Expected performance of the AugerPrime Radio Detector

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00578892" target="_blank" >RIV/68378271:_____/23:00578892 - isvavai.cz</a>
Alternative codes found
RIV/68378271:_____/22:00564963 RIV/61989592:15310/22:73616903
Result on the web
<a href="https://pos.sissa.it/424/028/pdf" target="_blank" >https://pos.sissa.it/424/028/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.424.0028" target="_blank" >10.22323/1.424.0028</a>

Result language
angličtina
Original language name
Expected performance of the AugerPrime Radio Detector
Original language description
The Auger Radio Detector (RD) will increase the sky coverage and overall aperture for mass-sensitive measurements of ultra-high-energy cosmic rays with the Pierre Auger Observatory. The installation of over 1600 dual-polarized short aperiodic loaded loop antennas (SALLAs) on an area of about 3000km2 will enable the detection of highly inclined air showers via the emitted electromagnetic radiation in coincidence with the Auger water-Cherenkov detector array (SD). The combination of complementary information from both detectors yields a strong sensitivity to the mass composition of cosmic rays.
Czech name
—
Czech description
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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

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