All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region

Average estimations of the shower energy components are presented and their sum gives E sub 0 (Rho sub 600) - an average function of the relation of E sub 0 with the shower size parameter Rho sub 600 measured at the Yakutsk extensive air showers (EAS) array. Using this relation to the EAS spectrum o...

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Bibliographic Details
Main Authors: Ivanov, A. A., Dyakonov, M. N., Kolosov, V. A., Sleptsov, I. Y., Krasilnikov, D. D., Lischenyuk, F. F.
Format: Other/Unknown Material
Language:unknown
Published: 1985
Subjects:
SPACE RADIATION
Rho
Yakutsk
Online Access:http://hdl.handle.net/2060/19850025743
id ftnasantrs:oai:casi.ntrs.nasa.gov:19850025743
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19850025743 2023-05-15T18:45:21+02:00 All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region Ivanov, A. A. Dyakonov, M. N. Kolosov, V. A. Sleptsov, I. Y. Krasilnikov, D. D. Lischenyuk, F. F. Unclassified, Unlimited, Publicly available Aug 1, 1985 application/pdf http://hdl.handle.net/2060/19850025743 unknown Document ID: 19850025743 Accession ID: 85N34056 http://hdl.handle.net/2060/19850025743 No Copyright CASI SPACE RADIATION OG-5.1-15 19th Intern. Cosmic Ray Conf - Vol. 2; p 190-193; NASA-CP-2376-VOL-2 1985 ftnasantrs 2019-07-21T09:46:08Z Average estimations of the shower energy components are presented and their sum gives E sub 0 (Rho sub 600) - an average function of the relation of E sub 0 with the shower size parameter Rho sub 600 measured at the Yakutsk extensive air showers (EAS) array. Using this relation to the EAS spectrum obtained at the Akeno and Yakutsk arrays the energy spectrum of the cosmic ray total flux within 15 lg (E sub 0,eV) 20 by the EAS methods is recovered. Other/Unknown Material Yakutsk NASA Technical Reports Server (NTRS) Rho ENVELOPE(-63.000,-63.000,-64.300,-64.300) Yakutsk
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic SPACE RADIATION
spellingShingle SPACE RADIATION
Ivanov, A. A.
Dyakonov, M. N.
Kolosov, V. A.
Sleptsov, I. Y.
Krasilnikov, D. D.
Lischenyuk, F. F.
All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
topic_facet SPACE RADIATION
description Average estimations of the shower energy components are presented and their sum gives E sub 0 (Rho sub 600) - an average function of the relation of E sub 0 with the shower size parameter Rho sub 600 measured at the Yakutsk extensive air showers (EAS) array. Using this relation to the EAS spectrum obtained at the Akeno and Yakutsk arrays the energy spectrum of the cosmic ray total flux within 15 lg (E sub 0,eV) 20 by the EAS methods is recovered.
format Other/Unknown Material
author Ivanov, A. A.
Dyakonov, M. N.
Kolosov, V. A.
Sleptsov, I. Y.
Krasilnikov, D. D.
Lischenyuk, F. F.
author_facet Ivanov, A. A.
Dyakonov, M. N.
Kolosov, V. A.
Sleptsov, I. Y.
Krasilnikov, D. D.
Lischenyuk, F. F.
author_sort Ivanov, A. A.
title All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
title_short All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
title_full All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
title_fullStr All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
title_full_unstemmed All particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power eV region
title_sort all particle energy spectrum of cosmic rays in 10 to the 15th power - 10 to the 20th power ev region
publishDate 1985
url http://hdl.handle.net/2060/19850025743
op_coverage Unclassified, Unlimited, Publicly available
long_lat ENVELOPE(-63.000,-63.000,-64.300,-64.300)
geographic Rho
Yakutsk
geographic_facet Rho
Yakutsk
genre Yakutsk
genre_facet Yakutsk
op_source CASI
op_relation Document ID: 19850025743
Accession ID: 85N34056
http://hdl.handle.net/2060/19850025743
op_rights No Copyright
_version_ 1766236391420723200

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