2022
First Results on the Revealing of Cognate Ancestors among the Particles of the Primary Cosmic Rays That Gave Rise to Extensive Air Showers Observed by the GELATICA Network
VERBETSKY, Yuri, Manana SVANIDZE, Ophir RUIMI, Tadeusz WIBIG, Levan KAKABADZE et. al.Základní údaje
Originální název
First Results on the Revealing of Cognate Ancestors among the Particles of the Primary Cosmic Rays That Gave Rise to Extensive Air Showers Observed by the GELATICA Network
Autoři
VERBETSKY, Yuri, Manana SVANIDZE, Ophir RUIMI, Tadeusz WIBIG, Levan KAKABADZE, Piotr HOMOLA, David E ALVAREZ-CASTILLO, Dmitry BEZNOSKO, Edward K SARKISYAN-GRINBAUM, Olaf BAR, Oleksandr SUSHCHOV a Arman TURSUNOV (860 Uzbekistán, domácí)
Vydání
SYMMETRY-BASEL, Švýcarsko, 2022, 2073-8994
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Švýcarsko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Kód RIV
RIV/47813059:19630/22:A0000231
Organizační jednotka
Fyzikální ústav v Opavě
UT WoS
000845389000001
Klíčová slova anglicky
cosmic ray ensembles; large scale primary cosmic ray correlations; extensive air showers; pairs of showers; proximity estimations; CREDO collaboration
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 10. 2. 2023 10:24, Mgr. Pavlína Jalůvková
Anotace
V originále
For the data on the observation times and directions of the motion of extensive air showers, which are observed at two stations of the GELATICA network, for the first time we apply the method we have developed previously for identifying pairs of mutually remote extensive air showers, the ancestor particles of which arose, possibly, in a single process. A brief description of the GELATICA network, a review of the properties of used samples of data on shower observations at two stations of the network during the 2019-2021 session, and the result of applying the above method to them are given. Some properties of a single peculiar pair of remote showers are discussed. A side question arose about the cause of the observed temporal asymmetry in the locations of the regions of mutual approach of independent primary cosmic ray particles.