| Literature DB >> 25978222 |
M Aguilar1, D Aisa2,3, B Alpat2, A Alvino2, G Ambrosi2, K Andeen4, L Arruda5, N Attig6, P Azzarello7,2, A Bachlechner8, F Barao5, A Barrau9, L Barrin10, A Bartoloni11, L Basara12,13, M Battarbee14, R Battiston13, J Bazo2, U Becker15, M Behlmann15, B Beischer8, J Berdugo1, B Bertucci2,3, G Bigongiari16,17, V Bindi18, S Bizzaglia2, M Bizzarri2,3, G Boella19,20, W de Boer4, K Bollweg21, V Bonnivard9, B Borgia11,22, S Borsini2, M J Boschini19, M Bourquin7, J Burger15, F Cadoux7, X D Cai15, M Capell15, S Caroff12, J Casaus1, V Cascioli2, G Castellini23, I Cernuda1, D Cerreta2,3, F Cervelli16, M J Chae24, Y H Chang25, A I Chen15, H Chen15, G M Cheng26, H S Chen26, L Cheng27, H Y Chou25, E Choumilov15, V Choutko15, C H Chung8, C Clark21, R Clavero28, G Coignet12, C Consolandi18, A Contin29,30, C Corti18, E Cortina Gil7, B Coste10,13, W Creus25, M Crispoltoni2,3, Z Cui27, Y M Dai31, C Delgado1, S Della Torre19, M B Demirköz32, L Derome9, S Di Falco16, L Di Masso2,3, F Dimiccoli13, C Díaz1, P von Doetinchem18, F Donnini2,3, W J Du27, M Duranti2,3, D D'Urso2, A Eline15, F J Eppling15, T Eronen14, Y Y Fan33, L Farnesini2, J Feng12, E Fiandrini2,3, A Fiasson12, E Finch34, P Fisher15, Y Galaktionov15, G Gallucci16, B García1, R García-López28, C Gargiulo10, H Gast8, I Gebauer4, M Gervasi19,20, A Ghelfi9, W Gillard25, F Giovacchini1, P Goglov15, J Gong35, C Goy12, V Grabski36, D Grandi19, M Graziani2,3, C Guandalini29,30, I Guerri16,17, K H Guo37, D Haas7, M Habiby7, S Haino25,33, K C Han38, Z H He37, M Heil15, J Hoffman25, T H Hsieh15, Z C Huang37, C Huh39, M Incagli16, M Ionica2,3, W Y Jang39, H Jinchi38, K Kanishev10,13, G N Kim39, K S Kim39, Th Kirn8, R Kossakowski12, O Kounina15, A Kounine15, V Koutsenko15, M S Krafczyk15, G La Vacca19, E Laudi2,3, G Laurenti29,30, I Lazzizzera13, A Lebedev15, H T Lee33, S C Lee33, C Leluc7, G Levi29,30, H L Li33, J Q Li35, Q Li15, Q Li15, T X Li37, W Li40, Y Li7, Z H Li26, Z Y Li33, S Lim39, C H Lin33, P Lipari11, T Lippert6, D Liu33, H Liu35, M Lolli29,30, T Lomtadze16, M J Lu13, S Q Lu33, Y S Lu26, K Luebelsmeyer8, J Z Luo35, S S Lv37, R Majka34, C Mañá1, J Marín1, T Martin21, G Martínez1, N Masi29,30, D Maurin9, A Menchaca-Rocha36, Q Meng35, D C Mo37, L Morescalchi16, P Mott21, M Müller8, J Q Ni37, N Nikonov4, F Nozzoli2, P Nunes5, A Obermeier8, A Oliva1, M Orcinha5, F Palmonari29,30, C Palomares1, M Paniccia7, A Papi2, M Pauluzzi2,3, E Pedreschi16, S Pensotti19,20, R Pereira18, N Picot-Clemente41, F Pilo16, A Piluso2,3, C Pizzolotto2, V Plyaskin15, M Pohl7, V Poireau12, E Postaci32, A Putze12, L Quadrani29,30, X M Qi37, X Qin2, Z Y Qu33, T Räihä8, P G Rancoita19, D Rapin7, J S Ricol9, I Rodríguez1, S Rosier-Lees12, A Rozhkov15, D Rozza19, R Sagdeev42, J Sandweiss34, P Saouter7, C Sbarra29,30, S Schael8, S M Schmidt6, A Schulz von Dratzig8, G Schwering8, G Scolieri2, E S Seo41, B S Shan40, Y H Shan40, J Y Shi35, X Y Shi15, Y M Shi43, T Siedenburg8, D Son39, F Spada11, F Spinella16, W Sun15, W H Sun15, M Tacconi10,19,20, C P Tang37, X W Tang26, Z C Tang26, L Tao12, D Tescaro28, Samuel C C Ting15, S M Ting15, N Tomassetti9, J Torsti14, C Türkoğlu32, T Urban21, V Vagelli4, E Valente11,22, C Vannini16, E Valtonen14, S Vaurynovich15, M Vecchi44, M Velasco1, J P Vialle12, V Vitale2, S Vitillo7, L Q Wang27, N H Wang27, Q L Wang31, R S Wang43, X Wang15, Z X Wang37, Z L Weng15, K Whitman18, J Wienkenhöver8, H Wu35, X Wu7, X Xia1, M Xie15, S Xie43, R Q Xiong35, G M Xin27, N S Xu37, W Xu26,15, Q Yan15, J Yang24, M Yang26, Q H Ye43, H Yi35, Y J Yu31, Z Q Yu26, S Zeissler4, J H Zhang35, M T Zhang37, X B Zhang37, Z Zhang37, Z M Zheng40, H L Zhuang26, V Zhukov8, A Zichichi29,30, N Zimmermann8, P Zuccon15, C Zurbach45.
Abstract
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin, acceleration, and propagation of cosmic rays. We present the detailed variation with rigidity of the flux spectral index for the first time. The spectral index progressively hardens at high rigidities.Entities:
Year: 2015 PMID： 25978222 DOI： 10.1103/PhysRevLett.114.171103
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161