Formation and propagation of cosmic-ray ensembles

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作者
Sushchov, Oleksandr [1 ]
Homola, Piotr [1 ]
Alvarez Castillo, David E. [1 ,2 ]
Beznosko, Dmitriy [3 ]
Budnev, Nikolai [4 ]
Gora, Dariusz [1 ]
Gupta, Alok C. [5 ]
Hnatyk, Bohdan [6 ]
Kasztelan, Marcin [7 ]
Kovacs, Peter [8 ]
Lozowski, Bartosz [9 ]
Medvedev, Mikhail V. [10 ,11 ]
Miszczyk, Justyna [1 ]
Mozgova, Alona [6 ]
Nazari, Vahab [1 ,2 ]
Niedzwiecki, Michal [12 ]
Pawlik, Maciej [13 ,14 ]
Rosas, Matias [15 ]
Rzecki, Krzysztof [14 ]
Smelcerz, Katarzyna [12 ]
Smolek, Karel [16 ]
Stasielak, Jaroslaw [1 ]
Stuglik, Slawomir [1 ]
Svanidze, Manana [17 ]
Tursunov, Arman [18 ]
Verbetsky, Yuri [17 ]
Wibig, Tadeusz [19 ]
Zamora-Saa, Jilberto [20 ]
机构
[1] Polish Acad Sci, Inst Nucl Phys, Radzikowskiego 152, PL-31342 Krakow, Poland
[2] Joint Inst Nucl Res, Dubna 141980, Russia
[3] Clayton State Univ, Morrow, GA USA
[4] Irkutsk State Univ, Irkutsk, Russia
[5] Aryabhatta Res Inst Observat Sci ARIES, Manora Peak, Naini Tal 263001, India
[6] Taras Shevchenko Natl Univ Kyiv, Astron Observ, UA-04053 Kiev, Ukraine
[7] Natl Ctr Nucl Res, Andrzeja Soltana 7, PL-05400 Otwock, Poland
[8] Inst Particle & Nucl Phys, Wigner Res Ctr Phys, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary
[9] Univ Silesia Katowice, Fac Nat Sci, Bankowa 9, PL-40007 Katowice, Poland
[10] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
[11] MIT, Lab Nucl Sci, Cambridge, MA 02139 USA
[12] Cracow Univ Technol, Fac Comp Sci & Telecommun, Dept Comp Sci, Warszawska 24, PL-31155 Krakow, Poland
[13] ACC Cyfronet AGH UST, PL-30950 Krakow, Poland
[14] AGH Univ Sci & Technol, Mickiewicz Ave, PL-30059 Krakow, Poland
[15] Liceo 6 Francisco Bauza, Montevideo, Uruguay
[16] Czech Tech Univ, Inst Expt & Appl Phys, Prague, Czech Republic
[17] Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Georgia
[18] Silesian Univ Opava, Inst Phys, Res Ctr Theoret Phys & Astrophys, Bezrucovo 13, CZ-74601 Opava, Czech Republic
[19] Univ Lodz, Fac Phys & Appl Informat, Pomorska 149-153, PL-90236 Lodz, Poland
[20] Univ Andres Bello, Fac Ciencias Exactas, Dept Ciencias Fisicas, Ave Republ 498, Santiago, Chile
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P1 [天文学];
学科分类号
0704 ;
摘要
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.
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