Cosmic Rays with Energy Above 10^{17} ev

The energy spectrum of primary cosmic rays with ultra high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis...

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Main Authors: Egorova, V P, Glushkov, A V, Ivanov, A A, Knurenko, S P, Kolosov, V A, Krasilnikov, A D, Makarov, I T, Mikhailov, A A, Olzoyev, V V, Pravdin, M I, Sabourov, A V, Sleptsov, I Ye, Struchkov, G G
Language:English
Published: 2004
Subjects:
Online Access:http://cds.cern.ch/record/807483
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author Egorova, V P
Glushkov, A V
Ivanov, A A
Knurenko, S P
Kolosov, V A
Krasilnikov, A D
Makarov, I T
Mikhailov, A A
Olzoyev, V V
Pravdin, M I
Sabourov, A V
Sleptsov, I Ye
Struchkov, G G
author_facet Egorova, V P
Glushkov, A V
Ivanov, A A
Knurenko, S P
Kolosov, V A
Krasilnikov, A D
Makarov, I T
Mikhailov, A A
Olzoyev, V V
Pravdin, M I
Sabourov, A V
Sleptsov, I Ye
Struchkov, G G
author_sort Egorova, V P
collection CERN Document Server (CDS)
description The energy spectrum of primary cosmic rays with ultra high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered.
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spelling ftcern:oai:cds.cern.ch:807483 2025-01-17T01:19:30+00:00 Cosmic Rays with Energy Above 10^{17} ev Egorova, V P Glushkov, A V Ivanov, A A Knurenko, S P Kolosov, V A Krasilnikov, A D Makarov, I T Mikhailov, A A Olzoyev, V V Pravdin, M I Sabourov, A V Sleptsov, I Ye Struchkov, G G 2004-11-25 http://cds.cern.ch/record/807483 eng eng http://cds.cern.ch/record/807483 astro-ph/0411685 oai:cds.cern.ch:807483 Astrophysics and Astronomy 2004 ftcern 2018-07-28T07:04:03Z The energy spectrum of primary cosmic rays with ultra high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered. Other/Unknown Material Yakutsk CERN Document Server (CDS) Yakutsk
spellingShingle Astrophysics and Astronomy
Egorova, V P
Glushkov, A V
Ivanov, A A
Knurenko, S P
Kolosov, V A
Krasilnikov, A D
Makarov, I T
Mikhailov, A A
Olzoyev, V V
Pravdin, M I
Sabourov, A V
Sleptsov, I Ye
Struchkov, G G
Cosmic Rays with Energy Above 10^{17} ev
title Cosmic Rays with Energy Above 10^{17} ev
title_full Cosmic Rays with Energy Above 10^{17} ev
title_fullStr Cosmic Rays with Energy Above 10^{17} ev
title_full_unstemmed Cosmic Rays with Energy Above 10^{17} ev
title_short Cosmic Rays with Energy Above 10^{17} ev
title_sort cosmic rays with energy above 10^{17} ev
topic Astrophysics and Astronomy
topic_facet Astrophysics and Astronomy
url http://cds.cern.ch/record/807483