Pierre Auger Observatory - triggers

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00617545" target="_blank" >RIV/68378271:_____/24:00617545 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Pierre Auger Observatory - triggers
Original language description
The Pierre Auger Observatory is conceived to study ultra-high-energy cosmic rays from about 10^17 eV to beyond 10^20 eV. It is a multi-hybrid Observatory comprising 1660 surface detector stations spread over an area of 3000 km^2 overlooked by 27 fluorescence telescopes located at four sites at its periphery. Phase I of data-taking spanned from its beginning in 2004 to the end of 2022, producing a plethora of scientific results. Phase II followed, featuring an upgraded Observatory with additional detectors and faster, more powerful electronics, enabling the exploration of new questions in ultra-high-energy physics. The triggering system of the Observatory in the Phase I will be described and compared with the new capabilities of the upgraded Observatory in the Phase II of operations.
Czech name
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Czech description
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Project
<a href="/en/project/LM2023032" target="_blank" >LM2023032: Pierre Auger Observatory - participation of the Czech Republic</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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