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 …

In this review, an overview of the recent history of stochastic differential equations (SDEs) in
application to particle transport problems in space physics and astrophysics is given. The …

ABSTRACT Since 2012 August Voyager 1 has been observing the local interstellar energy
spectra of Galactic cosmic-ray nuclei down to 3 MeV nuc− 1 and electrons down to 2.7 MeV …

During the recent prolonged solar minimum of cycle 23/24, the PAMELA detector measured
27-day averaged Galactic proton energy spectra over the energy range that is important for …

We review recent observations and modeling developments on the subject of galactic
cosmic rays through the heliosphere and in the Very Local Interstellar Medium, emphasizing …

The heliosphere is formed due to interaction between the solar wind (SW) and local
interstellar medium (LISM). The shape and position of the heliospheric boundary, the …

This paper summarizes the results obtained by the team “Heliosheath Processes and the
Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic …

In recent years, the increasing precision of direct cosmic rays measurements opened the
door to high-sensitivity indirect searches of dark matter and to more accurate predictions for …

Heliospheric modulation conditions were unusually quiet during the last solar minimum
activity between solar cycles 23 and 24. Fortunately, the PAMELA space experiment …

The radial and rigidity dependence of the cosmic ray (CR) diffusion tensor is investigated on
the basis of a recently developed 2D and slab turbulence transport model using nearly …