用混合方法估计200-10 000 TeV能量范围内宇宙射线的光成分谱

IF 0.48 Q4 Physics and Astronomy
L. G. Sveshnikova, E. A. Okuneva, I. I. Astapov, P. A. Bezyazeekov, A. V. Blinov, A. N. Borodin, E. A. Bonvech, N. M. Budnev, A. V. Bulan, D. V. Chernov, A. Chiavassa, A. N. Dyachok, A. R. Gafarov, A. Yu. Garmash, E. O. Gress, O. A. Gress, T. I. Gress, V. M. Grebenyuk, A. A. Grinyuk, O. G. Grishin, A. L. Ivanova, A. D. Ivanova, M. A. Iliushin, N. N. Kalmykov, V. V. Kindin, S. N. Kiryuhin, R. P. Kokoulin, K. G. Kompaniets, E. E. Korosteleva, V. A. Kozhin, E. A. Kravchenko, A. P. Kryukov, L. A. Kuzmichev, A. A. Lagutin, M. V. Lavrova, Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, A. D. Lukanov, S. D. Malakhov, R. R. Mirgazov, R. D. Monkhoev, E. A. Osipova, A. L. Pakhorukov, A. Pan, A. D. Panov, L. V. Pankov, A. A. Petrukhin, I. A. Poddubnyi, D. A. Podgrudkov, E. G. Popova, E. B. Postnikov, V. V. Prosin, A. A. Pushnin, R. I. Raikin, A. Yu. Razumov, G. I. Rubtsov, E. V. Ryabov, V. S. Samoliga, I. Satyshev, A. V. Shaikovskii, A. A. Silaev, A. A. Silaev Jr., A. Yu. Sidorenkov, A. V. Skurikhin, A. V. Sokolov, V. A. Tabolenko, A. B. Tanaev, M. Yu. Ternovoy, L. G. Tkachev, N. A. Ushakov, P. A. Volchugov, N. V. Volkov, D. M. Voronin, I. I. Yashin, A.V. Zagorodnikov, D. P. Zhurov, V. N. Zirakashvili
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引用次数: 0

摘要

本文介绍了在一次宇宙射线光谱中测量能量为~ 200 - 20000的经典膝区宇宙射线的光成分(质子+氦)光谱的新结果。结果来自TAIGA实验的混合数据,其中两个(IACT + HiSCORE)设备同时记录了阵雨的切伦科夫光。利用IACT大气成像望远镜记录的图像参数,首次将流星雨与光成分分离。开发的分离光分量的方法是基于蒙特卡罗计算并经蒙特卡罗计算证实的。在获得的200-20 000 TeV能量范围内的光组分光谱中,在约3 PeV能量处观察到明显的弯曲。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method

Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method

New results on measuring the spectrum of the light component (protons + helium) of cosmic rays in the classical knee region in the primary cosmic ray spectrum at energies of ∼200–20 000 are presented. The results were obtained from hybrid data of the TAIGA experiment in which Cherenkov light of the shower is recorded simultaneously by two (IACT + HiSCORE) facilities. The showers are separated from the light component for the first time using image parameters recorded by the IACT atmospheric image telescope. The developed approach to separation of the light component is based on and confirmed by Monte Carlo calculations. In the obtained spectrum of the light component in the energy range of 200–20 000 TeV, a pronounced knee is observed at an energy of about 3 PeV.

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来源期刊
Bulletin of the Russian Academy of Sciences: Physics
Bulletin of the Russian Academy of Sciences: Physics Physics and Astronomy-Physics and Astronomy (all)
CiteScore
0.90
自引率
0.00%
发文量
251
期刊介绍: Bulletin of the Russian Academy of Sciences: Physics is an international peer reviewed journal published with the participation of the Russian Academy of Sciences. It presents full-text articles (regular,  letters  to  the editor, reviews) with the most recent results in miscellaneous fields of physics and astronomy: nuclear physics, cosmic rays, condensed matter physics, plasma physics, optics and photonics, nanotechnologies, solar and astrophysics, physical applications in material sciences, life sciences, etc. Bulletin of the Russian Academy of Sciences: Physics  focuses on the most relevant multidisciplinary topics in natural sciences, both fundamental and applied. Manuscripts can be submitted in Russian and English languages and are subject to peer review. Accepted articles are usually combined in thematic issues on certain topics according to the journal editorial policy. Authors featured in the journal represent renowned scientific laboratories and institutes from different countries, including large international collaborations. There are globally recognized researchers among the authors: Nobel laureates and recipients of other awards, and members of national academies of sciences and international scientific societies.
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