The problem of small angular scale structure in the cosmic ray anisotropy data

Abstract

Recent observations have revealed structure on small angular scales in the anisotropy data of cosmic rays at multi TeV energies. Even though the absolute amplitudes are very small, these effects are somewhat surprising and a wide range of possible causes have been discussed. A possible origin associated with heliospheric electric fields is proposed.

To be presented at the International Cosmic Ray Conference ICRC32013 in Rio

References in corpus (1)

• Strangelets and the TeV-PeV cosmic-ray anisotropies

Cited by in corpus (6)

• Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
• Measurements and implications of cosmic ray anisotropies from TeV to trans-EeV energies
• Time variability of TeV cosmic ray sky map
• Snowmass 2021 LoI: Determination of cosmic ray properties in the local interstellar medium with all-sky anisotropy observations
• Cosmic ray propagation in the interstellar magnetic fields
• A search for small and medium scale anisotropy of cosmic rays above 1 PeV registered at the Tunka-133 array