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Электронный каталог: Prosin, V. - Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysi...
Prosin, V. - Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysi...
Книга (аналит. описание)
Автор: Prosin, V.
21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2022), Mumbai, India, 23-28 May 2022 [Electronic resource]: Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysi...
б.г.
ISBN отсутствует
Автор: Prosin, V.
21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2022), Mumbai, India, 23-28 May 2022 [Electronic resource]: Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysi...
б.г.
ISBN отсутствует
Книга (аналит. описание)
Prosin, V.
Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysical Complex / V.Prosin, A.Borodin, V.Grebenyuk, A.Grinyuk, M.Lavrova, A.Pan, Y.Sagan, L.Tkachev, [a.o.] // 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2022), Mumbai, India, 23-28 May 2022 [Electronic resource] : Online. – [S.l.] : SciPost Foundation, 2023. – P. 037. – URL: https://doi.org/10.21468/SciPostPhysProc.13.037. – Bibliogr.: 13.
The corrected dependence of the mean depth of the EAS maximum Xmax on the energy was obtained from the data of the Tunka-133 array for 7 years and the TAIGA-HiSCORE array for 2 years. The parameter ⟨ lnA ⟩, characterizing the mean mass compositon was derived from these results. The differential energy spectrum of primary cosmic rays in the energy range of 2⋅1014 – 2⋅1016 eV was reconstructed using the new parameter Q100 the Cherenkov light flux at the core distance 100 m. Change of the parameter for the energy reconstuction for the TAIGA-HiSCORE from Q200 to Q100 provides a decreasing energy threshold for the spectrum to about 200 TeV. – (SciPost Physics Proceedings, ISSN 2666-4003 ; Vol.13) .
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 347 б - Первичная компонента. Энергетический спектр и спектр масс
Спец.(статьи,препринты) = С 63 - Астрофизика$
Prosin, V.
Primary Cosmic Ray Energy Spectrum and Mean Mass Composition Using Data from the TAIGA Astrophysical Complex / V.Prosin, A.Borodin, V.Grebenyuk, A.Grinyuk, M.Lavrova, A.Pan, Y.Sagan, L.Tkachev, [a.o.] // 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2022), Mumbai, India, 23-28 May 2022 [Electronic resource] : Online. – [S.l.] : SciPost Foundation, 2023. – P. 037. – URL: https://doi.org/10.21468/SciPostPhysProc.13.037. – Bibliogr.: 13.
The corrected dependence of the mean depth of the EAS maximum Xmax on the energy was obtained from the data of the Tunka-133 array for 7 years and the TAIGA-HiSCORE array for 2 years. The parameter ⟨ lnA ⟩, characterizing the mean mass compositon was derived from these results. The differential energy spectrum of primary cosmic rays in the energy range of 2⋅1014 – 2⋅1016 eV was reconstructed using the new parameter Q100 the Cherenkov light flux at the core distance 100 m. Change of the parameter for the energy reconstuction for the TAIGA-HiSCORE from Q200 to Q100 provides a decreasing energy threshold for the spectrum to about 200 TeV. – (SciPost Physics Proceedings, ISSN 2666-4003 ; Vol.13) .
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 347 б - Первичная компонента. Энергетический спектр и спектр масс
Спец.(статьи,препринты) = С 63 - Астрофизика$