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  • 1
    Monograph available for loan
    Monograph available for loan
    The inverse problem; II. (1985)
    Associated volumes
    Details Availability
    Call number: O 6066
    In: Glacial-isostatic adjustment
    Type of Medium: Monograph available for loan
    Pages: S. 669-706
    Location: Upper compact magazine
    Branch Library: GFZ Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    The forward problem; I. (1985)
    Associated volumes
    Details Availability
    Call number: O 6065
    In: Glacial-isostatic adjustment
    Type of Medium: Monograph available for loan
    Pages: S. 605-646
    Location: Upper compact magazine
    Branch Library: GFZ Library
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  • 3
    Monograph available for loan
    Monograph available for loan
    Mantle convection : plate tectonics and global dynamics (1989)
    New York [u.a.] : Gordon and Research Science Publ.
    Associated volumes
    Details Availability
    Call number: M 92.0777 ; M 93.0395
    In: Fluid mechanics of astrophysics and geophysics
    Type of Medium: Monograph available for loan
    Pages: VIII, 881 S.
    ISBN: 0677221207
    Series Statement: Fluid mechanics of astrophysics and geophysics
    Classification:
    Geodynamics
    Language: English
    Location: Upper compact magazine
    Location: Upper compact magazine
    Branch Library: GFZ Library
    Branch Library: GFZ Library
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  • 4
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    Abrupt Climate Transition from Snowball to Moist or Runaway Greenhouse, links to model results in NetCDF format (2017)
    PANGAEA
    In:  Supplement to: Yang, Jun; Ding, Feng; Ramirez, Ramses M; Peltier, W R; Hu, Yongyun; Liu, Yonggang (2017): Abrupt climate transition of icy worlds from snowball to moist or runaway greenhouse. Nature Geoscience, 10(8), 556-560, https://doi.org/10.1038/ngeo2994
    Details
    Publication Date: 2023-01-13
    Description: Ongoing and future space missions aim to identify potentially habitable planets in our Solar System and beyond. Planetary habitability is determined not only by a planet's current stellar insolation and atmospheric properties, but also by the evolutionary history of its climate. It has been suggested that icy planets and moons become habitable after their initial ice shield melts as their host stars brighten. Here we show from global climate model simulations that a habitable state is not achieved in the climatic evolution of those icy planets and moons that possess an inactive carbonate-silicate cycle and low concentrations of greenhouse gases. Examples for such planetary bodies are the icy moons Europa and Enceladus, and certain icy exoplanets orbiting G and F stars. We find that the stellar fluxes that are required to overcome a planet's initial snowball state are so large that they lead to significant water loss and preclude a habitable planet. Specifically, they exceed the moist greenhouse limit, at which water vapour accumulates at high altitudes where it can readily escape, or the runaway greenhouse limit, at which the strength of the greenhouse increases until the oceans boil away. We suggest that some icy planetary bodies may transit directly to a moist or runaway greenhouse without passing through a habitable Earth-like state.
    Keywords: File content; File format; File name; File size; Uniform resource locator/link to file
    Type: Dataset
    Format: text/tab-separated-values, 420 data points
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    DATA PANGAEA
  • 5
    Electronic Resource
    Electronic Resource
    Mantle Convection and Viscoelasticity (1985)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Fluid Mechanics 17 (1985), S. 561-608 
    Details
    ISSN: 0066-4189
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.fl.17.010185.003021
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  • 6
    Electronic Resource
    Electronic Resource
    Ice Age Geodynamics (1981)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Earth and Planetary Sciences 9 (1981), S. 199-225 
    Details
    ISSN: 0084-6597
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.ea.09.050181.001215
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  • 7
    Electronic Resource
    Electronic Resource
    Constraint on deep mantle viscosity from Lageos acceleration data (1983)
    [s.l.] : Nature Publishing Group
    Nature 304 (1983), S. 434-436 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The question as to the value of the Earth's viscosity beneath a depth of 670 km remains an important issue. This depth is marked by the presence of a solid-solid phase transition from the low-pressure phase spinel to the high-pressure mixture of the minerals perovskite and magnesiowustite1. Because ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/304434a0
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  • 8
    Electronic Resource
    Electronic Resource
    New constraints on transient lower mantle rheology and internal mantle buoyancy from glacial rebound data (1985)
    [s.l.] : Nature Publishing Group
    Nature 318 (1985), S. 614-617 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] A model of mantle rheology which has an explicit transient component of its relaxation spectrum is shown to reconcile two apparently conflicting inferences of lower mantle viscosity. If recent analyses of isostatic geoid anomalies are correct in requiring a large increase of viscosity with depth, ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/318614a0
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  • 9
    Electronic Resource
    Electronic Resource
    Oceanic bathymetry profiles flattened by radiogenic heating in a convecting mantle (1980)
    [s.l.] : Nature Publishing Group
    Nature 285 (1980), S. 649-651 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Ignoring horizontal conduction and assuming isostatic compensation at the base of the lithospheric plate, Parsons and McKenzie2 derived the following energy balance equation for a column through the plate: - (?m - ?w) Cp/a D/t+ qu = qb + z H'(z)dz (1) where ?m is the mantle density (below the ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/285649a0
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  • 10
    Electronic Resource
    Electronic Resource
    Quasi-geostrophic simulations of the 1979 stratospheric major warming: The importance of middle-atmospheric drag (1986)
    Springer
    Pure and applied geophysics 124 (1986), S. 1051-1085 
    Details
    ISSN: 1420-9136
    Keywords: Quasi-geostrophic model ; stratospheric major warming ; middle-atmospheric drag
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract A detailed test of a simple nonlinear quasi-geostrophic model of stratospheric sudden warming has been performed. The model is of Matsuno's type, which includes only the interaction between a single planetary wave and the zonal mean flow. Given this limitation, the 1979 major stratospheric sudden warming has been employed to test the ability of the model to simulate an actual warming event. This event proved to be an especially appropriate testing ground for the model, since its main assumptions were reasonably well satisfied by the observational evidence. Results from the model simulations demonstrate (a) that such simple quasi-geostrophic dynamics are completely capable of providing a rather detailed simulation of the 1979 major warming event and (b) that the ability of the model to simulate successfully the observed evolution of the warming is extremely sensitive to the magnitude and form of the dissipation mechanism that is assumed to operate in the middle atmosphere.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00879931
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