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Article ; Online: Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite.

An, Q / Asfandiyarov, R / Azzarello, P / Bernardini, P / Bi, X J / Cai, M S / Chang, J / Chen, D Y / Chen, H F / Chen, J L / Chen, W / Cui, M Y / Cui, T S / Dai, H T / D'Amone, A / De Benedittis, A / De Mitri, I / Di Santo, M / Ding, M /
Dong, T K / Dong, Y F / Dong, Z X / Donvito, G / Droz, D / Duan, J L / Duan, K K / D'Urso, D / Fan, R R / Fan, Y Z / Fang, F / Feng, C Q / Feng, L / Fusco, P / Gallo, V / Gan, F J / Gao, M / Gargano, F / Gong, K / Gong, Y Z / Guo, D Y / Guo, J H / Guo, X L / Han, S X / Hu, Y M / Huang, G S / Huang, X Y / Huang, Y Y / Ionica, M / Jiang, W / Jin, X / Kong, J / Lei, S J / Li, S / Li, W L / Li, X / Li, X Q / Li, Y / Liang, Y F / Liang, Y M / Liao, N H / Liu, C M / Liu, H / Liu, J / Liu, S B / Liu, W Q / Liu, Y / Loparco, F / Luo, C N / Ma, M / Ma, P X / Ma, S Y / Ma, T / Ma, X Y / Marsella, G / Mazziotta, M N / Mo, D / Niu, X Y / Pan, X / Peng, W X / Peng, X Y / Qiao, R / Rao, J N / Salinas, M M / Shang, G Z / Shen, W H / Shen, Z Q / Shen, Z T / Song, J X / Su, H / Su, M / Sun, Z Y / Surdo, A / Teng, X J / Tykhonov, A / Vitillo, S / Wang, C / Wang, H / Wang, H Y / Wang, J Z / Wang, L G / Wang, Q / Wang, S / Wang, X H / Wang, X L / Wang, Y F / Wang, Y P / Wang, Y Z / Wang, Z M / Wei, D M / Wei, J J / Wei, Y F / Wen, S C / Wu, D / Wu, J / Wu, L B / Wu, S S / Wu, X / Xi, K / Xia, Z Q / Xu, H T / Xu, Z H / Xu, Z L / Xu, Z Z / Xue, G F / Yang, H B / Yang, P / Yang, Y Q / Yang, Z L / Yao, H J / Yu, Y H / Yuan, Q / Yue, C / Zang, J J / Zhang, F / Zhang, J Y / Zhang, J Z / Zhang, P F / Zhang, S X / Zhang, W Z / Zhang, Y / Zhang, Y J / Zhang, Y L / Zhang, Y P / Zhang, Y Q / Zhang, Z / Zhang, Z Y / Zhao, H / Zhao, H Y / Zhao, X F / Zhou, C Y / Zhou, Y / Zhu, X / Zhu, Y / Zimmer, S

Science advances

2019  Volume 5, Issue 9, Page(s) eaax3793

Abstract: The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton ... ...

Abstract The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton fluxes with kinetic energies from 40 GeV to 100 TeV, with 2
Language English
Publishing date 2019-09-27
Publishing country United States
Document type Journal Article ; Research Support, Non-U.S. Gov't
ZDB-ID 2810933-8
ISSN 2375-2548 ; 2375-2548
ISSN (online) 2375-2548
ISSN 2375-2548
DOI 10.1126/sciadv.aax3793
Database MEDical Literature Analysis and Retrieval System OnLINE

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