A method of observing Cherenkov light at the Yakutsk EAS array

A proposed new method for measuring the cherenkov light from extensive air showers (EAS) of cosmic rays (CR), which allows to determine not only the primary particle energy and angle of arrival, but also the parameters of the shower in the atmosphere – the maximum depth and “age”. For measurements i...

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Main Authors: Timofeev Lev, Ivanov Anatoly
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201714514002
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author Timofeev Lev
Ivanov Anatoly
author_facet Timofeev Lev
Ivanov Anatoly
author_sort Timofeev Lev
collection DOAJ
description A proposed new method for measuring the cherenkov light from extensive air showers (EAS) of cosmic rays (CR), which allows to determine not only the primary particle energy and angle of arrival, but also the parameters of the shower in the atmosphere – the maximum depth and “age”. For measurements it is proposed to use Cherenkov light produced by EAS in a ground network of wide-angle telescopes which are separated from each other by a distance 100–300 m depending on the total number of telescopes operating in coincidence, acting autonomously, or includes a detector of the charged components, radio waves, etc. as part of the EAS. Results of such an array should be developed. The energy measurement and CR angle of the arrival data on the depth of the maximum and the associated mass of the primary particle generating by EAS. This is particularly important in the study of galactic cosmic ray for E > 1014 eV, where currently there are no direct measurements of the maximum depth of the EAS.
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spelling doaj.art-6e78a7137f8d46f8b737b487b5de9a132022-12-21T22:10:23ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011451400210.1051/epjconf/201714514002epjconf-isvhecri2016_14002A method of observing Cherenkov light at the Yakutsk EAS arrayTimofeev Lev0Ivanov Anatoly1The Yu.G. Shafer Institute of Cosmophysical Research and AeronomyThe Yu.G. Shafer Institute of Cosmophysical Research and AeronomyA proposed new method for measuring the cherenkov light from extensive air showers (EAS) of cosmic rays (CR), which allows to determine not only the primary particle energy and angle of arrival, but also the parameters of the shower in the atmosphere – the maximum depth and “age”. For measurements it is proposed to use Cherenkov light produced by EAS in a ground network of wide-angle telescopes which are separated from each other by a distance 100–300 m depending on the total number of telescopes operating in coincidence, acting autonomously, or includes a detector of the charged components, radio waves, etc. as part of the EAS. Results of such an array should be developed. The energy measurement and CR angle of the arrival data on the depth of the maximum and the associated mass of the primary particle generating by EAS. This is particularly important in the study of galactic cosmic ray for E > 1014 eV, where currently there are no direct measurements of the maximum depth of the EAS.https://doi.org/10.1051/epjconf/201714514002
spellingShingle Timofeev Lev
Ivanov Anatoly
A method of observing Cherenkov light at the Yakutsk EAS array
EPJ Web of Conferences
title A method of observing Cherenkov light at the Yakutsk EAS array
title_full A method of observing Cherenkov light at the Yakutsk EAS array
title_fullStr A method of observing Cherenkov light at the Yakutsk EAS array
title_full_unstemmed A method of observing Cherenkov light at the Yakutsk EAS array
title_short A method of observing Cherenkov light at the Yakutsk EAS array
title_sort method of observing cherenkov light at the yakutsk eas array
url https://doi.org/10.1051/epjconf/201714514002
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