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dc.contributor.authorBecker, R.
dc.contributor.authorBecker, Ulrich J.
dc.contributor.authorBerges, P.
dc.contributor.authorBurger, Joseph D.
dc.contributor.authorCai, Xudong
dc.contributor.authorCapell, Michael H.
dc.contributor.authorDai, T. S.
dc.contributor.authorEppling, Frederic J.
dc.contributor.authorFisher, Peter H.
dc.contributor.authorKlimentov, A.
dc.contributor.authorKounine, Andrei
dc.contributor.authorKoutsenko, Vladimir
dc.contributor.authorLebedev, Alexei
dc.contributor.authorLuckey, P. David, Jr.
dc.contributor.authorShoutko, V.
dc.contributor.authorSiedenburg, T.
dc.contributor.authorSteuer, M.
dc.contributor.authorTing, Samuel C. C.
dc.contributor.authorWu, S. X.
dc.contributor.authorXu, S.
dc.contributor.authorZhou, F.
dc.contributor.authorWu. S. X.
dc.date.accessioned2014-09-05T18:02:48Z
dc.date.available2014-09-05T18:02:48Z
dc.date.issued2011-07
dc.date.submitted2010-12
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1721.1/89210
dc.description.abstractThe 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 [superscript 2]H/[superscript 4]He, [superscript 3]He/[superscript 4]He, [superscript 6]Li/[superscript 7]Li, [superscript 7]Be/([superscript 9]Be+[superscript 10]Be), and [superscript 10]B/[superscript 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.en_US
dc.description.sponsorshipUnited States. Dept. of Energyen_US
dc.description.sponsorshipMassachusetts Institute of Technologyen_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637x/736/2/105en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01en_US
dc.typeArticleen_US
dc.identifier.citationAguilar, M., J. Alcaraz, J. Allaby, B. Alpat, G. Ambrosi, H. Anderhub, L. Ao, et al. “ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01.” The Astrophysical Journal 736, no. 2 (August 1, 2011): 105.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.mitauthorBecker, R.en_US
dc.contributor.mitauthorBecker, Ulrich J.en_US
dc.contributor.mitauthorBerges, P.en_US
dc.contributor.mitauthorBurger, Joseph D.en_US
dc.contributor.mitauthorCai, Xudongen_US
dc.contributor.mitauthorCapell, Michael H.en_US
dc.contributor.mitauthorDai, T. S.en_US
dc.contributor.mitauthorEppling, Frederic J.en_US
dc.contributor.mitauthorFisher, Peter H.en_US
dc.contributor.mitauthorKlimentov, A.en_US
dc.contributor.mitauthorKounine, Andreien_US
dc.contributor.mitauthorKoutsenko, Vladimiren_US
dc.contributor.mitauthorLebedev, Alexeien_US
dc.contributor.mitauthorLuckey, P. David, Jr.en_US
dc.contributor.mitauthorShoutko, V.en_US
dc.contributor.mitauthorSiedenburg, T.en_US
dc.contributor.mitauthorSteuer, M.en_US
dc.contributor.mitauthorTing, Samuel C. C.en_US
dc.contributor.mitauthorWu. S. X.en_US
dc.contributor.mitauthorXu, S.en_US
dc.contributor.mitauthorZhou, F.en_US
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsAguilar, 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.; Buénerd, M.; Burger, J. D.; Burger, W. J.; Cai, X. D.; Cannarsa, P.; Capell, M.; Casadei, D.; Casaus, J.; Castellini, G.; Cernuda, I.; Chang, Y. H.; Chen, H. F.; Chen, H. S.; Chen, Z. G.; Chernoplekov, N. A.; Chiueh, T. H.; Choi, Y. Y.; Cindolo, F.; Commichau, V.; Contin, A.; Cortina-Gil, E.; Crespo, D.; Cristinziani, M.; Dai, T. S.; dela Guia, C.; Delgado, C.; Di Falco, S.; Djambazov, L.; D’Antone, I.; Dong, Z. R.; Duranti, M.; Engelberg, J.; Eppling, F. J.; Eronen, T.; Extermann, P.; Favier, J.; Fiandrini, E.; Fisher, P. H.; Flügge, G.; Fouque, N.; Galaktionov, Y.; Gervasi, M.; Giovacchini, F.; Giusti, P.; Grandi, D.; Grimm, O.; Gu, W. Q.; Haino, S.; Hangarter, K.; Hasan, A.; Hermel, V.; Hofer, H.; Hungerford, W.; Ionica, M.; Jongmanns, M.; Karlamaa, K.; Karpinski, W.; Kenney, G.; Kim, D. H.; Kim, G. N.; Kim, K. S.; 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, M. W.; Lee, S. C.; Levi, G.; Lin, C. H.; Liu, H. T.; Lu, G.; Lu, Y. S.; Lübelsmeyer, K.; Luckey, D.; Lustermann, W.; Maña, C.; Margotti, A.; Mayet, F.; McNeil, R. R.; Menichelli, M.; Mihul, A.; Mujunen, A.; Natale, S.; Oliva, A.; Palmonari, F.; Paniccia, M.; Park, H. B.; Park, W. H.; 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, P. G.; 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, A. Schultz; Schwering, G.; Seo, E. S.; Shin, J. W.; Shoumilov, E.; Shoutko, V.; Siedenburg, T.; Siedling, R.; Son, D.; Song, T.; Spada, F. R.; Spinella, F.; Steuer, M.; Sun, G. S.; Suter, H.; Tang, X. W.; Ting, Samuel C. C.; Ting, S. M.; Tomassetti, N.; Tornikoski, M.; Torsti, J.; Trümper, J.; Ulbricht, J.; Urpo, S.; Valtonen, E.; Vandenhirtz, J.; Velikhov, E.; Verlaat, B.; Vetlitsky, I.; Vezzu, F.; Vialle, J. P.; Viertel, G.; Vité, D.; Von Gunten, H.; Wicki, S. Waldmeier; Wallraff, W.; Wang, J. Z.; Wiik, K.; Williams, C.; Wu, S. X.; Xia, P. C.; Xu, S.; Xu, Z. Z.; Yan, J. L.; Yan, L. G.; Yang, C. G.; Yang, J.; Yang, M.; Ye, S. W.; Zhang, H. Y.; Zhang, Z. P.; Zhao, D. X.; Zhou, F.; Zhou, Y.; Zhu, G. Y.; Zhu, W. Z.; Zhuang, H. L.; Zichichi, A.; Zimmermann, B.; Zuccon, P.en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-4436-6077
dc.identifier.orcidhttps://orcid.org/0000-0001-7831-7460
dc.identifier.orcidhttps://orcid.org/0000-0002-0450-7007
dc.identifier.orcidhttps://orcid.org/0000-0002-5006-6847
dc.identifier.orcidhttps://orcid.org/0000-0003-3513-8408
dc.identifier.orcidhttps://orcid.org/0000-0002-8667-5660
dc.identifier.orcidhttps://orcid.org/0000-0002-0236-7274
dc.identifier.orcidhttps://orcid.org/0000-0002-7172-9021
dspace.mitauthor.errortrue
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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