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Classical Electrodynamics → Astrophysical Applications
This graduate-level path equips learners with the theoretical tools to describe plasma behavior in astrophysical environments, starting from electrodynamics and fluid mechanics, progressing through single-particle motion and MHD, and culminating in advanced topics like magnetic reconnection, dynamo theory, and collisionless shocks. Emphasis is on the physical principles and their application to stars, accretion disks, and the interstellar medium.
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11 steps · 3 stages. Click any step to inspect it and see it on the Path Map.
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