A three-component cosmic-ray model that includes the local interstellar cloud's motion and magnetic field reproduces the energy-dependent dipole anisotropy of cosmic rays from GeV to PeV energies, but with many fitted parameters.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Influence of interstellar environment near the solar system on cosmic-ray spectra and dipole anisotropy
A three-component cosmic-ray model that includes the local interstellar cloud's motion and magnetic field reproduces the energy-dependent dipole anisotropy of cosmic rays from GeV to PeV energies, but with many fitted parameters.