Characterization of muon simulations for the scintillator detector BATATA located at the Pierre Auger Observatory
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00551096" target="_blank" >RIV/68378271:_____/17:00551096 - isvavai.cz</a>
Výsledek na webu
<a href="https://iopscience.iop.org/article/10.1088/1742-6596/866/1/012005/pdf" target="_blank" >https://iopscience.iop.org/article/10.1088/1742-6596/866/1/012005/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1742-6596/866/1/012005" target="_blank" >10.1088/1742-6596/866/1/012005</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Characterization of muon simulations for the scintillator detector BATATA located at the Pierre Auger Observatory
Popis výsledku v původním jazyce
Ultra-High energy Cosmic rays (UHECR) reach us from our Galaxy and from extragalactic space. Their origin is still unknown and their study is one of the main aims of the Pierre Auger Observatory. The underground detector Buried Array Telescope at Auger (BATATA) was designed as part of the low energy enhancement of the Observatory. This telescope is a 3 m side cube with the main goal of analyzing the muon component from air showers produced by primary Cosmic Rays (CR) and quantifying the electromagnetic contamination of the muon signal as a function of depth in the 10 and 10 eV energy range. The objective of this work is to characterize the functionality of simulations developed exclusively for BATATA in order to understand the behavior of the muon component in the detector. This is done by comparing the simulations with analytical calculations. In this work, results on comparisons of the muon component are presented.n
Název v anglickém jazyce
Characterization of muon simulations for the scintillator detector BATATA located at the Pierre Auger Observatory
Popis výsledku anglicky
Ultra-High energy Cosmic rays (UHECR) reach us from our Galaxy and from extragalactic space. Their origin is still unknown and their study is one of the main aims of the Pierre Auger Observatory. The underground detector Buried Array Telescope at Auger (BATATA) was designed as part of the low energy enhancement of the Observatory. This telescope is a 3 m side cube with the main goal of analyzing the muon component from air showers produced by primary Cosmic Rays (CR) and quantifying the electromagnetic contamination of the muon signal as a function of depth in the 10 and 10 eV energy range. The objective of this work is to characterize the functionality of simulations developed exclusively for BATATA in order to understand the behavior of the muon component in the detector. This is done by comparing the simulations with analytical calculations. In this work, results on comparisons of the muon component are presented.n
Klasifikace
Druh
D - Stať ve sborníku
CEP obor
—
OECD FORD obor
10303 - Particles and field physics
Návaznosti výsledku
Projekt
—
Návaznosti
—
Ostatní
Rok uplatnění
2017
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název statě ve sborníku
Journal of Physics: Conference Series
ISBN
—
ISSN
1742-6588
e-ISSN
—
Počet stran výsledku
7
Strana od-do
1-7
Název nakladatele
IOP Publishing Ltd
Místo vydání
Bristol
Místo konání akce
Chiapas
Datum konání akce
17. 11. 2015
Typ akce podle státní příslušnosti
WRD - Celosvětová akce
Kód UT WoS článku
000409415200005