Issue No. 03 - May/June (2000 vol. 2)
DOI Bookmark: http://doi.ieeecomputersociety.org/10.1109/5992.841797
A computer simulation of magnetic field generation by convection in the Earth's fluid outer core produces a time dependent field that, like the Earth's, is strongly dipole dominated outside the core and occasionally undergoes spontaneous dipole reversals. The computational challenge posed by this rapidly-rotating low-viscosity magnetohydrodynamic problem and the numerical method used are discussed.
T. Clune and G. A. Glatzmaier, "Computational Aspects of Geodynamo Simulations," in Computing in Science & Engineering, vol. 2, no. , pp. 61-67, 2000.