Lecture

Astrophysics: Solar Magnetic Fields and Dynamo Theory

Related lectures (32)

Explores MHD dynamo theory, covering magnetic field generation by conductive fluid and the Babcock-Leighton mechanism.

Explores magnetohydrodynamics, emphasizing the two-fluid model, Alfvén's theorem, solar wind, dynamos, and magnetic reconnection.

Covers magnetohydrodynamics, focusing on modeling challenges and MHD equations in plasma physics.

Explores sunspots, the solar cycle, and magnetic fields on the Sun, including the 11-year cycle and the Hale's and Joy's laws.

Covers magnetic reconnection, rising flux tubes, the Sweet-Parker model, energy balance, and open questions in plasma physics.

Explores the solar cycle, sunspots, and magnetic fields in the Sun, including properties, dynamics, and historical observations.

Explores magnetic reconnection in astrophysics, focusing on solar flares and the solar wind.

Explores the Sun's magnetic-driven features like flares and coronal mass ejections.

Explores space mission design, Earth's magnetic field, solar activity, and cosmic radiation effects.

Delves into the dynamics of the solar wind, including observations, fluid models, and the Sun's mass loss rate.

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.