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Maxwell's Equations and Lorentz Force → Magnetic Fields in Galaxy Clusters
This graduate-level path explores the origin and role of magnetic fields across cosmic scales, from the interstellar medium to galaxy clusters. It builds from foundational electrodynamics and MHD through turbulence and dynamo theory to observational probes like the Zeeman effect and Faraday rotation.
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13 steps · 3 stages. Click any step to inspect it and see it on the Path Map.
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