 m in regions of very cold surface temperature (〈-15 °C) or in the deep ocean. The concentration of methane relative to water within the zone of stability determines whether or not clathrate will actually occur. The geologic setting of clathrate occurrences, the isotopic composition of the methane, and the methane to ethane plus propane ratio in both the clathrates and the associated pore fluids indicate that methane in clathrates is produced chiefly by anaerobic bacteria. Methane occurrences and the organic carbon content of sediments are the bases used to estimate the amount of carbon currently stored as clathrates. The estimate of about 11,000 Gt of carbon for ocean sediments, and about 400 Gt for sediments under permafrost regions is in rough accord with an independent estimate by Kvenvolden of 10,000 Gt. The shallowness of the clathrate zone of stability makes clathrates vulnerable to surface disturbances. Warming by ocean flooding of exposed continental shelf, and changes in pressure at depth, caused, for example, by sea-level drop, destabilize clathrates under the ocean, while ice-cap growth stabilizes clathrates under the ice cap. The time scale for thermal destabilization is set by the thermal properties of sediments and is on the order of thousands of years. The time required to fix methane in clathrates as a result of surface cooling is much longer, requiring several tens of thousands of years. The sensitivity of clathrates to surface change, the time scales involved, and the large quantities of carbon stored as clathrate indicate that clathrates may have played a significant role in modifying the composition of the atmosphere during the ice ages. The release of methane and its subsequent oxidation to carbon dioxide may be responsible for the observed swings in atmospheric methane and carbon dioxide concentrations during glacial times. Because methane and carbon dioxide are strong infrared absorbers, the release and trapping of methane by clathrates contribute strong feedback mechanisms to the radiative forcing of climate that results from earth's orbital variations.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Climatic change 42 (1999), S. 633-662 
    ISSN: 1573-1480
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Sulfur hexafluoride (SF6), perfluoromethane (CF4) and perfluoroethane (C2F6) are strong greenhouse gases with long (〉1000 year) atmospheric residence times. We derive emission factors for the major anthropogenic sources and project future emissions for 5 regions and the world. Although firms in many industrialized countries are already limiting emissions, without further policy intervention global emissions will rise 150% (CF4 and C2F6) and 210% (SF6) between 1990 and 2050; radiative forcing will increase 0.026 W m-2. Full application of available low-cost and costless policies in industrialized nations would cut that radiative forcing by one-quarter. Increased forcing due to these gases is small (〈2%) relative to other gases but permanent on the timescale of human civilization. We also quantify plausible manipulations to governmental data that will be used to determine compliance with the 1997 Kyoto Protocol, which includes commitments for industrialized countries to regulate these and other greenhouse gases. More complete and transparent data are urgently needed. West European nations, for example, can ‘cut’ their emissions of these gases by half by 2010 simply by manipulating emission factors within the current bounds of uncertainty.
    Type of Medium: Electronic Resource
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