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Volumn 21, Issue 1, 2004, Pages 71-86

Time structure of muonic showers

Author keywords

[No Author keywords available]

Indexed keywords


EID: 17044457171     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.astropartphys.2003.12.009     Document Type: Article
Times cited : (42)

References (27)
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    • M. Takeda et al. [AGASA Collaboration], Astropart. Phys. 19, 447 (2003)
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    • [High Resolution Fly's Eye Collaboration], arXiv:astro-ph/0208243
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    • The Pierre Auger Project Design Report, by Auger Collaboration, FERMILAB-PUB-96-024, Jan Auger Coll., Properties and Performance of the Prototype Instrument for the Pierre Auger Observatory, submitted to Nucl. Instr. and Meth. A
    • The Pierre Auger Project Design Report, by Auger Collaboration, FERMILAB-PUB-96-024, Jan 1996; (http://www.auger.org); Auger Coll., Properties and Performance of the Prototype Instrument for the Pierre Auger Observatory, submitted to Nucl. Instr. and Meth. A
    • (1996)
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    • See Auger papers to be presented at the ICRC conference in Tokyo
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    • (Kascade coll.)
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    • AIRES: A system for Air Shower Simulations
    • Salt Lake City
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    • Sciutto, S.J.1
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    • astro-ph/9911331
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    • μ∼2000 m
    • μ∼2000 m
    • (2000)
  • 27
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    • Note that dz/dt is negative because the delay decreases as z increases. A minus sign has been introduced in the definition of g(t) to make it positive
    • Note that dz/dt is negative because the delay decreases as z increases. A minus sign has been introduced in the definition of g(t) to make it positive


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.