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, Michał NIEDŹWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Manana SVANIDZE, Arman TURSUNOV, Yuri VERBETSKY, Tadeusz WIBIG, Jilberto ZAMORA-SAA, Bożena PONCYLJUSZ, Justyna MEDRALA, Gabriela OPIŁA, Łukasz BIBRZYCK a Marcin PIEKARCZYK. Simulations of Cosmic Ray Ensembles originated nearby the Sun. Online. In Proceedings of Science. Itálie: Sissa Medialab Srl, 2022, s. " 457-1"-" 457-8", 8 s. ISSN 1824-8039. Dostupné z: https://dx.doi.org/10.22323/1.395.0457.
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Základní údaje
Originální název Simulations of Cosmic Ray Ensembles originated nearby the Sun
Autoři 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, Michał NIEDŹWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Manana SVANIDZE, Arman TURSUNOV (860 Uzbekistán, domácí), Yuri VERBETSKY, Tadeusz WIBIG, Jilberto ZAMORA-SAA, Bożena PONCYLJUSZ, Justyna MEDRALA, Gabriela OPIŁA, Łukasz BIBRZYCK a Marcin PIEKARCZYK.
Vydání Itálie, Proceedings of Science, od s. " 457-1"-" 457-8", 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:A0000251
Organizační jednotka Fyzikální ústav v Opavě
ISSN 1824-8039
Doi http://dx.doi.org/10.22323/1.395.0457
Klíčová slova anglicky Cosmic Ray Ensembles;Cosmic rays;Cascade forms; Electromagnetic cascades; Electron pair; Higher energy photons; Particles distribution; Solar magnetic fields; Ultra-high energies
Štítky , RIV23
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Pavlína Jalůvková, učo 25213. Změněno: 16. 2. 2023 13:14.
Anotace
Cosmic Ray Ensembles (CRE) are yet not observed groups of cosmic rays with a common primary interaction vertex or the same parent particle. One of the processes capable of initiating identifiable CRE is an interaction of an ultra-high energy (UHE) photon with the solar magnetic field which results in an electron pair production and the subsequent synchrotron radiation. The resultant electromagnetic cascade forms a very characteristic line-like front of a very small width (∼ meters), stretching from tens of thousands to even many millions of kilometers. In this contribution we present the results of applying a toy model to simulate detections of such CRE at the ground level with an array of ideal detectors of different dimensions. The adopted approach allows us to assess the CRE detection feasibility for a specific configuration of a detector array. The process of initiation and propagation of an electromagnetic cascade originated from an UHE photon passing near the Sun, as well as the resultant particle distribution on ground, were simulated using the CORSIKA program with the PRESHOWER option, both modified accordingly. The studied scenario results in photons forming a cascade that extends even over tens of millions of kilometers when it arrives at the top of the Earth's atmosphere, and the photon energies span practically the whole cosmic ray energy spectrum. The topology of the signal consists of very extended CRE shapes, and the characteristic, very much elongated disk-shape of the particle distribution on ground illustrates the potential for identification of CRE of this type.
VytisknoutZobrazeno: 6. 5. 2024 18:39