Simulations of antenna response for the Radio Detector of the Pierre Auger Observatory

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00580162" target="_blank" >RIV/68378271:_____/23:00580162 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/23:73622855
Result on the web
<a href="https://pos.sissa.it/424/042/pdf" target="_blank" >https://pos.sissa.it/424/042/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.424.0042" target="_blank" >10.22323/1.424.0042</a>

Result language
angličtina
Original language name
Simulations of antenna response for the Radio Detector of the Pierre Auger Observatory
Original language description
After more than 15 years of successful operation, the Pierre Auger Observatory is currently undergoing a major upgrade called AugerPrime. The aim is to study the mass composition of ultra-high-energy cosmic rays. Part of the upgrade program consists in installing a Short Aperiodic Loaded Loop Antenna (SALLA) atop each of the 1660 water-Cherenkov detectors. To obtain an absolute calibration for the SALLA, the frequency and directionally dependent antenna response (or vector effective length) must be known. The characteristics of the SALLA depend on various parameters, most prominent is the considered frequency of reception and the antenna geometry. Moreover, the interaction with the structure elements and the presence of the ground has an impact.
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
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)