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Numerical MHD Simulations of Solar Phenomena

Magnetohydrodynamics (MHD) Theory → Simulation of Solar Flares and CMEs

This learning path guides graduate students in solar physics from foundational MHD theory and numerical methods to hands-on simulation of solar flares and CMEs. It emphasizes practical skills in high-performance computing and data analysis, culminating in the ability to design, run, and validate MHD simulations of solar phenomena.

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12 steps · 12 nodes · 3 stages

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12 nodes17 edges3 relationships

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Path Steps

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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