Lectures related to Astrophysics: Solar Magnetic Fields and Dynamo Theory

Covers the physics of plasmas, emphasizing magnetohydrodynamics and energy conversion processes.

Explores observational facts and the need for dynamos in generating magnetic fields.

Explores MHD waves, instabilities, magnetoconvection, and the impact of B-fields on convection.

Explores how fusion energy powers the Sun and drives powerful solar events.

Explores Magnetohydrodynamic equilibrium and stability, ideal MHD solutions, 'hairy ball' theorem, and boundary conditions.

Covers the Magnetohydrodynamic (MHD) description of plasma, including MHD equations, conservation properties, and ideal vs. resistive models.