Formation and propagation of cosmic-ray ensembles

@inproceedings{66642,
   author = {Sushchov, Oleksandr and Homola, Piotr and Alvarez Castillo, David E. and Beznosko, Dmitriy and Budnev, Nikolai and Góra, Dariusz and Gupta, Alok C. and Hnatyk, Bohdan and Kasztelan, Marcin and Kovacs, Peter and Łozowski, Bartosz and Medvedev, Mikhail V. and Miszczyk, Justyna and Mozgova, Alona and Nazari, Vahab and Niedźwiecki, Michal and Pawlik, Maciej and Rosas, Matías and Rzecki, Krzysztof and Smelcerz, Katarzyna and Smolek, Karel and Stasielak, Jaroslaw and Stuglik, Slawomir and Svanidze, Manana and Tursunov, Arman and Verbetsky, Yuri and Wibig, Tadeusz and ZamoraandSaa, Jilberto},
   address = {Itálie},
   booktitle = {Proceedings of Science},
   doi = {http://dx.doi.org/10.22323/1.395.0465},
   keywords = {Cosmology;Monte Carlo methods;Synchrotron radiation;Cosmic rays},
   howpublished = {elektronická verze "online"},
   language = {eng},
   location = {Itálie},
   pages = {"465-1"-"465-9"},
   publisher = {Sissa Medialab Srl},
   title = {Formation and propagation of cosmic-ray ensembles},
   url = {https://pos.sissa.it/395/465/},
   year = {2022}
}

TY  - JOUR
ID  - 66642
AU  - Sushchov, Oleksandr - Homola, Piotr - Alvarez Castillo, David E. - Beznosko, Dmitriy - Budnev, Nikolai - Góra, Dariusz - Gupta, Alok C. - Hnatyk, Bohdan - Kasztelan, Marcin - Kovacs, Peter - Łozowski, Bartosz - Medvedev, Mikhail V. - Miszczyk, Justyna - Mozgova, Alona - Nazari, Vahab - Niedźwiecki, Michal - Pawlik, Maciej - Rosas, Matías - Rzecki, Krzysztof - Smelcerz, Katarzyna - Smolek, Karel - Stasielak, Jaroslaw - Stuglik, Slawomir - Svanidze, Manana - Tursunov, Arman - Verbetsky, Yuri - Wibig, Tadeusz - Zamora-Saa, Jilberto
PY  - 2022
TI  - Formation and propagation of cosmic-ray ensembles
PB  - Sissa Medialab Srl
CY  - Itálie
KW  - Cosmology;Monte Carlo methods;Synchrotron radiation;Cosmic rays
UR  - https://pos.sissa.it/395/465/
N2  - High-energy particles undergo different interactions while propagating through the Universe. As a result, they initiate particle cascades of various types and sizes, referred to as cosmic-ray ensembles (CRE). Since recently, Cosmic-Ray Extremely Distributed Observatory (CREDO) Collaboration aims at pursuing a mission dedicated to CRE, since this observation channel, i.e. correlated observation of cosmic rays on the global scale, complements the current approach to cosmic-ray research, which focuses on air showers initiated by individual cosmic rays. Recent results of Monte Carlo simulations showing that there might be a chance of observing a CRE originating from synchrotron radiation occurring even as far away from the Earth as at distances exceeding the Galaxy size, are presented. The issues and perspectives of the CRE-oriented research are discussed as well.
ER  - 

SUSHCHOV, Oleksandr, 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, Michal NIED$\backslash$'ZWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jaroslaw STASIELAK, Slawomir STUGLIK, Manana SVANIDZE, Arman TURSUNOV, Yuri VERBETSKY, Tadeusz WIBIG a Jilberto ZAMORA-SAA. Formation and propagation of cosmic-ray ensembles. Online. In \textit{Proceedings of Science}. Itálie: Sissa Medialab Srl, 2022, s.~''465-1''-''465-9'', 9 s. ISSN~1824-8039. Dostupné z: https://dx.doi.org/10.22323/1.395.0465.