Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles

Modeling of time profiles of solar energetic particle (SEP) observations often considers transport along a large-scale magnetic field with a fixed path length from the source to the observer. Here, we point out that variability in the turbulent field line path length can affect the fits to SEP data...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Wirin Sonsrettee, Piyanate Chuychai, Achara Seripienlert, Paisan Tooprakai, Alejandro Sáiz, David Ruffolo, William H. Matthaeus, Rohit Chhiber
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Solar energetic particles Interplanetary magnetic fields Interplanetary turbulence Solar-terrestrial interactions
Online Access:	https://doi.org/10.3847/1538-4357/ad3d58