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  • In the fluorescence detection of ultra high energy cosmic rays, the number of emitted fluorescence photons is assumed to be proportional to the energy deposited in air by shower particles. We have performed measurements of the fluorescence yield in atmospheric gases excited by electrons over energies ranging from keV to hundreds of MeV in several accelerators. We found that within the measured energy ranges the proportionality holds at the level of few %.
  • In the fluorescence detection of ultra high energy cosmic rays, the number of emitted fluorescence photons is assumed to be proportional to the energy deposited in air by shower particles. We have performed measurements of the fluorescence yield in atmospheric gases excited by electrons over energies ranging from keV to hundreds of MeV in several accelerators. We found that within the measured energy ranges the proportionality holds at the level of few %. (en)
Title
  • Energy dependence of air fluorescence yield measured by AIRFLY
  • Energy dependence of air fluorescence yield measured by AIRFLY (en)
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  • Energy dependence of air fluorescence yield measured by AIRFLY
  • Energy dependence of air fluorescence yield measured by AIRFLY (en)
skos:notation
  • RIV/68407700:21220/08:00149857!RIV10-GA0-21220___
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  • P(1M06002), P(GA202/05/2470), P(LA08016), P(LC527), Z(AV0Z10100502), Z(AV0Z10100522)
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  • 1
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  • 366208
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  • RIV/68407700:21220/08:00149857
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  • Energy deposit; air fluorescence detection; ultra high energy cosmic rays (en)
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  • NL - Nizozemsko
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  • [6FA1BFA9FC74]
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  • Nuclear Instruments and Methods in Physics Research, Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
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  • 597
http://linked.open...iv/tvurceVysledku
  • Vacek, Václav
  • Doubrava, Michal
http://linked.open...ain/vavai/riv/wos
  • 000261700600006
http://linked.open...n/vavai/riv/zamer
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  • 0168-9002
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  • 21220
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