Charge-sign dependent solar modulation for everyone

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.

Contribution to the TAUP 2015 conference proceedings. 5 pages, 4 figures

References in corpus (4)

• Measurements of 0.2 to 20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer
• Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight
• AMS-02 Antiprotons Reloaded
• The Cosmic Ray Antiproton Background for AMS-02

Cited by in corpus (1)

• Time-dependent AMS-02 electron-positron fluxes in an extended force-field model