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A new numerical scheme in the solution of the geodynamo Z-model
[chapter]
1993
The Cosmic Dynamo
The hydromagnetic dynamo Z-model represents a nonlinear dynamic system. Its steady-state solution is derived by step-by-step integration of parabolic partial differential equations of the second order with the use of the finite difference method. Until now, two methods have been used: the semi-implicit method in which the θ-diffusion was carried out implicitly while the r-diffusion explicitly, and the implicit method in which the complete diffusion was carried out implicitly. In the present
doi:10.1007/978-94-011-0772-3_82
fatcat:nqlkqmdvfbaptlef7gkzonjsui