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Concept

Magnetic reconnection

Related lectures (32)

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

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

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

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

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

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

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

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

Explores solar magnetic fields, dynamo theory, turbulence effects, and solar cycle dynamics.

Explores MHD equilibrium and stability, emphasizing energy considerations for determining stability.

Covers exercises on plasma physics, focusing on the sun's power and magnetic flux tubes.

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

Covers ideal MHD waves, including the shear Alfvén wave and compressional waves with a longitudinal component.

Covers the concept of Ideal MHD waves and the behavior of plasma under different conditions.

Covers the behavior of electromagnetic waves in non-magnetized plasmas and the simplification of equations for non-collisional plasmas.

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