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Cosmic ray energy spectrum and mass composition from 10(15) to 10(17) eV by data of the Tunka EAS Cherenkov arrayстатья
Информация о цитировании статьи получена из
Web of Science
Дата последнего поиска статьи во внешних источниках: 25 ноября 2020 г.
- Авторы: Budnev N.M., Chernov D.V., Gress O.A., Gress T.I., Korosteleva E.E., Kuzmichev L.A., Lubsandorzhiev B.K., Pankov L.V., Parfenov Yu V., Prosin V.V., Semeney Yu V., Spiering Ch, Wischnewski R.P., Yashin I.V., Inst Fundamental Res Tata
- Сборник: Proceedings of the 29th International Cosmic Ray Conference
- Серия: HE 1.1, 1.2 & 1.3
- Том: 6
- Год издания: 2005
- Место издания: Tata Institute of Fundamental Research Pune, India TATA INST FUNDAMENTAL RESEARCH, HOMI BHABHA MARG, NAVY NAGAR, COLABA, MUMBAI, MH-400005, INDIA
- Первая страница: 257
- Последняя страница: 260
- Аннотация: We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka-25. A new function to fit the Cherenkov light lateral distribution LDF at core distances from 0 to 350 m has been developed on the base of CORSIKA simulations and applied to the analysis of Tunka data. Two methods to estimate the EAS maximum position have been used. The one is based on the pulse FWHM, the other on the light LDR We present the primary energy spectrum in the energy range 10(15) - 10(17) eV. The use of the depth of the EAS maximum to determine the mean mass composition is discussed.
- Добавил в систему: Чернов Дмитрий Валентинович