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  • 1
    Monograph available for loan
    Monograph available for loan
    Associated volumes
    Call number: 5/M 08.0033/8
    In: Treatise on geophysics
    Type of Medium: Monograph available for loan
    Pages: xi, 358 S.
    ISBN: 9780444519368
    Location: Reading room
    Branch Library: GFZ Library
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  • 2
    Monograph available for loan
    Monograph available for loan
    Cambridge : Cambridge University Press
    Call number: 5/M 02.0476 ; M 03.0559 ; PIK N 322-03-0113
    Type of Medium: Monograph available for loan
    Pages: xv, 940 S.
    Edition: 1st publ.
    ISBN: 0521798361
    Classification:
    Planetary Interiors
    Location: Reading room
    Location: Upper compact magazine
    Location: A 18 - must be ordered
    Branch Library: GFZ Library
    Branch Library: GFZ Library
    Branch Library: PIK Library
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 416 (2002), S. 591-594 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The motion of the Earth's liquid core is the geodynamo that generates the planet's magnetic field. Because the electrical conductivity of the molten iron in the core is high, the magnetic flux produced by the dynamo closely follows the fluid motions in the core. Much as oceanographers use dye to ...
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Macmillian Magazines Ltd.
    Nature 402 (1999), S. 170-173 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Numerical dynamo models have been successful in explaining the origin of the Earth's magnetic field and its secular variation by convection in the electrically conducting fluid outer core. An important component of the convection in the numerical dynamos are polar vortices beneath the ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 127 (1996), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: We present measurements of Joule heat production in a fluid gallium vortex permeated by a uniform transverse magnetic field. We find that the Joule heat production increases as the square of the imposed field intensity for weak and moderately strong magnetic fields and magnetic Reynolds numbers up to about one. For stronger magnetic fields. Lorentz forces destroy the 2-D structure of the vortex and the Joule heat production becomes nearly independent of the intensity of the imposed magnetic field. We derive scaling laws relating fluid velocity in the vortex, imposed magnetic field intensity and Joule heat production, for both low and high magnetic Reynolds number regimes. Application of these laws to magnetic induction in the Earth's fluid core indicates that Joule heat production by this mechanism is large enough to limit the intensity of magnetic fields within the core.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 118 (1994), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The influence of internal heat sources on mantle convection is investigated using numerical calculations of 2-D thermal convection in an infinite Prandtl number, incompressible fluid. The geometry is a cylindrical annulus with inner and outer radii in proportion to the whole mantle. Time-dependent calculations are made starting from random initial conditions, with Rayleigh numbers RaT (based on boundary-temperature difference) and RaH (based on internal-heat production) in the range 103≤RaT≤ 107 and 0 ≤RaH≤ 24 RaT. At fixed RaT, increasing RaH results in transitions in flow structure from steady cells, to a pattern of stationary cells with time-variable amplitude, and finally to thermally turbulent convection with a non-stationary cell count. For RaT 〈 105, the equilibrium cell-aspect ratio increases with RaH, from near unity (10-cell solution) at RaH= 0 to three (four-cell solution) at RaH= 8RaT. Above RaT= 105, the flow is fully time dependent and consists of unequal, non-stationary cells separated by migrating boundaries. Recurring plumes develop from instabilities in both the surface and the basal boundary layers, travel with and modify the large-scale circulation. For RaT 〉 105 and RaH 〉 RaT approximately, the travelling plumes disrupt the large-scale circulation, producing turbulent convection. At RaT= 107 the flow is fully developed thermal turbulence, and for RaH 〉 0, consists of a rapidly fluctuating, irregular flow driven by transient rising and sinking sheets of buoyant fluid. Large fluctuations in total kinetic energy occur in this regime, with periodicities ranging from 40 to 1400 Myr. The transition to thermal turbulence occurs in these calculations at Rayleigh numbers well below the value estimated for subsolidus convection in the mantle, suggesting thermally turbulent convection may occur in the mantle, a consequence of internal heat sources. Thermal turbulence offers an explanation for long-term fluctuations in the rate of subduction, sea-floor spreading and global volcanic activity.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 111 (1992), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The coupling between plate motions and mantle convection is investigated using a fully dynamic numerical model consisting of a thin non-Newtonian layer which is dynamically coupled to a thick Newtonian viscous layer. The non-Newtonian layer has a simple power-law rheology characterized by power-law index n and stiffness constant μp. A systematic investigation of steady, single cell configurations demonstrates that under certain conditions (n 〉 7 being one of them) the non-Newtonian layer behaves like a mobile tectonic plate. Time-dependent calculations with multicellular configurations show the ability of the plate-mantle coupling model to adjust the number of plates and their sizes in accordance with the flow in the Newtonian layer. These calculations show that the geometry and number of plates do not necessarily resemble the planform of convection below.
    Type of Medium: Electronic Resource
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  • 8
    ISSN: 1546-170X
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Medicine
    Notes: [Auszug] Thiazolidinediones (TZDs) are insulin-sensitizing drugs and are potent agonists of the nuclear peroxisome proliferator-activated receptor-γ (PPAR-γ). Although muscle is the major organ responsible for insulin-stimulated glucose disposal, PPAR-γ is more highly expressed in adipose ...
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature medicine 9 (2003), S. 1265-1266 
    ISSN: 1546-170X
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Medicine
    Notes: [Auszug] The role of the nuclear peroxisome proliferator–activated receptor (PPAR)-γ in cancer has been a subject of debate. The identification of loss-of-function mutations in PPARG in colon and prostate tumors has led to the idea that this gene may function as a tumor suppressor. We have ...
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 327 (1987), S. 409-413 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Fig. 1 Temperature contours and core-mantle boundary (CMB) topography in two simulations of the growth of convective instabilities in the D" thermal boundary layer with thermally activated viscosity. Contour interval is 40 K; vertical and horizontal axis units are 100 and 200 km respectively. The ...
    Type of Medium: Electronic Resource
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