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Volumn 574, Issue 2, 2007, Pages 255-263

The response function of the Aragats Solar Neutron Telescope

Author keywords

Monte Carlo simulation; Particle detectors; Solar cosmic rays

Indexed keywords

BROADBAND NETWORKS; COMMUNICATION CHANNELS (INFORMATION THEORY); COMPUTER SIMULATION; COSMIC RAYS; NEUTRON DETECTORS;

EID: 34047257655     PISSN: 01689002     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nima.2007.02.097     Document Type: Article
Times cited : (18)

References (19)
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    • A.A. Chilingarian, et al., in: Proceedings of the 26th ICRC, Salt-Lake-City, vol. 1., 1999, p. 240.
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    • GEANT3.21-Detector Description and Simulation Tool, CERN Program Library Long Writeup W5013, CERN, 1993.
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    • D. Heck, et al., Forschungszentrum Karlsryhe, FZKA Report 6019, 1998.
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    • J.A. Tsyrlin, Light-collection in scintillation counters, Atomizdat, 1975 (in Russian).
  • 12
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    • Phys. Rev. D Particles and Fields, Part I, Review of Particle Physics, 2002, p. 84.
  • 13
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    • E. Mnatsakanyan, et al., Calibration of the scintillation detectors of the particles density of the EAS. Preprint YerPhI 1610(8), 2006.
  • 16
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    • 〈http://cosray.unibe.ch/~laurent/planetocosmics/〉.
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    • M.Z. Zazyan, A.A. Chilingaryan, On the possibility to deduce proton energy spectrum of the 20 January 2005 GLE using Aragats and nor-amberd neutron monitors data, in: Proceedings of the 2nd International Symposium SEE-2005, Nor-Amberd, Armenia, 2005, pp. 200-202.
  • 19
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    • ACE News #87-Feb 23, 2005. Space Weather Aspects of the January 20, 2005 Solar Energetic Particle Event, 〈www.srl.caltech.edu/ACE/ACENews/ACENews87.html〉.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.