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Titolo:
FRACTAL BEHAVIOR OF COSMIC-RAY TIME-SERIES - CHAOS OR STOCHASTICITY
Autore:
AGLIETTA M; ALESSANDRO B; ARNEODO F; BERGAMASCO L; FAUTH AC; CASTAGNOLI C; CASTELLINA A; CATTADORI C; CHIAVASSA A; CINI G; PIAZZOLI BD; FULGIONE W; GALEOTTI P; GHIA PL; MANNOCCHI G; MORELLO C; NAVARRA G; OSBORNE AR; RICCATI L; SAAVEDRA O; SERIO M; TRINCHERO GC; VALLANIA P; VERNETTO S;
Indirizzi:
CNR,IST COSMOGEOFIS TURIN ITALY IST NAZL FIS NUCL,SEZ TORINO TURIN ITALY UNIV TORINO,IST FIS GEN TURIN ITALY IST NAZL FIS NUCL,SEZ MILANO MILAN ITALY UNIV NAPLES,DIPARTIMENTO SCI FISICHE I-80134 NAPLES ITALY IST NAZL FIS NUCL,SEZ NAPOLI NAPLES ITALY
Titolo Testata:
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
fascicolo: A9, volume: 98, anno: 1993,
pagine: 15241 - 15254
SICI:
2169-9380(1993)98:A9<15241:FBOCT->2.0.ZU;2-W
Fonte:
ISI
Lingua:
ENG
Soggetto:
INTERPLANETARY MAGNETIC-FIELD; EAS-TOP ARRAY; MULTIFRACTAL STRUCTURE; CORRELATION DIMENSION; STRANGE ATTRACTORS; RECURRENT STREAMS; 1-AU;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Science Citation Index Expanded
Science Citation Index Expanded
Science Citation Index Expanded
Citazioni:
26
Recensione:
Indirizzi per estratti:
Citazione:
M. Aglietta et al., "FRACTAL BEHAVIOR OF COSMIC-RAY TIME-SERIES - CHAOS OR STOCHASTICITY", J GEO R-S P, 98(A9), 1993, pp. 15241-15254

Abstract

This paper presents results on the fractal and statistical behavior of cosmic ray time series detected in an air shower experiment located at 2000-m altitude above the underground Gran Sasso Laboratory, Italy. We consider single particles (muons), corresponding to primary energies of greater-than-or-equal-to 10 GeV, and air showers, corresponding to primary energies of greater-than-or-equal-to 80 TeV. For all time series the analysis indicates a clear stochastic monofractal. non-Gaussian character; comparing these results with those obtained for underground muons and for neutron monitors, we conclude that these propertieslikely belong in general to cosmic ray time series, irrespective of the nature of the particles and the energies of their progenitors. In particular, the air shower time series from high-energy primaries have a fractal dimension larger than the single-muon time series originating from low-energy primaries.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 30/11/20 alle ore 19:33:15