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 and Marcin PIEKARCZYK. Simulations of Cosmic Ray Ensembles originated nearby the Sun. Online. In Proceedings of Science. Itálie: Sissa Medialab Srl, 2022, p. " 457-1"-" 457-8", 8 pp. ISSN 1824-8039. Available from: https://dx.doi.org/10.22323/1.395.0457. |
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@inproceedings{66781, 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, Michał and Pawlik, Maciej and Rosas, Matías and Rzecki, Krzysztof and Smelcerz, Katarzyna and Smolek, Karel and Stasielak, Jarosław and Stuglik, Sławomir and Svanidze, Manana and Tursunov, Arman and Verbetsky, Yuri and Wibig, Tadeusz and ZamoraandSaa, Jilberto and Poncyljusz, Bożena and Medrala, Justyna and Opiła, Gabriela and Bibrzyck, Łukasz and Piekarczyk, Marcin}, address = {Itálie}, booktitle = {Proceedings of Science}, doi = {http://dx.doi.org/10.22323/1.395.0457}, keywords = {Cosmic Ray Ensembles;Cosmic rays;Cascade forms; Electromagnetic cascades; Electron pair; Higher energy photons; Particles distribution; Solar magnetic fields; Ultra-high energies}, howpublished = {elektronická verze "online"}, language = {eng}, location = {Itálie}, pages = {" 457-1"-" 457-8"}, publisher = {Sissa Medialab Srl}, title = {Simulations of Cosmic Ray Ensembles originated nearby the Sun}, url = {https://pos.sissa.it/395/457}, year = {2022} }
TY - JOUR ID - 66781 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, Michał - Pawlik, Maciej - Rosas, Matías - Rzecki, Krzysztof - Smelcerz, Katarzyna - Smolek, Karel - Stasielak, Jarosław - Stuglik, Sławomir - Svanidze, Manana - Tursunov, Arman - Verbetsky, Yuri - Wibig, Tadeusz - Zamora-Saa, Jilberto - Poncyljusz, Bożena - Medrala, Justyna - Opiła, Gabriela - Bibrzyck, Łukasz - Piekarczyk, Marcin PY - 2022 TI - Simulations of Cosmic Ray Ensembles originated nearby the Sun PB - Sissa Medialab Srl CY - Itálie KW - Cosmic Ray Ensembles;Cosmic rays;Cascade forms KW - Electromagnetic cascades KW - Electron pair KW - Higher energy photons KW - Particles distribution KW - Solar magnetic fields KW - Ultra-high energies UR - https://pos.sissa.it/395/457 N2 - 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. 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, Michał NIED$\backslash$'ZWIECKI, 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, Bo$\backslash$.zena PONCYLJUSZ, Justyna MEDRALA, Gabriela OPIŁA, Łukasz BIBRZYCK and Marcin PIEKARCZYK. Simulations of Cosmic Ray Ensembles originated nearby the Sun. Online. In \textit{Proceedings of Science}. Itálie: Sissa Medialab Srl, 2022, p.~'' 457-1''-'' 457-8'', 8 pp. ISSN~1824-8039. Available from: https://dx.doi.org/10.22323/1.395.0457.
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