Constraining the charge-, time-, and rigidity-dependence of cosmic-ray solar modulation with AMS-02 observations during Solar Cycle 24
Author:
Funder
National Aeronautics and Space Administration
U.S. Department of Energy
Office of Science
High Energy Physics
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.106.063021/fulltext
Reference63 articles.
1. Solar modulation parameter for cosmic rays since 1936 reconstructed from ground-based neutron monitors and ionization chambers
2. Cosmic-ray yield and response functions in the atmosphere
3. Numerical Modeling of Galactic Cosmic-Ray Proton and Helium Observed by AMS-02 during the Solar Maximum of Solar Cycle 24
4. Test of validity of the Force-Field Approximation with AMS-02 and PAMELA Monthly Fluxes
5. Spectral Properties of the N Component of the Heliospheric Magnetic Field from IMP and ACE Observations for 1973–2020
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