The Two-Layer Geodynamo Model

Аннотация

A 2-D mean field geodynamo model with the algebraic form of nonlinearity is considered. The geostrophic alpha-effect and differential rotation are taken from the 3-D models of convection in the liquid core of the Earth. The analysis reveals that these both are located in different spatial areas, and their correlation is no more than ten percent. The model allows typical Z-distributions of the poloidal magnetic field to be generated within the Taylor cylinder. On the surface, this field configuration corresponds to the magnetic dipole. Because of the spatial homogeneity of the magnetic field in the cylinder, dissipation of the field is small, which causes its greater amplitude in this region. Owing to the simple form of alpha-effect quenching by the magnetic field, the model can be used to generate a magnetic field over geological times.