A 1D spherically symmetric Parker transport model with charge-sign and rigidity-dependent parameters fitted via solar-proxy cross-correlation is validated on PAMELA, AMS-02, and ACE data for long-term GCR forecasting.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
Time-dependent MHD models of the corona-heliosphere system produce magnetic connectivities consistent with observed strahl occurrence rates, unlike steady-state models.
citing papers explorer
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A new model for long-term forecasting of Galactic cosmic rays
A 1D spherically symmetric Parker transport model with charge-sign and rigidity-dependent parameters fitted via solar-proxy cross-correlation is validated on PAMELA, AMS-02, and ACE data for long-term GCR forecasting.
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Magnetic Connectivity in the Time-Dependent Corona and Heliosphere
Time-dependent MHD models of the corona-heliosphere system produce magnetic connectivities consistent with observed strahl occurrence rates, unlike steady-state models.