Solar and Heliospheric Observatory

Related lectures (12)

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.

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

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

Delves into the formation and observation of auroras, highlighting the distinctions between the northern and southern lights.

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

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

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

Explores the vulnerability of microelectronics to space radiations and mitigation techniques.

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

Explores the analysis of solar potential at EPFL using Grasshopper and Rhinoceros.

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