Description
The complete IceCube Observatory has collected over 690 billion cosmic-ray induced muon events from May 2011 to May 2022. These unprecedented statistics make it possible to observe significant structure in in the distribution of cosmic-ray arrival directions at both higher cosmic-ray energies and smaller angular scales. Combined with improved simulation and systematics, we can provide a newly detailed assessment of the energy- and time-dependence of the cosmic-ray anisotropy in the Southern Hemisphere. We present the preliminary results from a study with the extended event
sample.
Auteurs principaux
Prof.
Frank McNally
(Mercer University)
Dr
Juan Carlos Díaz Vélez
(University of Wisconsin–Madison)
Dr
Paolo Desiati
(WIPAC - University of Wisconsin-Madison)
Prof.
Rasha Abbasi
(Loyola University Chicago)
