Cosmic Protons

J Alcaraz,B Alpat,G Ambrosi,H Anderhub,L Ao,A Arefiev,P Azzarello,E Babucci,L Baldini,M Basile,D Barancourt,F Barao,G Barbier,G Barreira,R Battiston,R Becker,U Becker,L Bellagamba,P Bene,J Berdugo,P Berges,B Bertucci,A Biland,S Bizzaglia,S Blasko,G Boella,M Boschini,M Bourquin,L Brocco,G Bruni,M Buenerd,JD Burger,WJ Burger,XD Cai,C Camps, P Cannarsa,M Capell,D Casadei,J Casaus,G Castellini,C Cecchi,YH Chang,HF Chen,HS Chen,ZG Chen,NA Chernoplekov,TH Chiueh,YL Chuang,F Cindolo,V Commichau,A Contin,P Crespo, M Cristinziani,JP da Cunha,TS Dai,JD Deus,N Dinu,L Djambazov,I D'Antone,ZR Dong,P Emonet,J Engelberg,FJ Eppling,T Eronen,G Esposito,P Extermann,J Favier,E Fiandrini,PH Fisher,G Fluegge,N Fouque,Y Galaktionov,M Gervasi,P Giusti,D Grandi,O Grimm,WQ Gu,K Hangarter,A Hasan,V Hermel,H Hofer,MA Huang,W Hungerford,M Ionica,R Ionica,M Jongmanns,K Karlamaa,W Karpinski,G Kenney, J Kenny,W Kim, A Klimentov,R Kossakowski,V Koutsenko,M Kraeber,G Laborie,T Laitinen,G Lamanna,G Laurenti,A Lebedev,SC Lee,G Levi,P Levtchenko,CL Liu,HT Liu,I Lopes,G Lu,YS Lu,K Lubelsmeyer,D Luckey,W Lustermann,C Mana,A Margotti,F Mayet,RR McNeil,B Meillon,M Menichelli,A Mihul,A Mourao,A Mujunen,F Palmonari,A Papi,IH Park,M Pauluzzi,F Pauss,E Perrin,A Pesci,A Pevsner,M Pimenta,V Plyaskin,V Pojidaev,M Pohl,V Postolache,N Produit,PG Rancoita,D Rapin,F Raupach,D Ren,Z Ren,M Ribordy,JP Richeux,E Riihonen,J Ritakari,U Roeser,C Roissin,R Sagdeev,G Sartorelli,AS von Dratzig,G Schwering,G Scolieri,ES Seo,V Shoutko,E Shoumilov,R Siedling,D Son, T Song,M Steuer,GS Sun,H Suter, XW Tang,SCC Ting,SM Ting,M Tornikoski,J Torsti,J Trumper,J Ulbricht,S Urpo,I Usoskin,E Valtonen,J Vandenhirtz,F Velcea,E Velikhov,B Verlaat,I Vetlitsky,F Vezzu,JP Vialle,G Viertel,D Vite,H Von Gunten,SW Wicki,W Wallraff,BC Wang, JZ Wang, YN Wang,K Wiik, C Williams,SX Wu,PC Xia,JL Yan,LG Yan,CG Yang,M Yang, SW Ye,P Yeh, ZZ Xu,HY Zhang,ZP Zhang,DX Zhao,GY Zhu,WZ Zhu,HL Zhuang,A Zichichi,B Zimmermann

Physics Letters B（2000）

CIEMAT

被引用308|浏览123

摘要

The primary proton spectrum in the kinetic energy range 0.2 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle Right STS-91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented. (C) 2000 Elsevier Science B.V. All rights reserved.

更多

查看译文

关键词

Environmental Magnetism

上传PDF