Full-orbit simulations in a turbulent Parker spiral show drift reduction factors of 0.2-0.9, much larger (less suppression) than predicted by standard drift-suppression theories at low proton energies.
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Interplay of large-scale drift and turbulence in the heliospheric propagation of solar energetic particles
Full-orbit simulations in a turbulent Parker spiral show drift reduction factors of 0.2-0.9, much larger (less suppression) than predicted by standard drift-suppression theories at low proton energies.