Effects of the direct light in the surface detectors (SD) of the Pierre Auger Observatory and their change in time
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00551099" target="_blank" >RIV/68378271:_____/17:00551099 - isvavai.cz</a>
Výsledek na webu
<a href="https://iopscience.iop.org/article/10.1088/1742-6596/866/1/012012/pdf" target="_blank" >https://iopscience.iop.org/article/10.1088/1742-6596/866/1/012012/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1742-6596/866/1/012012" target="_blank" >10.1088/1742-6596/866/1/012012</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Effects of the direct light in the surface detectors (SD) of the Pierre Auger Observatory and their change in time
Popis výsledku v původním jazyce
Cosmic Rays (CR) are particles which come to the earth from Universe. Their origin and production mechanisms are still unknown. The Pierre Auger Observatory is located in Mendoza, Argentina. It is dedicated to the study of CR. When CR arrive to the earth's atmosphere they produce a shower of secondary particles called air shower. The surface detector (SD) of the Pierre Auger Observatory consists of tanks full of pure water, where CR produce Cherenkov radiation, when going through them. This light is detected by three photomultiplier tubes (PMT) located on the top of each tank. Depending of the angle of arrival direction of the primary CR, each PMT is able to register different signal than the other. The goal of this study is to look at these effects of direct light on the PMT's to explore if they change in time.nn
Název v anglickém jazyce
Effects of the direct light in the surface detectors (SD) of the Pierre Auger Observatory and their change in time
Popis výsledku anglicky
Cosmic Rays (CR) are particles which come to the earth from Universe. Their origin and production mechanisms are still unknown. The Pierre Auger Observatory is located in Mendoza, Argentina. It is dedicated to the study of CR. When CR arrive to the earth's atmosphere they produce a shower of secondary particles called air shower. The surface detector (SD) of the Pierre Auger Observatory consists of tanks full of pure water, where CR produce Cherenkov radiation, when going through them. This light is detected by three photomultiplier tubes (PMT) located on the top of each tank. Depending of the angle of arrival direction of the primary CR, each PMT is able to register different signal than the other. The goal of this study is to look at these effects of direct light on the PMT's to explore if they change in time.nn
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
5
Strana od-do
1-5
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
000409415200012