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Št. zadetkov: 3
Measuring large-scale anisotropy in the arrival directions of cosmic rays detected at the Telescope Array and the Pierre Auger Observatory above 10[sup]19 eV
O. Deligny, Andrej Filipčič, Thomas Paul, Samo Stanič, Darko Veberič, Danilo Zavrtanik, Marko Zavrtanik
Objavljeni znanstveni prispevek na konferenci
Oznake: Observatorij Pierre Auger;kozmični žarki;anizotropija;
Measuring large-scale anisotropy in the arrival directions of cosmic rays detected at the Telescope Array and the Pierre Auger Observatory above 10[sup]19 eV
Leto: 2013 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Large-scale distribution of arrival directions of cosmic rays detected at the Pierre Auger Observatory and the Telescope Array above 10[sup]19 eV
O. Deligny, Andrej Filipčič, Gašper Kukec Mezek, A. Saleh, Samo Stanič, M. Trini, Darko Veberič, Serguei Vorobiov, Lili Yang, Danilo Zavrtanik, Marko Zavrtanik
Objavljeni znanstveni prispevek na konferenci
Oznake: Telescope Array;high-energy cosmic rays;large-scale anisotropies;angular power spectrum;Pierre Auger Observatory;
The large-scale distribution of arrival directions of high-energy cosmic rays is a key observable in attempts to understanding their origin. The dipole and quadrupole moments are of special interest in revealing potential anisotropies. An unambiguous measurement of these moments as well as ...
Leto: 2015 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
ǂThe ǂenergy spectrum of ultra-high energy cosmic rays measured at the Pierre Auger Observatory and at the Telescope Array
Olivier Deligny, Andrej Filipčič, Gašper Kukec Mezek, Samo Stanič, M. Trini, Serguei Vorobiov, Lili Yang, Danilo Zavrtanik, Marko Zavrtanik, Lukas Zehrer
Objavljeni znanstveni prispevek na konferenci
Oznake: Pierre Auger Observatory;ultra-high energy cosmic rays;UHECR energy spectrum;Telescope Array;
The energy spectrum of ultra-high energy cosmic rays measured at the Pierre Auger Observatory and at the Telescope Array
Leto: 2019 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Št. zadetkov: 3
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