Cosmic protons
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 flight STS–91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented.
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| Veröffentlicht in: | Physics letters. B 2000-09, Vol.490 (1), p.27-35 |
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| container_title | Physics letters. B |
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| creator | Ambrosi, G. Ao, L. Arefiev, A. Azzarello, P. Basile, M. Barancourt, D. Barao, F. Becker, R. Becker, U. Berdugo, J. Berges, P. Bertucci, B. Blasko, S. Bourquin, M. Brocco, L. Buenerd, M. Burger, J.D. Burger, W.J. Cai, X.D. Capell, M. Cecchi, C. Chang, Y.H. Chen, Z.G. Cindolo, F. Commichau, V. Crespo, P. Cristinziani, M. Deus, J.D. Djambazov, L. D'Antone, I. Emonet, P. Engelberg, J. Eppling, F.J. Eronen, T. Esposito, G. Fiandrini, E. Fisher, P.H. Gervasi, M. Gu, W.Q. Hangarter, K. Hasan, A. Hermel, V. Huang, M.A. Ionica, M. Ionica, R. Jongmanns, M. Karlamaa, K. Kim, W. Kossakowski, R. Kraeber, M. Laborie, G. Lee, S.C. Levtchenko, P. Liu, C.L. Liu, H.T. Lu, G. Lu, Y.S. Luckey, D. Lustermann, W. Palmonari, F. Pesci, A. Pevsner, A. Pimenta, M. Plyaskin, V. Pojidaev, V. Rapin, D. Ren, Z. Ribordy, M. Roissin, C. Sagdeev, R. Schwering, G. Scolieri, G. Seo, E.S. Song, T. Ting, Samuel C.C. Tornikoski, M. Torsti, J. Trümper, J. Usoskin, I. Vandenhirtz, J. Velcea, F. Verlaat, B. Vezzu, F. Von Gunten, H. Waldmeier Wicki, S. Wang, J.Z. Wang, Y.H. Wiik, K. Wu, S.X. Yan, J.L. Yan, L.G. Yang, C.G. Yang, M. Ye, S.W. Xu, Z.Z. Zhang, Z.P. Zhao, D.X. Zhu, G.Y. Zhuang, H.L. Zimmermann, B. |
| description | 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 flight STS–91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented. |
| doi_str_mv | 10.1016/S0370-2693(00)00970-9 |
| format | Article |
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protons</title><title>Physics letters. B</title><description>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 flight STS–91 at an altitude of 380 km. 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B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0001-9995-4792</orcidid><orcidid>https://orcid.org/0000-0003-4365-3282</orcidid><orcidid>https://orcid.org/0000-0003-3842-8531</orcidid><orcidid>https://orcid.org/0000-0001-5760-8939</orcidid><orcidid>https://orcid.org/0000-0002-1288-833X</orcidid><orcidid>https://orcid.org/0000-0003-1249-6026</orcidid></search><sort><creationdate>20000928</creationdate><title>Cosmic protons</title><author>Ambrosi, G. ; Ao, L. ; Arefiev, A. ; Azzarello, P. ; Basile, M. ; Barancourt, D. ; Barao, F. ; Becker, R. ; Becker, U. ; Berdugo, J. ; Berges, P. ; Bertucci, B. ; Blasko, S. ; Bourquin, M. ; Brocco, L. ; Buenerd, M. ; Burger, J.D. ; Burger, W.J. ; Cai, X.D. ; Capell, M. ; Cecchi, C. ; Chang, Y.H. ; Chen, Z.G. ; Cindolo, F. ; Commichau, V. ; Crespo, P. ; Cristinziani, M. ; Deus, J.D. ; Djambazov, L. ; D'Antone, I. ; Emonet, P. ; Engelberg, J. ; Eppling, F.J. ; Eronen, T. ; Esposito, G. ; Fiandrini, E. ; Fisher, P.H. ; Gervasi, M. ; Gu, W.Q. ; Hangarter, K. ; Hasan, A. ; Hermel, V. ; Huang, M.A. ; Ionica, M. ; Ionica, R. ; Jongmanns, M. ; Karlamaa, K. ; Kim, W. ; Kossakowski, R. ; Kraeber, M. ; Laborie, G. ; Lee, S.C. ; Levtchenko, P. ; Liu, C.L. ; Liu, H.T. ; Lu, G. ; Lu, Y.S. ; Luckey, D. ; Lustermann, W. ; Palmonari, F. ; Pesci, A. ; Pevsner, A. ; Pimenta, M. ; Plyaskin, V. ; Pojidaev, V. ; Rapin, D. ; Ren, Z. ; Ribordy, M. ; Roissin, C. ; Sagdeev, R. ; Schwering, G. ; Scolieri, G. ; Seo, E.S. ; Song, T. ; Ting, Samuel C.C. ; Tornikoski, M. ; Torsti, J. ; Trümper, J. ; Usoskin, I. ; Vandenhirtz, J. ; Velcea, F. ; Verlaat, B. ; Vezzu, F. ; Von Gunten, H. ; Waldmeier Wicki, S. ; Wang, J.Z. ; Wang, Y.H. ; Wiik, K. ; Wu, S.X. ; Yan, J.L. ; Yan, L.G. ; Yang, C.G. ; Yang, M. ; Ye, S.W. ; Xu, Z.Z. ; Zhang, Z.P. ; Zhao, D.X. ; Zhu, G.Y. ; Zhuang, H.L. ; Zimmermann, B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c390t-c017f5a9e42be7c4a0bd79b7bc2e30638ca6eaf8f989f4c04b0e58556ff2c96e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Astrophysics</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ambrosi, G.</creatorcontrib><creatorcontrib>Ao, L.</creatorcontrib><creatorcontrib>Arefiev, A.</creatorcontrib><creatorcontrib>Azzarello, P.</creatorcontrib><creatorcontrib>Basile, M.</creatorcontrib><creatorcontrib>Barancourt, D.</creatorcontrib><creatorcontrib>Barao, F.</creatorcontrib><creatorcontrib>Becker, R.</creatorcontrib><creatorcontrib>Becker, U.</creatorcontrib><creatorcontrib>Berdugo, J.</creatorcontrib><creatorcontrib>Berges, P.</creatorcontrib><creatorcontrib>Bertucci, 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T.</creatorcontrib><creatorcontrib>Esposito, G.</creatorcontrib><creatorcontrib>Fiandrini, E.</creatorcontrib><creatorcontrib>Fisher, P.H.</creatorcontrib><creatorcontrib>Gervasi, M.</creatorcontrib><creatorcontrib>Gu, W.Q.</creatorcontrib><creatorcontrib>Hangarter, K.</creatorcontrib><creatorcontrib>Hasan, A.</creatorcontrib><creatorcontrib>Hermel, V.</creatorcontrib><creatorcontrib>Huang, M.A.</creatorcontrib><creatorcontrib>Ionica, M.</creatorcontrib><creatorcontrib>Ionica, R.</creatorcontrib><creatorcontrib>Jongmanns, M.</creatorcontrib><creatorcontrib>Karlamaa, K.</creatorcontrib><creatorcontrib>Kim, W.</creatorcontrib><creatorcontrib>Kossakowski, R.</creatorcontrib><creatorcontrib>Kraeber, M.</creatorcontrib><creatorcontrib>Laborie, G.</creatorcontrib><creatorcontrib>Lee, S.C.</creatorcontrib><creatorcontrib>Levtchenko, P.</creatorcontrib><creatorcontrib>Liu, C.L.</creatorcontrib><creatorcontrib>Liu, H.T.</creatorcontrib><creatorcontrib>Lu, G.</creatorcontrib><creatorcontrib>Lu, 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I.</creatorcontrib><creatorcontrib>Vandenhirtz, J.</creatorcontrib><creatorcontrib>Velcea, F.</creatorcontrib><creatorcontrib>Verlaat, B.</creatorcontrib><creatorcontrib>Vezzu, F.</creatorcontrib><creatorcontrib>Von Gunten, H.</creatorcontrib><creatorcontrib>Waldmeier Wicki, S.</creatorcontrib><creatorcontrib>Wang, J.Z.</creatorcontrib><creatorcontrib>Wang, Y.H.</creatorcontrib><creatorcontrib>Wiik, K.</creatorcontrib><creatorcontrib>Wu, S.X.</creatorcontrib><creatorcontrib>Yan, J.L.</creatorcontrib><creatorcontrib>Yan, L.G.</creatorcontrib><creatorcontrib>Yang, C.G.</creatorcontrib><creatorcontrib>Yang, M.</creatorcontrib><creatorcontrib>Ye, S.W.</creatorcontrib><creatorcontrib>Xu, Z.Z.</creatorcontrib><creatorcontrib>Zhang, Z.P.</creatorcontrib><creatorcontrib>Zhao, D.X.</creatorcontrib><creatorcontrib>Zhu, G.Y.</creatorcontrib><creatorcontrib>Zhuang, H.L.</creatorcontrib><creatorcontrib>Zimmermann, B.</creatorcontrib><creatorcontrib>AMS Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ambrosi, G.</au><au>Ao, L.</au><au>Arefiev, A.</au><au>Azzarello, P.</au><au>Basile, M.</au><au>Barancourt, D.</au><au>Barao, F.</au><au>Becker, R.</au><au>Becker, U.</au><au>Berdugo, J.</au><au>Berges, P.</au><au>Bertucci, B.</au><au>Blasko, S.</au><au>Bourquin, M.</au><au>Brocco, L.</au><au>Buenerd, M.</au><au>Burger, J.D.</au><au>Burger, W.J.</au><au>Cai, X.D.</au><au>Capell, M.</au><au>Cecchi, C.</au><au>Chang, Y.H.</au><au>Chen, Z.G.</au><au>Cindolo, F.</au><au>Commichau, V.</au><au>Crespo, P.</au><au>Cristinziani, M.</au><au>Deus, J.D.</au><au>Djambazov, L.</au><au>D'Antone, I.</au><au>Emonet, P.</au><au>Engelberg, J.</au><au>Eppling, F.J.</au><au>Eronen, T.</au><au>Esposito, G.</au><au>Fiandrini, E.</au><au>Fisher, P.H.</au><au>Gervasi, M.</au><au>Gu, W.Q.</au><au>Hangarter, K.</au><au>Hasan, A.</au><au>Hermel, V.</au><au>Huang, M.A.</au><au>Ionica, M.</au><au>Ionica, R.</au><au>Jongmanns, M.</au><au>Karlamaa, K.</au><au>Kim, W.</au><au>Kossakowski, R.</au><au>Kraeber, M.</au><au>Laborie, G.</au><au>Lee, S.C.</au><au>Levtchenko, P.</au><au>Liu, C.L.</au><au>Liu, H.T.</au><au>Lu, G.</au><au>Lu, Y.S.</au><au>Luckey, D.</au><au>Lustermann, W.</au><au>Palmonari, F.</au><au>Pesci, A.</au><au>Pevsner, A.</au><au>Pimenta, M.</au><au>Plyaskin, V.</au><au>Pojidaev, V.</au><au>Rapin, D.</au><au>Ren, Z.</au><au>Ribordy, M.</au><au>Roissin, C.</au><au>Sagdeev, R.</au><au>Schwering, G.</au><au>Scolieri, G.</au><au>Seo, E.S.</au><au>Song, T.</au><au>Ting, Samuel C.C.</au><au>Tornikoski, M.</au><au>Torsti, J.</au><au>Trümper, J.</au><au>Usoskin, I.</au><au>Vandenhirtz, J.</au><au>Velcea, F.</au><au>Verlaat, B.</au><au>Vezzu, F.</au><au>Von Gunten, H.</au><au>Waldmeier Wicki, S.</au><au>Wang, J.Z.</au><au>Wang, Y.H.</au><au>Wiik, K.</au><au>Wu, S.X.</au><au>Yan, J.L.</au><au>Yan, L.G.</au><au>Yang, C.G.</au><au>Yang, M.</au><au>Ye, S.W.</au><au>Xu, Z.Z.</au><au>Zhang, Z.P.</au><au>Zhao, D.X.</au><au>Zhu, G.Y.</au><au>Zhuang, H.L.</au><au>Zimmermann, B.</au><aucorp>AMS Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Cosmic protons</atitle><jtitle>Physics letters. B</jtitle><date>2000-09-28</date><risdate>2000</risdate><volume>490</volume><issue>1</issue><spage>27</spage><epage>35</epage><pages>27-35</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><abstract>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 flight STS–91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented.</abstract><pub>Elsevier B.V</pub><doi>10.1016/S0370-2693(00)00970-9</doi><tpages>9</tpages><orcidid>https://orcid.org/0000-0001-9995-4792</orcidid><orcidid>https://orcid.org/0000-0003-4365-3282</orcidid><orcidid>https://orcid.org/0000-0003-3842-8531</orcidid><orcidid>https://orcid.org/0000-0001-5760-8939</orcidid><orcidid>https://orcid.org/0000-0002-1288-833X</orcidid><orcidid>https://orcid.org/0000-0003-1249-6026</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0370-2693 |
| ispartof | Physics letters. B, 2000-09, Vol.490 (1), p.27-35 |
| issn | 0370-2693 1873-2445 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_in2p3_00006367v1 |
| source | Elsevier ScienceDirect Journals |
| subjects | Astrophysics Cosmology and Extra-Galactic Astrophysics Physics |
| title | Cosmic protons |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T03%3A31%3A41IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_hal_p&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Cosmic%20protons&rft.jtitle=Physics%20letters.%20B&rft.au=Ambrosi,%20G.&rft.aucorp=AMS%20Collaboration&rft.date=2000-09-28&rft.volume=490&rft.issue=1&rft.spage=27&rft.epage=35&rft.pages=27-35&rft.issn=0370-2693&rft.eissn=1873-2445&rft_id=info:doi/10.1016/S0370-2693(00)00970-9&rft_dat=%3Celsevier_hal_p%3ES0370269300009709%3C/elsevier_hal_p%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_els_id=S0370269300009709&rfr_iscdi=true |