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    题名: ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01
    作者: Aguilar,M;Alcaraz,J;Allaby,J;Alpat,B;Ambrosi,G;Anderhub,H;Ao,L;Arefiev,A;Arruda,L;Azzarello,P;Basile,M;Barao,F;Barreira,G;Bartoloni,A;Battiston,R;Becker,R;Becker,U;Bellagamba,L;Berdugo,J;Berges,P;Bertucci,B;Biland,A;Bindi,V;Boella,G;Boschini,M;Bourquin,M;Bruni,G;Buenerd,M;Burger,JD;Burger,WJ;Cai,XD;Cannarsa,P;Capell,M;Casadei,D;Casaus,J;Castellini,G;Cernuda,I;Chang,YH;Chen,HF;Chen,HS;Chen,ZG;Chernoplekov,NA;Chiueh,TH;Choi,YY;Cindolo,F;Commichau,V;Contin,A;Cortina-Gil,E;Crespo,D;Cristinziani,M;Dai,TS;Dela Guia,C;Delgado,C;Di Falco,S;Djambazov,L;D'Antone,I;Dong,ZR;Duranti,M;Engelberg,J;Eppling,FJ;Eronen,T;Extermann,P;Favier,J;Fiandrini,E;Fisher,PH;Flugge,G;Fouque,N;Galaktionov,Y;Gervasi,M;Giovacchini,F;Giusti,P;Grandi,D;Grimm,O;Gu,WQ;Haino,S;Hangarter,K;Hasan,A;Hermel,V;Hofer,H;Hungerford,W;Ionica,M;Jongmanns,M;Karlamaa,K;Karpinski,W;Kenney,G;Kim,DH;Kim,GN;Kim,KS;Kirn,T;Klimentov,A;Kossakowski,R;Kounine,A;Koutsenko,V;Kraeber,M;Laborie,G;Laitinen,T;Lamanna,G;Laurenti,G;Lebedev,A;Lechanoine-Leluc,C;Lee,MW;Lee,SC;Levi,G;Lin,CH;Liu,HT;Lu,G;Lu,YS;Lubelsmeyer,K;Luckey,D;Lustermann,W;Mana,C;Margotti,A;Mayet,F;McNeil,RR;Menichelli,M;Mihul,A;Mujunen,A;Natale,S;Oliva,A;Palmonari,F;Paniccia,M;Park,HB;Park,WH;Pauluzzi,M;Pauss,F;Pereira,R;Perrin,E;Pevsner,A;Pilo,F;Pimenta,M;Plyaskin,V;Pojidaev,V;Pohl,M;Produit,N;Quadrani,L;Rancoita,PG;Rapin,D;Ren,D;Ren,Z;Ribordy,M;Riihonen,E;Ritakari,J;Ro,S;Roeser,U;Sagdeev,R;Santos,D;Sartorelli,G;Saouter,P;Sbarra,C;Schael,S;von Dratzig,AS;Schwering,G;Seo,ES;Shin,JW;Shoumilov,E;Shoutko,V;Siedenburg,T;Siedling,R;Son,D;Song,T;Spada,FR;Spinella,F;Steuer,M;Sun,GS;Suter,H;Tang,XW;Ting,SCC;Ting,SM;Tomassetti,N;Tornikoski,M;Torsti,J;Trumper,J;Ulbricht,J;Urpo,S;Valtonen,E;Vandenhirtz,J;Velikhov,E;Verlaat,B;Vetlitsky,I;Vezzu,F;Vialle,JP;Viertel,G;Vite,D;Von Gunten,H;Wicki,SW;Wallraff,W;Wang,JZ;Wiik,K;Williams,C;Wu,SX;Xia,PC;Xu,S;Xu,ZZ;Yan,JL;Yan,LG;Yang,CG;Yang,J;Yang,M;Ye,SW;Zhang,HY;Zhang,ZP;Zhao,DX;Zhou,F;Zhou,Y;Zhu,GY;Zhu,WZ;Zhuang,HL;Zichichi,A;Zimmermann,B;Zuccon,P
    贡献者: 物理學系
    关键词: RELATIVE ABUNDANCE;ENERGY-SPECTRA;BE-10;PROPAGATION;HELIUM;GALAXY;HE-3;AGE;NUCLEON(-1);RATIO
    日期: 2011
    上传时间: 2012-06-11 10:49:23 (UTC+8)
    出版者: 國立中央大學
    摘要: The variety of isotopes in cosmic rays allows us to study different aspects of the processes that cosmic rays undergo between the time they are produced and the time of their arrival in the heliosphere. In this paper, we present measurements of the isotopic ratios (2)H/(4)He, (3)He/(4)He, (6)Li/(7)Li, (7)Be/((9)Be+(10)Be), and (10)B/(11)B in the range 0.2-1.4 GeV of kinetic energy per nucleon. The measurements are based on the data collected by the Alpha Magnetic Spectrometer, AMS-01, during the STS-91 flight in 1998 June.
    關聯: ASTROPHYSICAL JOURNAL
    显示于类别:[物理學系] 期刊論文

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