Energy Spectra of Cosmic-Ray Protons and Nuclei Measured in the NUCLEON Experiment Using a New Method

被引：28

作者：

Atkin, E. V. ^{[1
]}

Bulatov, V. L. ^{[2
]}

Vasiliev, O. A. ^{[3
]}

Voronin, A. G. ^{[3
]}

Gorbunov, N. V. ^{[4
]}

Grebenyuk, V. M. ^{[4
]}

Dorokhov, V. A. ^{[2
]}

Karmanov, D. E. ^{[3
]}

Kovalev, I. M. ^{[3
]}

Kudryashov, I. A. ^{[3
]}

Kurganov, A. A. ^{[3
]}

Merkin, M. M. ^{[3
]}

Panov, A. D. ^{[3
]}

Podorozhny, D. M. ^{[3
]}

Polkov, D. A. ^{[2
]}

Porokhovoi, S. Yu. ^{[4
]}

Sveshnikova, L. G. ^{[3
]}

Tkachev, L. G. ^{[4
]}

Tkachenko, A. V. ^{[4
]}

Turundaevskiy, A. N. ^{[3
]}

Filippov, S. B. ^{[2
]}

Shumikhin, V. V. ^{[1
]}

机构：

[1] Moscow Engn Phys Inst, Natl Nucl Res Inst, Moscow, Russia

[2] OOO Gorizont, Ekaterinburg, Russia

[3] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119234, Russia

[4] Joint Inst Nucl Res, Dubna 141980, Moscow Region, Russia

来源：

ASTRONOMY REPORTS | 2019年 / 63卷 / 01期

关键词：

PARTICLE ENERGY; COMPONENT; PROTOTYPE; SETUP; MODEL; BEAM;

D O I：

10.1134/S1063772919010013

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Some results of studies of cosmic rays obtained during the NUCLEON space experiment in 2015-2017 are presented. This experiment was intended for direct measurements of the energy spectra and chemical composition of cosmic rays (Z = 1-30) in the energy range 2-500 TeV. Results presented include energy spectra for various abundant nuclei measured using the new Kinematic Lightweight Energy Meter (KLEM). The primary energies are established using the spatial densities of secondary particles produced in inelastic interactions with a carbon target.

引用

页码：66 / 78

页数：13

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