# Propagation of Cosmic Rays in Heliosphere: the HelMod Model

## TL;DR

The exttt{HelMod} model simulates cosmic ray propagation in the heliosphere, incorporating drift effects and matching observational data from multiple space missions during solar cycles 23 and 24.

## Contribution

This paper presents the current version 3 of the exttt{HelMod} model, including detailed implementation of drift effects and validation against experimental data.

## Key findings

- exttt{HelMod} reproduces measured cosmic ray spectra within experimental errors.
- Model results agree with Ulysses measurements at high solar latitudes.
- The model accurately simulates cosmic ray modulation during solar cycles 23 and 24.

## Abstract

The heliospheric modulation model \helmod{} is a two dimensional treatment dealing with the helio-colatitude and radial distance from Sun and is employed to solve the transport-equation for the GCR propagation through the heliosphere down to Earth. This work presents the current version 3 of the \helmod{} model and reviews how main processes involved in GCR propagation were implemented.~The treatment includes the so-called particle drift effects --~e.g., those resulting, for instance, from the extension of the neutral current sheet inside the heliosphere and from the curvature and gradient of the IMF --, which affect the transport of particles entering the solar cavity as a function of their charge sign.~The \helmod{} model is capable to provide modulated spectra which well agree within the experimental errors with those measured by AMS-01, BESS, PAMELA and AMS-02 during the solar cycles 23 and 24.~Furthermore, the counting rate measured by Ulysses at +/- 80degree of solar latitude and 1 to 5\,AU was also found in agreement with that expected by \helmod{} code version 3.