ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

On the possible method of identification of two probably cognate Extensive Air Showers

NázevTitle
On the possible method of identification of two probably cognate Extensive Air ShowersOn the possible method of identification of two probably cognate Extensive Air Showers
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
Y. Verbetsky, M. Svanidze, D. Beznosko, P. Homola, K. Smolek
Klíčová slovaKeywords
cosmic ray, cosmic ray shower, CREDO
KonferenceConference
37th International Cosmic Ray Conference (Berlin, Germany, 2021-07-15)
Časopis / citaceJournal / citation
In: 37th International Cosmic Ray Conference, Proceedings of Science, 2022 · ISSN 1824-8039
RokYear
2022
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.; Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

The persistent attempts are undertaken to show existence and investigate the special pairs of Extensive Air Showers (EAS) that can be suspected in common origin in the near space, i.e. to observe some consequence of existence of Cosmic Ray Ensemble (CRE). The remote cosmic ray stations observing EAS events are useful for this investigation. Such stations are operating within the GELATICA net (GEorgian Large-area Angle and TIme Coincidence Array) and are planed within the CREDO Collaboration (Cosmic Ray Extremely Distributed Observatory) as the CREDO-Maze project. The possible criteria are developed in the paper for detecting of two specific showers which ancestors have probable mutual proximity in their past.

The persistent attempts are undertaken to show existence and investigate the special pairs of Extensive Air Showers (EAS) that can be suspected in common origin in the near space, i.e. to observe some consequence of existence of Cosmic Ray Ensemble (CRE). The remote cosmic ray stations observing EAS events are useful for this investigation. Such stations are operating within the GELATICA net (GEorgian Large-area Angle and TIme Coincidence Array) and are planed within the CREDO Collaboration (Cosmic Ray Extremely Distributed Observatory) as the CREDO-Maze project. The possible criteria are developed in the paper for detecting of two specific showers which ancestors have probable mutual proximity in their past.

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