An empirical modification of the force field approach to describe the modulation of galactic cosmic rays close to Earth in a broad range of rigidities
Jan Gieseler, Bernd Heber, Konstantin Herbst

TL;DR
This paper introduces a modified force field approach to better model galactic cosmic ray modulation near Earth across a broad energy range, addressing limitations of the traditional method by incorporating energy and solar epoch dependencies.
Contribution
It presents a new tool that improves the description of GCR proton spectra from hundreds of MeV to tens of GeV over multiple solar cycles, accounting for energy and epoch effects.
Findings
Severe limitations of the traditional force field approach at low energies.
Strong dependence of GCR modulation on solar magnetic epoch.
Enhanced modeling of cosmogenic radionuclide production rates.
Abstract
On their way through the heliosphere, Galactic Cosmic Rays (GCRs) are modulated by various effects before they can be detected at Earth. This process can be described by the Parker equation, which calculates the phase space distribution of GCRs depending on the main modulation processes: convection, drifts, diffusion and adiabatic energy changes. A first order approximation of this equation is the force field approach, reducing it to a one-parameter dependency, the solar modulation potential . Utilizing this approach, it is possible to reconstruct from ground based and spacecraft measurements. However, it has been shown previously that depends not only on the Local Interstellar Spectrum (LIS) but also on the energy range of interest. We have investigated this energy dependence further, using published proton intensity spectra obtained by PAMELA as well as heavier…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Astronomy and Astrophysical Research · Solar and Space Plasma Dynamics
