New solar modulation modeling of the galactic proton flux measured by the AMS02 and PAMELA experiments
1 Dipartimento di Fisica e Geologia, University of Perugia and INFN Perugia, Italy
2 INFN Perugia, Italy and ASI Space Science Data Center (SSDC), Roma, Italy
a e-mail: email@example.com
Published online: 13 May 2019
A thorough understanding of solar effects on the galactic cosmic rays is relevant both to infer the local interstellar spectrum characteristics and to investigate the dynamics of charged particles in the heliosphere. We present a newly developed numerical modulation model to study the transport of galactic protons in the heliosphere. The model was applied to the 27-day averaged galactic proton flux recently released by the PAMELA and AMS02 experiments, covering an extended time period from mid-2006 to mid-2017.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.