11th GRC International Frontier Seminar



"The thermal and magnetic evolution of the core"

Prof. S. Labrosse (IPGP, France)


3 March 2005 13:30-16:00
Meeting room, 6th floor, Advanced Research Building, Ehime University

 



 The magnetic field of the Earth is generated by convection in the liquid core and energy necessary for this process comes from the cooling of the core which provide several buoyancy sources. The Energy balance shows that the heat flow at the CMB is equilibrated by the sum of four energy sources: secular cooling, latent heat offreezing at the ICB,compositional energy due to the redistribution of light elements upon freezing and, perhaps, radiogenic heating. The entropy balance can be used to show that the compositional energy is most effectively transformed into ohmic dissipation. All these energy sources, save the radioactivity, are a function of the radius of the inner core and are proportional to its growth rate. This growth rate can be computed for any given ohmic dissipation in the core, and this allows the computation of the heat flow across the CMB. Alternatively, if the heat flow at the CMB is known, the growth rate of the inner core can be computed, giving the ohmic dissipation in the core. Unfortunately, neither the ohmic dissipation nor the heat flow at the CMB is known with precision. Additional uncertainties come from the imperfectly density difference of chemical origin between the inner and outer cores. Nevertheless, exploration of a reasonable parameter space, show that the inner core likely no older than 2 Ga, and that the magnetic field prior to that time was sustained by thermal convection alone.





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主催:愛媛大学地球深部ダイナミクス研究センター


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