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Understanding the Structure of the Interplanetary Magnetic Field

Solar Wind Basics → Alfvénic Fluctuations

This learning path guides undergraduate space physics students through the essential concepts needed to understand the large-scale structure of the interplanetary magnetic field (IMF). Starting with solar wind basics and magnetohydrodynamics, it progresses through the Parker spiral, sector structure, and various IMF variations, including magnetic clouds and Alfvénic fluctuations. The path emphasizes the physical mechanisms and observational evidence that define the IMF's structure.

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8 steps · 8 nodes · 2 stages

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Path Steps

8 steps · 2 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

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