Magnetohydrodynamics: Two-Fluid Model

Related lectures (32)

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

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

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

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

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

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

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

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

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

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