Recent data from the Pierre Auger Observatory has revealed the presence of a large-scale
dipole in the arrival direction distribution of ultrahigh-energy cosmic rays (UHECR). In this …

We study the spectrum and anisotropies of ultrahigh energy cosmic ray transient sources,
accounting for the effects of their propagation through the turbulent extragalactic magnetic …

We study the anisotropies on large angular scales which can be present in the flux of cosmic
rays reaching the Earth from a population of extragalactic sources, focusing on the energy …

The telescope Mini-EUSO has been observing, since 2019, the Earth in the ultraviolet band
(290–430 nm) through a nadir-facing UV-transparent window in the Russian Zvezda module …

Ultra-high-energy cosmic rays (UHECRs), accelerated hadrons that can exceed energies of
10 20 eV, are the highest-energy particles ever observed. While the sources producing …

The extremely low flux of ultra-high energy cosmic rays (UHECR) makes their direct
observation by orbital experiments practically impossible. For this reason all current and …

Abstract The Pierre Auger Observatory has been detecting ultra-high energy cosmic rays
(UHECRs) for more than fifteen years. An essential feature of the Observatory is its hybrid …

We present a solution to Liouville's equation for an ensemble of charged particles
propagating in magnetic fields. The solution is presented using an expansion in spherical …

Recent anisotropy studies of UHECR data at energies≳ 40 EeV have disclosed a correlation
of their angular distribution with the extragalactic local structure, specifically with either local …

Photodisintegration is a main energy loss process for ultrahigh-energy cosmic-ray (UHECR)
nuclei in intergalactic space. Therefore, it is crucial to understand systematic uncertainty in …