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The rapid rotation of planets causes cyclonic thermal turbulence in their cores which may generate the large-scale magnetic fields observed outside the planets. We investigate numerically a model base...
High-Order Compact Implicit Difference Methods For Parabolic Equations in Geodynamo Simulation
Parabolic Equations Geodynamo Simulation magnetohydrodynamic
2009/9/4
A series of compact implicit schemes of fourth and sixth orders are developed for solving differential equations involved in geodynamics simulations. Three illustrative examples are described to demon...