The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle

M. Aguilar; J. Alcaraz; J. Allaby; B. Alpat; G. Ambrosi; H. Anderhub; L. Ao; A. Arefiev; P. Azzarello; E. Babucci; L. Baldini; M. Basile; D. Barancourt; F. Barao; G. Barbier; G. Barreira; R. Battiston; R. Becker; U. Becker; L. Bellagamba; P. Béné; J. Berdugo; P. Berges; B. Bertucci; A. Biland; S. Bizzaglia; S. Blasko; G. Boella; M. Boschini; M. Bourquin; L. Brocco; G. Bruni; M. Buénerd; J. D. Burger; W. J. Burger; X. D. Cai; C. Camps; P. Cannarsa; M. Capell; D. Casadei; J. Casaus; G. Castellini; C. Cecchi; Y. H. Chang; H. F. Chen; H. S. Chen; Z. G. Chen; N. A. Chernoplekov; T. H. Chiueh; K. Cho; M. J. Choi; Y. Y. Choi; Y. L. Chuang; F. Cindolo; V. Commichau; A. Contin; E. Cortina-Gil; M. Cristinziani; J. P. da Cunha; T. S. Dai; C. Delgado; J. D. Deus; N. Dinu; L. Djambazov; I. D'Antone; Z. R. Dong; P. Emonet; J. Engelberg; F. J. Eppling; T. Eronen; G. Esposito; P. Extermann; J. Favier; E. Fiandrini; P. H. Fisher; G. Fluegge; N. Fouque; Yu Galaktionov; M. Gervasi; P. Giusti; D. Grandi; O. Grimms; W. Q. Gu; K. Hangarter; A. Hasan; V. Hermel; H. Hofer; M. A. Huang; W. Hungerford; M. Ionica; R. Ionica; M. Jongmanns; K. Karlamaa; W. Karpinski; G. Kenney; J. Kenny; D. H. Kim; G. N. Kim; K. S. Kim; M. Y. Kim; A. Klimentov; R. Kossakowski; V. Koutsenko; M. Kraeber; G. Laborie; T. Laitinen; G. Lamanna; E. Lanciotti; G. Laurenti; A. Lebedev; C. Lechanoine-Leluc; M. W. Lee; S. C. Lee; G. Levi; P. Levtchenko; C. L. Liu; H. T. Liu; I. Lopes; G. Lu; Y. S. Lu; K. Lübelsmeyer; D. Luckey; W. Lustermann; C. Maña; A. Margotti; F. Mayet; R. R. McNeil; B. Meillon; M. Menichelli; A. Mihul; A. Mourao; A. Mujunen; F. Palmonari; A. Papi; H. B. Park; W. H. Park; M. Pauluzzi; F. Pauss; E. Perrin; A. Pesci; A. Pevsner; M. Pimenta; V. Plyaskin; V. Pojidaev; M. Pohl; V. Postolache; N. Produit; P. G. Rancoita; D. Rapin; F. Raupach; D. Ren; Z. Ren; M. Ribordy; J. P. Richeux; E. Riihonen; J. Ritakari; S. Ro; U. Roeser; C. Rossin; R. Sagdeev; D. Santos; G. Sartorelli; C. Sbarra; S. Schael; A. Schultz von Dratzig; G. Schwering; G. Scolieri; E. S. Seo; J. W. Shin; V. Shoutko; E. Shoumilov; R. Siedling; D. Son; T. Song; M. Steuer; G. S. Sun; H. Suter; X. W. Tang; Samuel C.C. Ting; S. M. Ting; M. Tornikoski; J. Torsti; J. Trümper; J. Ulbricht; S. Urpo; E. Valtonen; J. Vandenhirtz; F. Velcea; E. Velikhov; B. Verlaat; I. Vetlitsky; F. Vezzu; J. P. Vialle; G. Viertel; D. Vité; H. von Gunten; S. Waldmeier Wicki; W. Wallraff; B. C. Wang; J. Z. Wang; Y. H. Wang; K. Wiik; C. Williams; S. X. WU; P. C. Xia; J. L. Yan; L. G. Yan; C. G. Yang; J. Yang; M. Yang; S. W. Ye; P. Yeh; Z. Z. Xu; H. Y. Zhang; Z. P. Zhang; D. X. Zhao; G. Y. Zhu; W. Z. Zhu; H. L. Zhuang; A. Zichichi; B. Zimmermann; P. Zuccon

doi:10.1016/S0370-1573(02)00013-3

The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle

M. Aguilar, J. Alcaraz, J. Allaby, B. Alpat, G. Ambrosi, H. Anderhub, L. Ao, A. Arefiev, P. Azzarello, E. Babucci, L. Baldini, M. Basile, D. Barancourt, F. Barao, G. Barbier, G. Barreira, R. Battiston, R. Becker, U. Becker, L. BellagambaP. Béné, J. Berdugo, P. Berges, B. Bertucci, A. Biland, S. Bizzaglia, S. Blasko, G. Boella, M. Boschini, M. Bourquin, L. Brocco, G. Bruni, M. Buénerd, J. D. Burger, W. J. Burger, X. D. Cai, C. Camps, P. Cannarsa, M. Capell, D. Casadei, J. Casaus, G. Castellini, C. Cecchi, Y. H. Chang, H. F. Chen, H. S. Chen, Z. G. Chen, N. A. Chernoplekov, T. H. Chiueh, K. Cho, M. J. Choi, Y. Y. Choi, Y. L. Chuang, F. Cindolo, V. Commichau, A. Contin, E. Cortina-Gil, M. Cristinziani, J. P. da Cunha, T. S. Dai, C. Delgado, J. D. Deus, N. Dinu, L. Djambazov, I. D'Antone, Z. R. Dong, P. Emonet, J. Engelberg, F. J. Eppling, T. Eronen, G. Esposito, P. Extermann, J. Favier, E. Fiandrini, P. H. Fisher, G. Fluegge, N. Fouque, Yu Galaktionov, M. Gervasi, P. Giusti, D. Grandi, O. Grimms, W. Q. Gu, K. Hangarter, A. Hasan, V. Hermel, H. Hofer, M. A. Huang, W. Hungerford, M. Ionica, R. Ionica, M. Jongmanns, K. Karlamaa, W. Karpinski, G. Kenney, J. Kenny, D. H. Kim, G. N. Kim, K. S. Kim, M. Y. Kim, A. Klimentov, R. Kossakowski, V. Koutsenko, M. Kraeber, G. Laborie, T. Laitinen, G. Lamanna, E. Lanciotti, G. Laurenti, A. Lebedev, C. Lechanoine-Leluc, M. W. Lee, S. C. Lee, G. Levi, P. Levtchenko, C. L. Liu, H. T. Liu, I. Lopes, G. Lu, Y. S. Lu, K. Lübelsmeyer, D. Luckey, W. Lustermann, C. Maña, A. Margotti, F. Mayet, R. R. McNeil, B. Meillon, M. Menichelli, A. Mihul, A. Mourao, A. Mujunen, F. Palmonari, A. Papi, H. B. Park, W. H. Park, M. Pauluzzi, F. Pauss, E. Perrin, A. Pesci, A. Pevsner, M. Pimenta, V. Plyaskin, V. Pojidaev, M. Pohl, V. Postolache, N. Produit, P. G. Rancoita, D. Rapin, F. Raupach, D. Ren, Z. Ren, M. Ribordy, J. P. Richeux, E. Riihonen, J. Ritakari, S. Ro, U. Roeser, C. Rossin, R. Sagdeev, D. Santos, G. Sartorelli, C. Sbarra, S. Schael, A. Schultz von Dratzig, G. Schwering, G. Scolieri, E. S. Seo, J. W. Shin, V. Shoutko, E. Shoumilov, R. Siedling, D. Son, T. Song, M. Steuer, G. S. Sun, H. Suter, X. W. Tang, Samuel C.C. Ting, S. M. Ting, M. Tornikoski, J. Torsti, J. Trümper, J. Ulbricht, S. Urpo, E. Valtonen, J. Vandenhirtz, F. Velcea, E. Velikhov, B. Verlaat, I. Vetlitsky, F. Vezzu, J. P. Vialle, G. Viertel, D. Vité, H. von Gunten, S. Waldmeier Wicki, W. Wallraff, B. C. Wang, J. Z. Wang, Y. H. Wang, K. Wiik, C. Williams, S. X. WU, P. C. Xia, J. L. Yan, L. G. Yan, C. G. Yang, J. Yang, M. Yang, S. W. Ye, P. Yeh, Z. Z. Xu, H. Y. Zhang, Z. P. Zhang, D. X. Zhao, G. Y. Zhu, W. Z. Zhu, H. L. Zhuang, A. Zichichi, B. Zimmermann, P. Zuccon

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摘要

The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1-140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 × 10^-6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e⁺) and negative ones (e^-) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1-1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10^-3(m² s sr)^-1. Over 90 percent of the helium flux was determined to be ³He at the 90% confidence level.

原文	???core.languages.en_GB???
頁（從 - 到）	331-405
頁數	75
期刊	Physics Reports
卷	366
發行號	6
DOIs	https://doi.org/10.1016/S0370-1573(02)00013-3
出版狀態	已出版 - 2002

存取文件

10.1016/S0370-1573(02)00013-3

引用此

Aguilar, M., Alcaraz, J., Allaby, J., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., ... Zuccon, P. (2002). The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle. Physics Reports, 366(6), 331-405. https://doi.org/10.1016/S0370-1573(02)00013-3

@article{cc75c5cd59054c47ac3586d0e1c9e299,

title = "The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle",

abstract = "The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1-140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 × 10-6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e+) and negative ones (e-) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1-1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10-3(m2 s sr)-1. Over 90 percent of the helium flux was determined to be 3He at the 90% confidence level.",

author = "M. Aguilar and J. Alcaraz and J. Allaby and B. Alpat and G. Ambrosi and H. Anderhub and L. Ao and A. Arefiev and P. Azzarello and E. Babucci and L. Baldini and M. Basile and D. Barancourt and F. Barao and G. Barbier and G. Barreira and R. Battiston and R. Becker and U. Becker and L. Bellagamba and P. B{\'e}n{\'e} and J. Berdugo and P. Berges and B. Bertucci and A. Biland and S. Bizzaglia and S. Blasko and G. Boella and M. Boschini and M. Bourquin and L. Brocco and G. Bruni and M. Bu{\'e}nerd and Burger, {J. D.} and Burger, {W. J.} and Cai, {X. D.} and C. Camps and P. Cannarsa and M. Capell and D. Casadei and J. Casaus and G. Castellini and C. Cecchi and Chang, {Y. H.} and Chen, {H. F.} and Chen, {H. S.} and Chen, {Z. G.} and Chernoplekov, {N. A.} and Chiueh, {T. H.} and K. Cho and Choi, {M. J.} and Choi, {Y. Y.} and Chuang, {Y. L.} and F. Cindolo and V. Commichau and A. Contin and E. Cortina-Gil and M. Cristinziani and {da Cunha}, {J. P.} and Dai, {T. S.} and C. Delgado and Deus, {J. D.} and N. Dinu and L. Djambazov and I. D'Antone and Dong, {Z. R.} and P. Emonet and J. Engelberg and Eppling, {F. J.} and T. Eronen and G. Esposito and P. Extermann and J. Favier and E. Fiandrini and Fisher, {P. H.} and G. Fluegge and N. Fouque and Yu Galaktionov and M. Gervasi and P. Giusti and D. Grandi and O. Grimms and Gu, {W. Q.} and K. Hangarter and A. Hasan and V. Hermel and H. Hofer and Huang, {M. A.} and W. Hungerford and M. Ionica and R. Ionica and M. Jongmanns and K. Karlamaa and W. Karpinski and G. Kenney and J. Kenny and Kim, {D. H.} and Kim, {G. N.} and Kim, {K. S.} and Kim, {M. Y.} and A. Klimentov and R. Kossakowski and V. Koutsenko and M. Kraeber and G. Laborie and T. Laitinen and G. Lamanna and E. Lanciotti and G. Laurenti and A. Lebedev and C. Lechanoine-Leluc and Lee, {M. W.} and Lee, {S. C.} and G. Levi and P. Levtchenko and Liu, {C. L.} and Liu, {H. T.} and I. Lopes and G. Lu and Lu, {Y. S.} and K. L{\"u}belsmeyer and D. Luckey and W. Lustermann and C. Ma{\~n}a and A. Margotti and F. Mayet and McNeil, {R. R.} and B. Meillon and M. Menichelli and A. Mihul and A. Mourao and A. Mujunen and F. Palmonari and A. Papi and Park, {H. B.} and Park, {W. H.} and M. Pauluzzi and F. Pauss and E. Perrin and A. Pesci and A. Pevsner and M. Pimenta and V. Plyaskin and V. Pojidaev and M. Pohl and V. Postolache and N. Produit and Rancoita, {P. G.} and D. Rapin and F. Raupach and D. Ren and Z. Ren and M. Ribordy and Richeux, {J. P.} and E. Riihonen and J. Ritakari and S. Ro and U. Roeser and C. Rossin and R. Sagdeev and D. Santos and G. Sartorelli and C. Sbarra and S. Schael and {von Dratzig}, {A. Schultz} and G. Schwering and G. Scolieri and Seo, {E. S.} and Shin, {J. W.} and V. Shoutko and E. Shoumilov and R. Siedling and D. Son and T. Song and M. Steuer and Sun, {G. S.} and H. Suter and Tang, {X. W.} and Ting, {Samuel C.C.} and Ting, {S. M.} and M. Tornikoski and J. Torsti and J. Tr{\"u}mper and J. Ulbricht and S. Urpo and E. Valtonen and J. Vandenhirtz and F. Velcea and E. Velikhov and B. Verlaat and I. Vetlitsky and F. Vezzu and Vialle, {J. P.} and G. Viertel and D. Vit{\'e} and {von Gunten}, H. and {Waldmeier Wicki}, S. and W. Wallraff and Wang, {B. C.} and Wang, {J. Z.} and Wang, {Y. H.} and K. Wiik and C. Williams and WU, {S. X.} and Xia, {P. C.} and Yan, {J. L.} and Yan, {L. G.} and Yang, {C. G.} and J. Yang and M. Yang and Ye, {S. W.} and P. Yeh and Xu, {Z. Z.} and Zhang, {H. Y.} and Zhang, {Z. P.} and Zhao, {D. X.} and Zhu, {G. Y.} and Zhu, {W. Z.} and Zhuang, {H. L.} and A. Zichichi and B. Zimmermann and P. Zuccon",

year = "2002",

doi = "10.1016/S0370-1573(02)00013-3",

language = "???core.languages.en_GB???",

volume = "366",

pages = "331--405",

journal = "Physics Reports",

issn = "0370-1573",

number = "6",

}

Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Béné, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buénerd, M, Burger, JD, Burger, WJ, Cai, XD, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, YH, Chen, HF, Chen, HS, Chen, ZG, Chernoplekov, NA, Chiueh, TH, Cho, K, Choi, MJ, Choi, YY, Chuang, YL, Cindolo, F, Commichau, V, Contin, A, Cortina-Gil, E, Cristinziani, M, da Cunha, JP, Dai, TS, Delgado, C, Deus, JD, Dinu, N, Djambazov, L, D'Antone, I, Dong, ZR, Emonet, P, Engelberg, J, Eppling, FJ, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, PH, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimms, O, Gu, WQ, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, MA, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, DH, Kim, GN, Kim, KS, Kim, MY, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Lanciotti, E, Laurenti, G, Lebedev, A, Lechanoine-Leluc, C, Lee, MW, Lee, SC, Levi, G, Levtchenko, P, Liu, CL, Liu, HT, Lopes, I, Lu, G, Lu, YS, Lübelsmeyer, K, Luckey, D, Lustermann, W, Maña, C, Margotti, A, Mayet, F, McNeil, RR, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, HB, Park, WH, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Postolache, V, Produit, N, Rancoita, PG, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, JP, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Rossin, C, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, von Dratzig, AS, Schwering, G, Scolieri, G, Seo, ES, Shin, JW, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, GS, Suter, H, Tang, XW, Ting, SCC, Ting, SM, Tornikoski, M, Torsti, J, Trümper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, JP, Viertel, G, Vité, D, von Gunten, H, Waldmeier Wicki, S, Wallraff, W, Wang, BC, Wang, JZ, Wang, YH, Wiik, K, Williams, C, WU, SX, Xia, PC, Yan, JL, Yan, LG, Yang, CG, Yang, J, Yang, M, Ye, SW, Yeh, P, Xu, ZZ, Zhang, HY, Zhang, ZP, Zhao, DX, Zhu, GY, Zhu, WZ, Zhuang, HL, Zichichi, A, Zimmermann, B & Zuccon, P 2002, 'The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle', Physics Reports, 卷 366, 編號 6, 頁 331-405. https://doi.org/10.1016/S0370-1573(02)00013-3

TY - JOUR

T1 - The Alpha Magnetic Spectrometer (AMS) on the international space station

T2 - Part I - Results from the test flight on the space shuttle

AU - Aguilar, M.

AU - Alcaraz, J.

AU - Allaby, J.

AU - Alpat, B.

AU - Ambrosi, G.

AU - Anderhub, H.

AU - Ao, L.

AU - Arefiev, A.

AU - Azzarello, P.

AU - Babucci, E.

AU - Baldini, L.

AU - Basile, M.

AU - Barancourt, D.

AU - Barao, F.

AU - Barbier, G.

AU - Barreira, G.

AU - Battiston, R.

AU - Becker, R.

AU - Becker, U.

AU - Bellagamba, L.

AU - Béné, P.

AU - Berdugo, J.

AU - Berges, P.

AU - Bertucci, B.

AU - Biland, A.

AU - Bizzaglia, S.

AU - Blasko, S.

AU - Boella, G.

AU - Boschini, M.

AU - Bourquin, M.

AU - Brocco, L.

AU - Bruni, G.

AU - Buénerd, M.

AU - Burger, J. D.

AU - Burger, W. J.

AU - Cai, X. D.

AU - Camps, C.

AU - Cannarsa, P.

AU - Capell, M.

AU - Casadei, D.

AU - Casaus, J.

AU - Castellini, G.

AU - Cecchi, C.

AU - Chang, Y. H.

AU - Chen, H. F.

AU - Chen, H. S.

AU - Chen, Z. G.

AU - Chernoplekov, N. A.

AU - Chiueh, T. H.

AU - Cho, K.

AU - Choi, M. J.

AU - Choi, Y. Y.

AU - Chuang, Y. L.

AU - Cindolo, F.

AU - Commichau, V.

AU - Contin, A.

AU - Cortina-Gil, E.

AU - Cristinziani, M.

AU - da Cunha, J. P.

AU - Dai, T. S.

AU - Delgado, C.

AU - Deus, J. D.

AU - Dinu, N.

AU - Djambazov, L.

AU - D'Antone, I.

AU - Dong, Z. R.

AU - Emonet, P.

AU - Engelberg, J.

AU - Eppling, F. J.

AU - Eronen, T.

AU - Esposito, G.

AU - Extermann, P.

AU - Favier, J.

AU - Fiandrini, E.

AU - Fisher, P. H.

AU - Fluegge, G.

AU - Fouque, N.

AU - Galaktionov, Yu

AU - Gervasi, M.

AU - Giusti, P.

AU - Grandi, D.

AU - Grimms, O.

AU - Gu, W. Q.

AU - Hangarter, K.

AU - Hasan, A.

AU - Hermel, V.

AU - Hofer, H.

AU - Huang, M. A.

AU - Hungerford, W.

AU - Ionica, M.

AU - Ionica, R.

AU - Jongmanns, M.

AU - Karlamaa, K.

AU - Karpinski, W.

AU - Kenney, G.

AU - Kenny, J.

AU - Kim, D. H.

AU - Kim, G. N.

AU - Kim, K. S.

AU - Kim, M. Y.

AU - Klimentov, A.

AU - Kossakowski, R.

AU - Koutsenko, V.

AU - Kraeber, M.

AU - Laborie, G.

AU - Laitinen, T.

AU - Lamanna, G.

AU - Lanciotti, E.

AU - Laurenti, G.

AU - Lebedev, A.

AU - Lechanoine-Leluc, C.

AU - Lee, M. W.

AU - Lee, S. C.

AU - Levi, G.

AU - Levtchenko, P.

AU - Liu, C. L.

AU - Liu, H. T.

AU - Lopes, I.

AU - Lu, G.

AU - Lu, Y. S.

AU - Lübelsmeyer, K.

AU - Luckey, D.

AU - Lustermann, W.

AU - Maña, C.

AU - Margotti, A.

AU - Mayet, F.

AU - McNeil, R. R.

AU - Meillon, B.

AU - Menichelli, M.

AU - Mihul, A.

AU - Mourao, A.

AU - Mujunen, A.

AU - Palmonari, F.

AU - Papi, A.

AU - Park, H. B.

AU - Park, W. H.

AU - Pauluzzi, M.

AU - Pauss, F.

AU - Perrin, E.

AU - Pesci, A.

AU - Pevsner, A.

AU - Pimenta, M.

AU - Plyaskin, V.

AU - Pojidaev, V.

AU - Pohl, M.

AU - Postolache, V.

AU - Produit, N.

AU - Rancoita, P. G.

AU - Rapin, D.

AU - Raupach, F.

AU - Ren, D.

AU - Ren, Z.

AU - Ribordy, M.

AU - Richeux, J. P.

AU - Riihonen, E.

AU - Ritakari, J.

AU - Ro, S.

AU - Roeser, U.

AU - Rossin, C.

AU - Sagdeev, R.

AU - Santos, D.

AU - Sartorelli, G.

AU - Sbarra, C.

AU - Schael, S.

AU - von Dratzig, A. Schultz

AU - Schwering, G.

AU - Scolieri, G.

AU - Seo, E. S.

AU - Shin, J. W.

AU - Shoutko, V.

AU - Shoumilov, E.

AU - Siedling, R.

AU - Son, D.

AU - Song, T.

AU - Steuer, M.

AU - Sun, G. S.

AU - Suter, H.

AU - Tang, X. W.

AU - Ting, Samuel C.C.

AU - Ting, S. M.

AU - Tornikoski, M.

AU - Torsti, J.

AU - Trümper, J.

AU - Ulbricht, J.

AU - Urpo, S.

AU - Valtonen, E.

AU - Vandenhirtz, J.

AU - Velcea, F.

AU - Velikhov, E.

AU - Verlaat, B.

AU - Vetlitsky, I.

AU - Vezzu, F.

AU - Vialle, J. P.

AU - Viertel, G.

AU - Vité, D.

AU - von Gunten, H.

AU - Waldmeier Wicki, S.

AU - Wallraff, W.

AU - Wang, B. C.

AU - Wang, J. Z.

AU - Wang, Y. H.

AU - Wiik, K.

AU - Williams, C.

AU - WU, S. X.

AU - Xia, P. C.

AU - Yan, J. L.

AU - Yan, L. G.

AU - Yang, C. G.

AU - Yang, J.

AU - Yang, M.

AU - Ye, S. W.

AU - Yeh, P.

AU - Xu, Z. Z.

AU - Zhang, H. Y.

AU - Zhang, Z. P.

AU - Zhao, D. X.

AU - Zhu, G. Y.

AU - Zhu, W. Z.

AU - Zhuang, H. L.

AU - Zichichi, A.

AU - Zimmermann, B.

AU - Zuccon, P.

PY - 2002

Y1 - 2002

N2 - The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1-140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 × 10-6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e+) and negative ones (e-) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1-1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10-3(m2 s sr)-1. Over 90 percent of the helium flux was determined to be 3He at the 90% confidence level.

AB - The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1-140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 × 10-6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e+) and negative ones (e-) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1-1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10-3(m2 s sr)-1. Over 90 percent of the helium flux was determined to be 3He at the 90% confidence level.

UR - http://www.scopus.com/inward/record.url?scp=0036296546&partnerID=8YFLogxK

U2 - 10.1016/S0370-1573(02)00013-3

DO - 10.1016/S0370-1573(02)00013-3

M3 - 回顧評介論文

AN - SCOPUS:0036296546

SN - 0370-1573

VL - 366

SP - 331

EP - 405

JO - Physics Reports

JF - Physics Reports

IS - 6

ER -

The Alpha Magnetic Spectrometer (AMS) on the international space station: Part I - Results from the test flight on the space shuttle

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