Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere

Standard

Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere. / TAIGA Collaboration.

в: Physics of Atomic Nuclei, Том 81, № 9, 01.12.2018, стр. 1294-1300.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

TAIGA Collaboration 2018, 'Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere', Physics of Atomic Nuclei, Том. 81, № 9, стр. 1294-1300. https://doi.org/10.1134/S1063778818090090

APA

TAIGA Collaboration (2018). Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere. Physics of Atomic Nuclei, 81(9), 1294-1300. https://doi.org/10.1134/S1063778818090090

Vancouver

TAIGA Collaboration. Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere. Physics of Atomic Nuclei. 2018 дек. 1;81(9):1294-1300. doi: 10.1134/S1063778818090090

Author

TAIGA Collaboration. / Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere. в: Physics of Atomic Nuclei. 2018 ; Том 81, № 9. стр. 1294-1300.

BibTeX

@article{a205a4cd26614ded9937adb417bd037b,

title = "Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere",

abstract = "A new knee-like approximation of the lateral distribution function (LDF) of EAS Cherenkov light in the 30–3000 TeV energy range was proposed and tested with simulated showers in our earlier studies. This approximation fits the LDFs of individual showers accurately for all types of primary particles gamma-rays, protons, and nuclei) and is suitable for reconstructing the shower core, determining the energy, and separating gamma-induced showers from hadron-induced ones. In the present study, the knee-like fitting function is used to determine the parameters of real showers detected by TAIGA-HiSCORE. It is demonstrated that this approximation characterizes properly all types of individual LDFs of experimental events in the 300–1000 TeV range. The accuracy of fit is governed by fluctuations intrinsic to the process of measurement of the Cherenkov photon density. The probability density function of these fluctuations was reconstructed and introduced into simulations. Certain useful methodical applications of the knee-like approximation are con-sidered, and the possibility of shower sorting into nuclei groups is examined. The extensive statistical coverage and detailed LDF measurement data of HiSCORE have provided the first opportunity to examine in depth the LDF of Cherenkov radiation in the 300–1000 TeV range.",

keywords = "chemical composition, Cherenkov light, cosmic rays, EAS, primary nuclei",

author = "{the TAIGA Collaboration} and Elshoukrofy, {A. Sh M.} and Postnikov, {E. B.} and Astapov, {I. I.} and Bezyazeekov, {P. A.} and V. Boreyko and Borodin, {A. N.} and Budnev, {N. M.} and R. Wischnewski and Garmash, {A. Y.} and Gafarov, {A. R.} and Gorbunov, {N. V.} and Grebenyuk, {V. M.} and Gress, {O. A.} and Gress, {T. I.} and Grinyuk, {A. A.} and Grishin, {O. G.} and Dyachok, {A. N.} and Zagorodnikov, {A. V.} and Zurbanov, {V. L.} and Ivanova, {A. L.} and Kazarina, {Y. A.} and Kalmykov, {N. N.} and Karpov, {N. I.} and Kindin, {V. V.} and Kirilenko, {P. S.} and Kiryuhin, {S. N.} and Kozhin, {V. A.} and Kokoulin, {R. P.} and Kompaniets, {K. G.} and Korosteleva, {E. E.} and Kravchenko, {E. A.} and Kuzmichev, {L. A.} and M. Kunnas and A. Chiavassa and Lagutin, {A. A.} and Lenok, {V. V.} and Lubsandorzhiev, {B. K.} and Lubsandorzhiev, {N. B.} and Mirgazov, {R. R.} and R. Mirzoyan and Monkhoev, {R. D.} and Motaweh, {H. A.} and R. Nachtigall and Osipova, {E. A.} and Panasyuk, {M. I.} and Pankov, {L. V.} and Pakhorukov, {A. L.} and Petrukhin, {A. A.} and Poleschuk, {V. A.} and Sokolov, {A. V.}",

note = "Publisher Copyright: {\textcopyright} 2018, Pleiades Publishing, Ltd.",

year = "2018",

month = dec,

day = "1",

doi = "10.1134/S1063778818090090",

language = "English",

volume = "81",

pages = "1294--1300",

journal = "Physics of Atomic Nuclei",

issn = "1063-7788",

publisher = "Maik Nauka-Interperiodica Publishing",

number = "9",

}

RIS

TY - JOUR

T1 - Application of New Approximations of the Lateral Distribution of EAS Cherenkov Light in the Atmosphere

AU - the TAIGA Collaboration

AU - Elshoukrofy, A. Sh M.

AU - Postnikov, E. B.

AU - Astapov, I. I.

AU - Bezyazeekov, P. A.

AU - Boreyko, V.

AU - Borodin, A. N.

AU - Budnev, N. M.

AU - Wischnewski, R.

AU - Garmash, A. Y.

AU - Gafarov, A. R.

AU - Gorbunov, N. V.

AU - Grebenyuk, V. M.

AU - Gress, O. A.

AU - Gress, T. I.

AU - Grinyuk, A. A.

AU - Grishin, O. G.

AU - Dyachok, A. N.

AU - Zagorodnikov, A. V.

AU - Zurbanov, V. L.

AU - Ivanova, A. L.

AU - Kazarina, Y. A.

AU - Kalmykov, N. N.

AU - Karpov, N. I.

AU - Kindin, V. V.

AU - Kirilenko, P. S.

AU - Kiryuhin, S. N.

AU - Kozhin, V. A.

AU - Kokoulin, R. P.

AU - Kompaniets, K. G.

AU - Korosteleva, E. E.

AU - Kravchenko, E. A.

AU - Kuzmichev, L. A.

AU - Kunnas, M.

AU - Chiavassa, A.

AU - Lagutin, A. A.

AU - Lenok, V. V.

AU - Lubsandorzhiev, B. K.

AU - Lubsandorzhiev, N. B.

AU - Mirgazov, R. R.

AU - Mirzoyan, R.

AU - Monkhoev, R. D.

AU - Motaweh, H. A.

AU - Nachtigall, R.

AU - Osipova, E. A.

AU - Panasyuk, M. I.

AU - Pankov, L. V.

AU - Pakhorukov, A. L.

AU - Petrukhin, A. A.

AU - Poleschuk, V. A.

AU - Sokolov, A. V.

PY - 2018/12/1

Y1 - 2018/12/1

N2 - A new knee-like approximation of the lateral distribution function (LDF) of EAS Cherenkov light in the 30–3000 TeV energy range was proposed and tested with simulated showers in our earlier studies. This approximation fits the LDFs of individual showers accurately for all types of primary particles gamma-rays, protons, and nuclei) and is suitable for reconstructing the shower core, determining the energy, and separating gamma-induced showers from hadron-induced ones. In the present study, the knee-like fitting function is used to determine the parameters of real showers detected by TAIGA-HiSCORE. It is demonstrated that this approximation characterizes properly all types of individual LDFs of experimental events in the 300–1000 TeV range. The accuracy of fit is governed by fluctuations intrinsic to the process of measurement of the Cherenkov photon density. The probability density function of these fluctuations was reconstructed and introduced into simulations. Certain useful methodical applications of the knee-like approximation are con-sidered, and the possibility of shower sorting into nuclei groups is examined. The extensive statistical coverage and detailed LDF measurement data of HiSCORE have provided the first opportunity to examine in depth the LDF of Cherenkov radiation in the 300–1000 TeV range.

AB - A new knee-like approximation of the lateral distribution function (LDF) of EAS Cherenkov light in the 30–3000 TeV energy range was proposed and tested with simulated showers in our earlier studies. This approximation fits the LDFs of individual showers accurately for all types of primary particles gamma-rays, protons, and nuclei) and is suitable for reconstructing the shower core, determining the energy, and separating gamma-induced showers from hadron-induced ones. In the present study, the knee-like fitting function is used to determine the parameters of real showers detected by TAIGA-HiSCORE. It is demonstrated that this approximation characterizes properly all types of individual LDFs of experimental events in the 300–1000 TeV range. The accuracy of fit is governed by fluctuations intrinsic to the process of measurement of the Cherenkov photon density. The probability density function of these fluctuations was reconstructed and introduced into simulations. Certain useful methodical applications of the knee-like approximation are con-sidered, and the possibility of shower sorting into nuclei groups is examined. The extensive statistical coverage and detailed LDF measurement data of HiSCORE have provided the first opportunity to examine in depth the LDF of Cherenkov radiation in the 300–1000 TeV range.

KW - chemical composition

KW - Cherenkov light

KW - cosmic rays

KW - EAS

KW - primary nuclei

UR - http://www.scopus.com/inward/record.url?scp=85062590988&partnerID=8YFLogxK

U2 - 10.1134/S1063778818090090

DO - 10.1134/S1063778818090090

M3 - Article

AN - SCOPUS:85062590988

VL - 81

SP - 1294

EP - 1300

JO - Physics of Atomic Nuclei

JF - Physics of Atomic Nuclei

SN - 1063-7788

IS - 9

ER -

ID: 18787653