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Acceleration Mechanisms of Solar Energetic Particles

Solar Flares and CMEs → Observational Signatures of Acceleration

This advanced graduate-level learning path systematically covers the physics of solar energetic particle (SEP) acceleration, focusing on flare and shock acceleration mechanisms, particle transport, and their observational context. It builds from foundational plasma physics and particle dynamics to specialized topics such as diffusive shock acceleration and shock-drift acceleration, culminating in a comprehensive understanding of SEP events.

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12 steps · 12 nodes · 3 stages

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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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