Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic (∼∼ few
GeV) energies are accelerated near the Sun in at least two ways:(1) by magnetic …

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …

We present a new analysis of the transport of cosmic rays in a turbulent magnetic field that
varies in all three spatial dimensions. The analysis utilizes a numerical simulation that …

The interaction of the solar wind with the local interstellar medium (LISM) is attracting
renewed interest, thanks to the possibility that the Voyager spacecraft may, in the not too …

If charged particles move through the interplanetary or interstellar medium, they interact with
a large-scale magnetic field such as the magnetic field of the Sun or the Galactic magnetic …

While observations have suggested that power-law electron energy spectra are a common
outcome of strong energy release during magnetic reconnection, eg, in solar flares, kinetic …

Energization at a quasi‐perpendicular shock is described for ions which approach the shock
with a speed much less than that of the incoming plasma. These ions may be trapped …

Scientists have explored how energetic particles such as solar energetic particles and
cosmic rays move through a magnetized plasma such as the interplanetary and interstellar …

Transport of charged particles across the mean magnetic field due to broad band, powerlaw‐
distributed magnetic fluctuations is examined by direct computation of a large number of …

The computation of charged particle orbits in model turbulent magnetic fields is used to
investigate the properties of particle transport in the directions perpendicular to the large …