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Measurement of the Cosmic Ray Proton Spectrum from 40 GeV to 100 TeV with the DAMPE Satellite

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

Science Advances（2019）

Cited 212|Views29
Key words
Cosmic Rays
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