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Naslov:Study of Ultra-High Energy Cosmic Ray composition using Telescope Array’s Middle Drum detector and surface array in hybrid mode
Avtorji:ID Abbasi, R.U. (Avtor)
ID Lundquist, Jon Paul, UNG (Avtor), et al.
Datoteke: Gradivo nima datotek, ki so prostodostopne za javnost. Gradivo je morda fizično dosegljivo v knjižnici fakultete, zalogo lahko preverite v COBISS-u. Povezava se odpre v novem oknu
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:UNG - Univerza v Novi Gorici
Opis:Previous measurements of the composition of Ultra-High Energy Cosmic Rays (UHECRs) made by the High Resolution Fly’s Eye (HiRes) and Pierre Auger Observatory (PAO) are seemingly contradictory, but utilize different detection methods, as HiRes was a stereo detector and PAO is a hybrid detector. The five year Telescope Array (TA) Middle Drum hybrid composition measurement is similar in some, but not all, respects in methodology to PAO, and good agreement is evident between data and a light, largely protonic, composition when comparing the measurements to predictions obtained with the QGSJetII-03 and QGSJet-01c models. These models are also in agreement with previous HiRes stereo measurements, confirming the equivalence of the stereo and hybrid methods. The data is incompatible with a pure iron composition, for all models examined, over the available range of energies. The elongation rate and mean values of are in good agreement with Pierre Auger Observatory data. This analysis is presented using two methods: data cuts using simple geometrical variables and a new pattern recognition technique.
Ključne besede:Ultra-High Energy Cosmic Rays, Cosmic ray composition, Atmospheric fluorescence, Extensive air shower array, Hybrid, Telescope Array
Verzija publikacije:Recenzirani rokopis
Leto izida:2015
Št. strani:23
Številčenje:64, 64
PID:20.500.12556/RUNG-5145-5d15f908-23c3-8579-e6c5-2fa2160df902 Novo okno
COBISS.SI-ID:5616635 Novo okno
DOI:https://doi.org/10.1016/j.astropartphys.2014.11.004 Novo okno
NUK URN:URN:SI:UNG:REP:2UN9PIMZ
Datum objave v RUNG:24.04.2020
Število ogledov:4275
Število prenosov:0
Metapodatki:XML DC-XML DC-RDF
:
ABBASI, R.U. in LUNDQUIST, Jon Paul, 2015, Study of Ultra-High Energy Cosmic Ray composition using Telescope Array’s Middle Drum detector and surface array in hybrid mode. Astroparticle Physics [na spletu]. 2015. Vol. 64, no. 64. [Dostopano 10 april 2025]. DOI https://doi.org/10.1016/j.astropartphys.2014.11.004. Pridobljeno s: https://repozitorij.ung.si/IzpisGradiva.php?lang=slv&id=5145
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Gradivo je del revije

Naslov:Astroparticle Physics
Skrajšan naslov:Astro. Phys.
Leto izida:2015

Licence

Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
Opis:Najbolj omejujoča licenca Creative Commons. Uporabniki lahko prenesejo in delijo delo v nekomercialne namene in ga ne smejo uporabiti za nobene druge namene.
Začetek licenciranja:24.04.2020

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