Numerical tracing of stochastic Parker spirals yields an angular field line spread of ~25° at 1 AU that narrows to ~4° when integrated backward to the solar source surface at 0.25 AU.
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2 Pith papers cite this work. Polarity classification is still indexing.
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A review of ML models for SEP prediction that compares architectures, datasets, inputs and outputs while recommending good practices for future work.
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Turbulent Diffusion of Magnetic Field Lines in the Heliosphere
Numerical tracing of stochastic Parker spirals yields an angular field line spread of ~25° at 1 AU that narrows to ~4° when integrated backward to the solar source surface at 0.25 AU.
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Review of Machine Learning Models for Solar Energetic Particle Prediction
A review of ML models for SEP prediction that compares architectures, datasets, inputs and outputs while recommending good practices for future work.