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Physics of Solar Flares

Sunspots and Active Regions → Synthesis: Standard Flare Model

A comprehensive learning path for undergraduate solar physics students to understand solar flares, from plasma and MHD foundations through magnetic reconnection, particle acceleration, and emission mechanisms, culminating in flare classification and a synthesis of the standard flare model.

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9 steps · 9 nodes · 3 stages

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Path Steps

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

Stage 1

Foundation

3 steps

Stage 2

Core Concepts

3 steps

Stage 3

Advanced Topics

3 steps

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