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Reconstruction of Cherenkov radiation signals from extensive air showers of cosmic rays using data of a wide field-of-view telescope.

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Title: Reconstruction of Cherenkov radiation signals from extensive air showers of cosmic rays using data of a wide field-of-view telescope.
Authors: Ivanov, A. A.1 (AUTHOR) ivanov@ikfia.ysn.ru, Matarkin, S. V.1 (AUTHOR), Timofeev, L. V.1 (AUTHOR)
Source: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology. Apr2020, Vol. 29 Issue 5, pN.PAG-N.PAG. 16p.
Subjects: Cherenkov radiation, Cosmic ray showers, Cosmic rays, Data acquisition systems, Telescopes, Very large array telescopes
Geographic Terms: IAkutsk (Russia)
Abstract: The operation of a wide field-of-view (WFOV) Cherenkov telescope is described. The detection of extensive air showers (EASs) of cosmic rays (CRs) is based upon the coincidence with signals from the Yakutsk array. The data acquisition system of the telescope yields signals connected with EAS development parameters: presumably, shower age and position of shower maximum in the atmosphere. Here, we describe the method of signal processing used to reconstruct Cherenkov radiation signals induced by CR showers. An analysis of signal parameters results in the confirmation of the known correlation of the duration of the Cherenkov radiation signal with the distance to the shower core. The measured core distance dependence is used to set an upper limit to the dimensions of the area along the EAS axis where the Cherenkov radiation intensity is above half-peak amplitude. [ABSTRACT FROM AUTHOR]
Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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DbLabel: Engineering Source
An: 143042183
AccessLevel: 6
PubType: Academic Journal
PubTypeId: academicJournal
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  Data: Reconstruction of Cherenkov radiation signals from extensive air showers of cosmic rays using data of a wide field-of-view telescope.
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– Name: Abstract
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  Data: The operation of a wide field-of-view (WFOV) Cherenkov telescope is described. The detection of extensive air showers (EASs) of cosmic rays (CRs) is based upon the coincidence with signals from the Yakutsk array. The data acquisition system of the telescope yields signals connected with EAS development parameters: presumably, shower age and position of shower maximum in the atmosphere. Here, we describe the method of signal processing used to reconstruct Cherenkov radiation signals induced by CR showers. An analysis of signal parameters results in the confirmation of the known correlation of the duration of the Cherenkov radiation signal with the distance to the shower core. The measured core distance dependence is used to set an upper limit to the dimensions of the area along the EAS axis where the Cherenkov radiation intensity is above half-peak amplitude. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1142/S0218271820500339
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      – Code: eng
        Text: English
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        PageCount: 16
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      – SubjectFull: Cherenkov radiation
        Type: general
      – SubjectFull: Cosmic ray showers
        Type: general
      – SubjectFull: Cosmic rays
        Type: general
      – SubjectFull: Data acquisition systems
        Type: general
      – SubjectFull: Telescopes
        Type: general
      – SubjectFull: Very large array telescopes
        Type: general
      – SubjectFull: IAkutsk (Russia)
        Type: general
    Titles:
      – TitleFull: Reconstruction of Cherenkov radiation signals from extensive air showers of cosmic rays using data of a wide field-of-view telescope.
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            NameFull: Ivanov, A. A.
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            NameFull: Matarkin, S. V.
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            NameFull: Timofeev, L. V.
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              M: 04
              Text: Apr2020
              Type: published
              Y: 2020
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            – TitleFull: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology
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