Dynamic simulation of the hydromagnetic dynamo behavior in a rotating spherical layer under various initial conditions

We simulated the effects of initial conditions on the properties and structure of the hydromagnetic dynamo a rotating spherical layer. We developed an MHD code for the computational experiments adapted for hybrid computing systems with GPUs. We obtained quasi-stationary solutions with the stable energy of the generated magnetic field. The impact of the Rayleigh number on the solutions is also studied.