Monte Carlo simulations for the Pierre Auger Observatory using the VO auger grid resources

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00564875" target="_blank" >RIV/68378271:_____/22:00564875 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/22:73616806
Result on the web
<a href="https://pos.sissa.it/395/232/pdf" target="_blank" >https://pos.sissa.it/395/232/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0232" target="_blank" >10.22323/1.395.0232</a>

Result language
angličtina
Original language name
Monte Carlo simulations for the Pierre Auger Observatory using the VO auger grid resources
Original language description
The Pierre Auger Observatory, located near Malargüe, Argentina, is the world's largest cosmic-ray detector. It comprises a 3000km2 surface detector and 27 fluorescence telescopes, which measure the lateral and longitudinal distributions of the many millions of air-shower particles produced in the interactions initiated by a cosmic ray in the Earth's atmosphere. The determination of the nature of cosmic rays and studies of the detector performances rely on extensive Monte Carlo simulations describing the physics processes occurring in extensive air showers and the detector responses. The aim of the Monte Carlo simulations task is to produce and provide the Auger Collaboration with reference libraries used in a wide variety of analyses.
Czech name
—
Czech description
—

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)