--- abstract: 'Propagation of energetic particles across the mean field direction in turbulent magnetic fields is often described as spatial diffusion. Recently, it has been suggested that initially the particles propagate systematically along meandering field lines, and only later reach the time-asymptotic diffusive cross-field propagation. In this paper, we analyse cross-field propagation of 1-100 MeV protons in composite 2D-slab turbulence superposed on a constant background magnetic field, using full-orbit particle simulations, to study the non-diffusive phase of particle propagation with a wide range of turbulence parameters. We show that the early-time non-diffusive propagation of the particles is consistent with particle propagation along turbulently meandering field lines. This results in a wide cross-field extent of the particles already at the initial arrival of particles to a given distance along the mean field direction, unlike when using spatial diffusion particle transport models. The cross-field extent of the particle distribution remains constant for up to tens of hours in turbulence environment consistent with the inner heliosphere during solar energetic particle events. Subsequently, the particles escape from their initial meandering field lines, and the particle propagation across the mean field reaches time- asymptotic diffusion. Our analysis shows that in order to understand solar energetic particle event origins, particle transport modelling must include non-diffusive particle propagation along meandering field lines.' adsnote: Provided by the SAO/NASA Astrophysics Data System adsurl: https://ui.adsabs.harvard.edu/abs/2017MNRAS.470.3149L archivePrefix: arXiv authors: - T. Laitinen - S. Dalla - D. Marriott category: publications date: '2017-09-01' doi: 10.1093/mnras/stx1509 draft: false eprint: '1706.06580' featured: false journal: MNRAS month: September number: '3' pages: 3149-3158 primaryClass: physics.space-ph projects: [] publication: MNRAS publication_types: - '2' tags: - Diffusion - Magnetic fields - Turbulence - 'Sun: particle emission' - Physics - space physics - Astrophysics - solar and stellar astrophysics title: 'Early propagation of energetic particles across the mean field in turbulent plasmas' type: ARTICLE volume: '470' year: '2017' ---