Drift-induced perpendicular transport of Solar Energetic Particles

TL;DR

This paper demonstrates that particle drifts significantly influence the perpendicular transport of Solar Energetic Particles, challenging the current assumption that drifts are negligible in SEP propagation models.

Contribution

It introduces full-orbit simulations showing that SEP drifts cause notable perpendicular propagation, emphasizing the need to incorporate drift effects into SEP models.

Findings

High-energy SEPs experience significant perpendicular displacement due to drifts.

Drift effects are more pronounced for heavy ion SEPs with larger mass-to-charge ratios.

SEP drifts can transport particles across the magnetic field over distances of about 1 AU within typical event timescales.

Abstract

Drifts are known to play a role in galactic cosmic ray transport within the heliosphere and are a standard component of cosmic ray propagation models. However, the current paradigm of Solar Energetic Particle (SEP) propagation holds the effects of drifts to be negligible, and they are not accounted for in most current SEP modelling efforts. We present full-orbit test particle simulations of SEP propagation in a Parker spiral interplanetary magnetic field which demonstrate that high energy particle drifts cause significant asymmetric propagation perpendicular to the interplanetary magnetic field. Thus in many cases the assumption of field aligned propagation of SEPs may not be valid. We show that SEP drifts have dependencies on energy, heliographic latitude, and charge to mass ratio, that are capable of transporting energetic particles perpendicular to the field over significant distances within interplanetary space, e.g. protons of initial energy 100 MeV propagate distances across the field on the order of 1 AU, over timescales typical of a gradual SEP event. Our results demonstrate the need for current models of SEP events to include the effects of particle drift. We show that the drift is considerably stronger for heavy ion SEPs due to their larger mass to charge ratio. This paradigm shift has important consequences for the modelling of SEP events and is crucial to the understanding and interpretation of in-situ observations.