Cosmic-ray anisotropy: sensitivity of methods and implications for KASCADE data

arXiv:2607.11405 · astro-ph.HE · Submitted 2026-07-13 · Read on arXiv

M. Yu. Kuznetsov, N. A. Petrov, E. M. Shinkevich

astro-ph.HE

Submitted: 2026-07-13

Comments: 22 pages, 17 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Anisotropy — 94× in this paper · explained in 3 episodes
• Diffusion Model — 3× in this paper · explained in 8 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes

Sources

• Cosmic Ray Models
• Origin of Small-Scale Anisotropies in Galactic Cosmic Rays
• Evolution of the cosmic ray anisotropy above 10^{14} eV
• Northern sky Galactic Cosmic Ray anisotropy between 10-1000 TeV with the Tibet Air Shower Array
• Galactic Cosmic-Ray Anisotropy in the Northern hemisphere from the ARGO-YBJ Experiment during 2008-2012
• Observation of Cosmic Ray Anisotropy with the IceTop Air Shower Array
• Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector
• Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino Observatory
• Large- and Medium-Scale Anisotropies in the Arrival Directions of Cosmic Rays observed with KASCADE-Grande
• New insights from old cosmic rays: A novel analysis of archival KASCADE data
• Methods of machine learning for the analysis of cosmic rays mass composition with the KASCADE experiment data
• Energy spectra of elemental groups of cosmic rays with the KASCADE experiment data and machine learning
• The East-West method: an exposure-independent method to search for large scale anisotropies of cosmic rays
• Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

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