ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01
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 [superscript 2]H/[superscript 4]He,...
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| Language: | en_US |
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IOP Publishing
2014
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| Online Access: | http://hdl.handle.net/1721.1/89210 https://orcid.org/0000-0002-4436-6077 https://orcid.org/0000-0001-7831-7460 https://orcid.org/0000-0002-0450-7007 https://orcid.org/0000-0002-5006-6847 https://orcid.org/0000-0003-3513-8408 https://orcid.org/0000-0002-8667-5660 https://orcid.org/0000-0002-0236-7274 https://orcid.org/0000-0002-7172-9021 |
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| author | Becker, R. Becker, Ulrich J. Berges, P. Burger, Joseph D. Cai, Xudong Capell, Michael H. Dai, T. S. Eppling, Frederic J. Fisher, Peter H. Klimentov, A. Kounine, Andrei Koutsenko, Vladimir Lebedev, Alexei Luckey, P. David, Jr. Shoutko, V. Siedenburg, T. Steuer, M. Ting, Samuel C. C. Wu, S. X. Xu, S. Zhou, F. Wu. S. X. |
| author2 | Massachusetts Institute of Technology. Department of Physics |
| author_facet | Massachusetts Institute of Technology. Department of Physics Becker, R. Becker, Ulrich J. Berges, P. Burger, Joseph D. Cai, Xudong Capell, Michael H. Dai, T. S. Eppling, Frederic J. Fisher, Peter H. Klimentov, A. Kounine, Andrei Koutsenko, Vladimir Lebedev, Alexei Luckey, P. David, Jr. Shoutko, V. Siedenburg, T. Steuer, M. Ting, Samuel C. C. Wu, S. X. Xu, S. Zhou, F. Wu. S. X. |
| author_sort | Becker, R. |
| collection | MIT |
| description | 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 [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. |
| first_indexed | 2024-09-23T14:07:08Z |
| format | Article |
| id | mit-1721.1/89210 |
| institution | Massachusetts Institute of Technology |
| language | en_US |
| last_indexed | 2024-09-23T14:07:08Z |
| publishDate | 2014 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | mit-1721.1/892102022-10-01T19:18:10Z ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 Becker, R. Becker, Ulrich J. Berges, P. Burger, Joseph D. Cai, Xudong Capell, Michael H. Dai, T. S. Eppling, Frederic J. Fisher, Peter H. Klimentov, A. Kounine, Andrei Koutsenko, Vladimir Lebedev, Alexei Luckey, P. David, Jr. Shoutko, V. Siedenburg, T. Steuer, M. Ting, Samuel C. C. Wu, S. X. Xu, S. Zhou, F. Wu. S. X. Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Laboratory for Nuclear Science Becker, R. Becker, Ulrich J. Berges, P. Burger, Joseph D. Cai, Xudong Capell, Michael H. Dai, T. S. Eppling, Frederic J. Fisher, Peter H. Klimentov, A. Kounine, Andrei Koutsenko, Vladimir Lebedev, Alexei Luckey, P. David, Jr. Shoutko, V. Siedenburg, T. Steuer, M. Ting, Samuel C. C. Wu. S. X. Xu, S. Zhou, F. 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 [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. United States. Dept. of Energy Massachusetts Institute of Technology 2014-09-05T18:02:48Z 2014-09-05T18:02:48Z 2011-07 2010-12 Article http://purl.org/eprint/type/JournalArticle 0004-637X 1538-4357 http://hdl.handle.net/1721.1/89210 Aguilar, 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. https://orcid.org/0000-0002-4436-6077 https://orcid.org/0000-0001-7831-7460 https://orcid.org/0000-0002-0450-7007 https://orcid.org/0000-0002-5006-6847 https://orcid.org/0000-0003-3513-8408 https://orcid.org/0000-0002-8667-5660 https://orcid.org/0000-0002-0236-7274 https://orcid.org/0000-0002-7172-9021 en_US http://dx.doi.org/10.1088/0004-637x/736/2/105 The Astrophysical Journal Creative Commons Attribution-Noncommercial-Share Alike http://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf IOP Publishing arXiv |
| spellingShingle | Becker, R. Becker, Ulrich J. Berges, P. Burger, Joseph D. Cai, Xudong Capell, Michael H. Dai, T. S. Eppling, Frederic J. Fisher, Peter H. Klimentov, A. Kounine, Andrei Koutsenko, Vladimir Lebedev, Alexei Luckey, P. David, Jr. Shoutko, V. Siedenburg, T. Steuer, M. Ting, Samuel C. C. Wu, S. X. Xu, S. Zhou, F. Wu. S. X. ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title | ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title_full | ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title_fullStr | ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title_full_unstemmed | ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title_short | ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01 |
| title_sort | isotopic composition of light nuclei in cosmic rays results from ams 01 |
| url | http://hdl.handle.net/1721.1/89210 https://orcid.org/0000-0002-4436-6077 https://orcid.org/0000-0001-7831-7460 https://orcid.org/0000-0002-0450-7007 https://orcid.org/0000-0002-5006-6847 https://orcid.org/0000-0003-3513-8408 https://orcid.org/0000-0002-8667-5660 https://orcid.org/0000-0002-0236-7274 https://orcid.org/0000-0002-7172-9021 |
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