Initial results of a direct comparison between the Surface Detectors of the Pierre Auger Observatory and the Telescope Array

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00551699" target="_blank" >RIV/68378271:_____/16:00551699 - isvavai.cz</a>

Výsledek na webu

<a href="https://pos.sissa.it/236/393/pdf" target="_blank" >https://pos.sissa.it/236/393/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.236.0393" target="_blank" >10.22323/1.236.0393</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Initial results of a direct comparison between the Surface Detectors of the Pierre Auger Observatory and the Telescope Array

Popis výsledku v původním jazyce

The Pierre Auger Observatory (Auger) in Mendoza, Argentina and the Telescope Array (TA) in Utah, USA aim at unraveling the origin and nature of Ultra-High Energy Cosmic Rays (UHECR). At present, there appear to be subtle differences between Auger and TA results and interpretations. Joint working groups have been established and have already reported preliminary findings. From an experimental standpoint, the Surface Detectors (SD) of both experiments make use of different detection processes not equally sensitive to the components of the extensive air showers making it to the ground. In particular, the muonic component of the shower measured at ground level can be traced back to the primary composition, which is critical for understanding the origin of UHECRs.

Název v anglickém jazyce

Initial results of a direct comparison between the Surface Detectors of the Pierre Auger Observatory and the Telescope Array

Popis výsledku anglicky

The Pierre Auger Observatory (Auger) in Mendoza, Argentina and the Telescope Array (TA) in Utah, USA aim at unraveling the origin and nature of Ultra-High Energy Cosmic Rays (UHECR). At present, there appear to be subtle differences between Auger and TA results and interpretations. Joint working groups have been established and have already reported preliminary findings. From an experimental standpoint, the Surface Detectors (SD) of both experiments make use of different detection processes not equally sensitive to the components of the extensive air showers making it to the ground. In particular, the muonic component of the shower measured at ground level can be traced back to the primary composition, which is critical for understanding the origin of UHECRs.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2016

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Proceedings of Science

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

8

Strana od-do

1-8

Název nakladatele

Sissa Medilab srl

Místo vydání

Trieste

Místo konání akce

The Hague

Datum konání akce

30. 7. 2015

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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