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Solar Wind Driving of Magnetospheric Dynamics

Solar Wind Basics → Magnetospheric Convection

This learning path guides undergraduate space physics students from solar wind fundamentals through the Dungey cycle to understand how solar wind drives magnetospheric dynamics. It covers magnetic reconnection, polar cap potential, and dayside/nightside coupling, building a systematic understanding of solar wind-magnetosphere interaction.

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10 steps · 10 nodes · 3 stages

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Path Steps

10 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

3 steps

Stage 3

Advanced Topics

3 steps

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