STANEK, Weronika, Jerzy PRYGA, Krzysztof W. WOŹNIAK, Piotr HOMOLA, David E. ALVAREZ CASTILLO, Dmitriy BEZNOSKO, Nikolai BUDNEV, Dariusz GÓRA, Alok C. GUPTA, Bohdan HNATYK, Marcin KASZTELAN, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Justyna MISZCZYK, Alona MOZGOVA, Vahab NAZARI, Michał NIEDŹWIECKI, Matías ROSAS, Krzysztof RZECKI, Smelcerz KATARZYNA, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Oleksandr SUSHCHOV, Arman TURSUNOV, Tadeusz WIBIG a Jilberto ZAMORA-SAA. Particle density fluctuations and correlations in low energy Cosmic-Ray showers simulated with CORSIKA. Online. In Proceedings of Science. Itálie: Sissa Medialab Srl, 2022, s. "462-1"-"462-8", 8 s. ISSN 1824-8039. Dostupné z: https://dx.doi.org/10.22323/1.395.0462.
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Základní údaje
Originální název Particle density fluctuations and correlations in low energy Cosmic-Ray showers simulated with CORSIKA
Autoři STANEK, Weronika, Jerzy PRYGA, Krzysztof W. WOŹNIAK, Piotr HOMOLA, David E. ALVAREZ CASTILLO, Dmitriy BEZNOSKO, Nikolai BUDNEV, Dariusz GÓRA, Alok C. GUPTA, Bohdan HNATYK, Marcin KASZTELAN, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Justyna MISZCZYK, Alona MOZGOVA, Vahab NAZARI, Michał NIEDŹWIECKI, Matías ROSAS, Krzysztof RZECKI, Smelcerz KATARZYNA, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Oleksandr SUSHCHOV, Arman TURSUNOV (860 Uzbekistán, domácí), Tadeusz WIBIG a Jilberto ZAMORA-SAA.
Vydání Itálie, Proceedings of Science, od s. "462-1"-"462-8", 8 s. 2022.
Nakladatel Sissa Medialab Srl
Další údaje
Originální jazyk angličtina
Typ výsledku Stať ve sborníku
Obor 10308 Astronomy
Stát vydavatele Itálie
Utajení není předmětem státního či obchodního tajemství
Forma vydání elektronická verze "online"
WWW URL
Kód RIV RIV/47813059:19630/22:A0000240
Organizační jednotka Fyzikální ústav v Opavě
ISSN 1824-8039
Doi http://dx.doi.org/10.22323/1.395.0462
Klíčová slova anglicky Cosmic ray showers;Density correlation;Density fluctuation;Lower energies;High-energy particles;
Štítky , RIV23
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Pavlína Jalůvková, učo 25213. Změněno: 15. 2. 2023 15:38.
Anotace
The current studies of cosmic rays are focused on most energetic particles entering the atmosphere and producing a single Extensive Air Shower (EAS). There are, however, models predicting that interactions of high energy particles may result in Cosmic-Ray Ensembles (CRE) created far from the Earth. They could be observed as some number of correlated air showers of relatively low energies spread over a large area. The objective of the Cosmic Ray Extremely Distributed Observatory (CREDO) is to search for CRE using all available data from different detectors and observatories including even small but numerous detectors spread over large areas. Interpretation of such measurements require precise information on properties of EAS in a very wide energy spectrum. Low energy EAS are analysed using events from CORSIKA, the program performing air shower simulations. The primary cosmic ray particle energy range extends from 1 TeV up to 4 000 TeV. The secondary particles at the ground level are studied in order to obtain their density fluctuations and correlations in location. Although the fluctuations observed in multiplicity distributions are consistent with random the more detailed analysis reveals that near a selected particle the density of other particles is enhanced over that expected in the absence of correlations. The results of this analysis may be useful in further calculations, for example to obtain probability of detection of an EAS without special simulations.
VytisknoutZobrazeno: 6. 5. 2024 22:11