Explore the fascinating world of planetary dynamos in this comprehensive lecture. Delve into the mechanisms behind planetary magnetospheres and auroras, indicators of magnetic dipole fields. Examine the internal dynamo processes occurring in liquid cores that generate main planetary magnetic fields. Study planetary data and learn about key geodynamo researchers. Investigate the Earth's interior structure, including its inner core, and analyze the geological record of geomagnetic excursions. Understand the basic equations and mathematical models based on magnetohydrodynamic (MHD) equations with buoyancy. Discover numerical modeling techniques for solving nonlinear partial differential equations, including spectral methods for regular geometries. Explore geodynamo parameters, magnetic fields, and turbulent relaxation of ideal magneto-fluid. Learn about spherical harmonics, function expansions for spherical shells, and the transformation of PDEs into coupled ODEs. Examine the statistics of ideal MHD turbulence, probability density functions, and invariants. Investigate cross helicity and its relationship to the expected dipole angle. Gain insights into large-scale numerical simulations of ideal, rotating MHD turbulence in spherical shells and their implications for effective cross helicity. Read more