Charge-sign dependent solar modulation for everyone

TL;DR

This paper introduces a publicly available tool that models charge-sign dependent solar modulation of cosmic rays, providing a more detailed alternative to the traditional force-field approximation, with applications to recent proton and antiproton data.

Contribution

The paper presents a new computational tool that improves modeling of charge-sign dependent solar modulation for cosmic rays, surpassing the traditional force-field approach.

Findings

The tool effectively models proton and antiproton fluxes.

It offers improved accuracy over existing models.

Applications demonstrate consistency with recent experimental data.

Abstract

We present a tool to compute the influence of charge-sign dependent solar modulation for cosmic ray spectra. The code is publicly available, easy to use and offers an extended view on solar modulation compared to the force-field approximation. We present some examples for proton and antiproton fluxes in the light of recent experimental data.