Auroras: Northern and Southern Lights

Related lectures (20)

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

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

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

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

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

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

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

Explores the geomagnetic field distortions due to the solar wind and the Aurora phenomenon.

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.