Formation and propagation of cosmic-ray ensembles

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F22%3AA0000241" target="_blank" >RIV/47813059:19630/22:A0000241 - isvavai.cz</a>
Alternative codes found
RIV/68407700:21670/22:00373859
Result on the web
<a href="https://pos.sissa.it/395/465/" target="_blank" >https://pos.sissa.it/395/465/</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0465" target="_blank" >10.22323/1.395.0465</a>

Result language
angličtina
Original language name
Formation and propagation of cosmic-ray ensembles
Original language description
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.
Czech name
—
Czech description
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Project
<a href="/en/project/EF16_019%2F0000766" target="_blank" >EF16_019/0000766: Engineering applications of microworld physics</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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