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Solar Energetic Particles: Acceleration, Transport, and Space Weather Effects

Solar Atmosphere and Solar Wind → Observations of SEPs

A comprehensive graduate-level learning path covering the physics of solar energetic particles (SEPs), from their acceleration at the Sun to their propagation through the heliosphere and their impacts on Earth. The path systematically builds from fundamental plasma and particle physics to advanced topics in SEP acceleration mechanisms, transport theory, and space weather applications.

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14 steps · 14 nodes · 3 stages

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14 nodes33 edges3 relationships

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Path Steps

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

Stage 1

Foundation

5 steps

Stage 2

Core Concepts

5 steps

Stage 3

Advanced Topics

4 steps

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