Lecture

MHD Turbulence and Dynamo Instabilities

In course

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Description

This lecture covers the observational facts related to MHD dynamos, including planets, stars, interstellar galaxies, and galaxy clusters. It also discusses Zeemann splitting, blazar observations, and the solar cycle. The lecture delves into the need for dynamos, the presence of extremely weak seed magnetic fields, and the generation of magnetic fields in the Universe.

Official source

https://mediaspace.epfl.ch/media/0_wo6x825h

About this result

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Ontological neighbourhood

Astronomy

Astrophysics: Stellar astronomy, Physical cosmology

Physics

Plasma physics: Space-plasma physics

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