Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations
The experimental technique of fluorescence light measurement is used for indirect observations of cosmic ray particles at very high energies. Extensive Air Showers (EAS) initiated by Extreme Energy Cosmic Rays (EECRs), up to 100 EeV and entering the Earth’s atmosphere, are simulated with the CORSIKA...
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EDP Sciences
2019-01-01
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doaj-e48b279b0ca042fca51fd91a3cbf48a02021-08-02T07:19:19ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012080801110.1051/epjconf/201920808011epjconf_isvhecri2018_08011Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observationsBouhali ZohraDjemil TaoufikThe experimental technique of fluorescence light measurement is used for indirect observations of cosmic ray particles at very high energies. Extensive Air Showers (EAS) initiated by Extreme Energy Cosmic Rays (EECRs), up to 100 EeV and entering the Earth’s atmosphere, are simulated with the CORSIKA package. The influence of different simulation parameters on the EAS characteristics is studied, especially on the longitudinal distribution of charged particles, depth of shower maximum and energy released to the air. By taking the atmospheric scattering of light into account, the number of fluorescence photons, with wavelengths between 300-430 nm, and their arrival time distribution to an ideal space telescope are calculated.https://www.epj-conferences.org/articles/epjconf/pdf/2019/13/epjconf_isvhecri2018_08011.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Bouhali Zohra Djemil Taoufik |
spellingShingle |
Bouhali Zohra Djemil Taoufik Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations EPJ Web of Conferences |
author_facet |
Bouhali Zohra Djemil Taoufik |
author_sort |
Bouhali Zohra |
title |
Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
title_short |
Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
title_full |
Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
title_fullStr |
Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
title_full_unstemmed |
Simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
title_sort |
simulation of the fluorescence signal detected by a space telescope for extreme energy cosmic ray observations |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2019-01-01 |
description |
The experimental technique of fluorescence light measurement is used for indirect observations of cosmic ray particles at very high energies. Extensive Air Showers (EAS) initiated by Extreme Energy Cosmic Rays (EECRs), up to 100 EeV and entering the Earth’s atmosphere, are simulated with the CORSIKA package. The influence of different simulation parameters on the EAS characteristics is studied, especially on the longitudinal distribution of charged particles, depth of shower maximum and energy released to the air. By taking the atmospheric scattering of light into account, the number of fluorescence photons, with wavelengths between 300-430 nm, and their arrival time distribution to an ideal space telescope are calculated. |
url |
https://www.epj-conferences.org/articles/epjconf/pdf/2019/13/epjconf_isvhecri2018_08011.pdf |
work_keys_str_mv |
AT bouhalizohra simulationofthefluorescencesignaldetectedbyaspacetelescopeforextremeenergycosmicrayobservations AT djemiltaoufik simulationofthefluorescencesignaldetectedbyaspacetelescopeforextremeenergycosmicrayobservations |
_version_ |
1721239505876287488 |