ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01

作者：M. Aguilar, J. Alcaraz Maestre, J. Allaby, B. Alpat, G. Ambrosi, H. Anderhub, L. Ao, A. Arefiev, L. Arruda, P. Azzarello, M. Basile, F. Barão, G. Barreira, A. Bartoloni, R. Battiston, R. H. Becker, U. Becker, L. Bellagamba, J. Berdugo, P. Berges, B. Bertucci, A. Biland, V. Bindi, G. Boella, M. Boschini, M. Bourquin, G. Bruni, M. Buénerd, J.D. Burger, W.J. Burger, Xudong Cai, Piermarco Cannarsa, M. Capell, D. Casadei, J. Casaus, G. Castellini, I. Cernuda, Yuan-Hann Chang, H. F. Chen, Hongyao Chen, Z. G. Chen, N.A. Chernoplekov, Tzihong Chiueh, Young-Jun Choi, F. Cindolo, V. Commichau, A. Contin, E. Cortina-Gil, D. Crespo, M. Cristinziani, T.S. Dai, C. dela Guia, C. Delgado, S. Di Falco, L. Djambazov, I. DʼAntone, Zhiwen Dong, M. Duranti, J. Engelberg, F.J. Eppling, T. Eronen, P. Extermann, Judith Favier, E. Fiandrini, P.H. Fisher, G. Flügge, N. Fouque, Yu. Galaktionov, M. Gervasi, F. Giovacchini, P. Giusti, D. Grandi, O. Grimm, W. Gu, S. Haino, K. Hangarter, A. Hasan, V. Hermel, H. Hofer, W. Hungerford, M. Ionica, M. Jongmanns, K. Karlamaa, W. Karpiński, G. Kenney, D.H. Kim, G. N. Kim, K. S. Kim, T. Kirn, A. Klimentov, R. Kossakowski, A. Kounine, V. Koutsenko, M. Kraeber, G. Laborie, T. Laitinen, G. Lamanna, G. Laurenti, A. Lebedev, C. Lechanoine-Leluc, M.W. Lee, S.C. Lee, G. Lévi, Chao‐Hung Lin, H.T. Liu, G. Lu, Yao Lu, K. Lübelsmeyer, D. Luckey, W. Lustermann, C. Mañá, A. Margotti, F. Mayet, R.R. McNeil, M. Menichelli, A. Mihul, Ari Mujunen, Sonia Natale, A. Oliva, F. Palmonari, M. Paniccia, H.B. Park, W. H. Park, M. Pauluzzi, F. Pauss, R. M. Faisca Rodrigues Pereira, E. Perrin, A. Pevsner, F. Pilo, M. Pimenta, V. Plyaskin, V. Pojidaev, M. Pohl, N. Produit, L. Quadrani, P.G. Rancoita, D. Rapin, D. Ren, Z. Ren, M. Ribordy, E. Riihonen, Jouko Ritakari, S. R. Ro, U. Roeser, R. Z. Sagdeev, D. Santos, G. Sartorelli, P. Saouter, C. Sbarra, S. Schael, A. Schultz von Dratzig, G. Schwering, E. S. Seo, Jaejin Shin, E. Shoumilov, V. Shoutko, T. Siedenburg, R. Siedling, D. Son, Tao Song, F.R. Spada, F. Spinella, M. Steuer, G.S. Sun, H. Suter, Xiao Tang, Samuel C.C. Ting, S.M. Ting, Nicola Tomassetti, M. Tornikoski, J. Torsti, J. Trümper, J. Ulbricht, S. Urpo, E. Valtonen, J. Vandenhirtz, E. P. Velikhov, B. Verlaat, I. Vetlitsky, F. Vezzu, J. P. Vialle, G. Viertel, Davide Vitè, H. von Gunten, S. Waldmeier Wicki, W. Wallraff, J. Z. Wang, K. Wiik, C. Williams, S.X. Wu, P. C. Xia, Shui Xu, Z.Z. Xu, J.L. Yan, Limei Yan, C.G. Yang, J. Yang, Min Yang, S.W. Ye, H.Y. Zhang, Z. P. Zhang, D.X. Zhao, F. Zhou, Y. Zhou, G.Y. Zhu, Wei Zhu, H. L. Zhuang, A. Zichichi, B. Zimmermann, P. Zuccon · 发表于：The Astrophysical Journal · 年份：2011 · DOI：10.1088/0004-637x/736/2/105 · 被引用次数：64 · 研究领域：Solar and Space Plasma Dynamics、Dark Matter and Cosmic Phenomena、Astro and Planetary Science

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.