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- W2023227136 abstract "We present the results of numerical simulations of solar energetic particles (SEPs) moving in a model heliospheric magnetic field. We find that the onset time of a given SEP event can be sooner than estimated by assuming that particles move along the usual Parker spiral, which is generally believed to be the earliest time. This is because for a random magnetic field, some magnetic field lines are shorter than the nominal (Parker spiral) length. This is important with regard to the physics of injection and/or acceleration at the origin of the particle event." @default.
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- W2023227136 date "2006-04-20" @default.
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- W2023227136 title "Effect of a Random Magnetic Field on the Onset Times of Solar Particle Events" @default.
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- W2023227136 doi "https://doi.org/10.1086/427161" @default.
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