Astrophysical Dynamo in a Stellar Interior

Domain: Model a portion of the interior of a star.

Boundary Conditions:

• Insulated boundaries.

Initial Conditions:

• Seed magnetic field and temperature distribution.

Dynamo Term:

• Consider the combined effects of convection and rotation.

These test cases provide a starting point for simulating MHD Dynamo Theory. Actual applications may involve more complex geometries, additional physical effects, and tailored boundary conditions based on specific scenarios. Dynamo theory often involves studying the evolution of magnetic fields over time and understanding the mechanisms that amplify and sustain magnetic fields in astrophysical and laboratory plasmas.