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Magnetohydrodynamics for Astrophysical Applications

Vector Calculus for MHD → MHD Applications in Astrophysics

This path equips graduate astrophysics students with the theoretical and mathematical foundations of magnetohydrodynamics (MHD) and its application to key astrophysical phenomena. Starting from vector calculus and electrodynamics, it progresses through the MHD equations, wave modes, and advanced concepts like reconnection and dynamos, culminating in the analysis of jets and outflows.

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12 steps · 12 nodes · 3 stages

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Path Steps

12 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

4 steps

Stage 2

Core Concepts

4 steps

Stage 3

Advanced Topics

4 steps

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