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    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Geophysical Research Letters Vol. 27, No. 19 ( 2000-10), p. 3125-3128
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 27, No. 19 ( 2000-10), p. 3125-3128
    Abstract: The effects of gravitational coupling between the inner core and the mantle are incorporated into numerical simulations of the geodynamo. Differential rotation between the inner core and the mantle is permitted by allowing the inner core to viscously deform. Calculations with a deformation time scale of 1 yr, corresponding to an average viscosity of 5 × 10 16 Pa s, predict eastward rotation of the inner core with a mean rate of 0.02deg/yr relative to the mantle. Fluctuations about this mean rate of rotation occur with a typical period of 75 yr and have sufficient amplitude to explain observed changes in length of day at decadal periods. When gravitational coupling is removed, or viscous coupling is added by imposing no‐slip boundary conditions, the mean inner core rotation rate is almost an order of magnitude greater.
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
    detail.hit.zdb_id: 2021599-X
    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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