The Alpha Magnetic Spectrometer (AMS) on the International Space Station:: Part I -: results from the test flight on the space shuttle

被引:393
作者
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 [1 ]
Casadei, D
Casaus, J
Castellini, G
Cecchi, C
Chang, YH
Chen, HF
Chen, HS
Chen, ZG
Chernoplekov, NA
Chiueh, TH
Cho, K
机构
[1] CIEMAT, Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain
[2] CERN, European Lab Particle Phys, CH-1211 Geneva 23, Switzerland
[3] Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy
[4] Univ Perugia, I-06100 Perugia, Italy
[5] Univ Geneva, CH-1211 Geneva 4, Switzerland
[6] Swiss Fed Inst Technol, CH-8093 Zurich, Switzerland
[7] Chinese Acad Launching Vehicle Technol, CALT, Beijing 100076, Peoples R China
[8] Inst Theoret & Expt Phys, Moscow 117259, Russia
[9] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy
[10] Univ Bologna, I-40126 Bologna, Italy
[11] MIT, Cambridge, MA 02139 USA
[12] CNRS, Inst Nucl Sci, IN2P3, F-38026 Grenoble, France
[13] LIP, Lab Instrumentacao & Fis Expt Particulas, P-1000 Lisbon, Portugal
[14] Inst Super Tecn, P-1096 Lisbon, Portugal
[15] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy
[16] Rhein Westfal TH Aachen, Inst Phys 3, D-52056 Aachen, Germany
[17] CNR, IROE, I-50125 Florence, Italy
[18] Natl Cent Univ, Chungli 32054, Taiwan
[19] Univ Sci & Technol China, USTC, Hefei 230029, Anhui, Peoples R China
[20] Chinese Acad Sci, IHEP, Beijing 100039, Peoples R China
[21] IV Kurchatov Atom Energy Inst, Moscow 123182, Russia
[22] Kyungpook Natl Univ, CHEP, Taegu 702701, South Korea
[23] Ewha Womans Univ, Seoul 120750, South Korea
[24] Acad Sinica, Taipei 11529, Taiwan
[25] LIP, Lab Instrumentacao & Fis Expt Particulas, P-3000 Coimbra, Portugal
[26] Chinese Acad Sci, Inst Elect Engn, Beijing 100080, Peoples R China
[27] Aalto Univ, FIN-02540 Kylmala, Finland
[28] Turku Univ, FIN-20014 Turku, Finland
[29] Lab Annecy Le Vieux Phys Particules, LAPP, F-74941 Annecy Le Vieux, France
[30] Rhein Westfal TH Aachen, Inst Phys 1, D-52056 Aachen, Germany
[31] Chung Shan Inst Sci & Technol, Tao Yuan 325, Taiwan
[32] Louisiana State Univ, Baton Rouge, LA 70803 USA
[33] Univ Politehn Bucuresti, Inst Microtechnol, R-76900 Bucharest, Romania
[34] Univ Bucharest, HEPPG, R-76900 Bucharest, Romania
[35] Johns Hopkins Univ, Baltimore, MD 21218 USA
[36] Univ Maryland, College Pk, MD 20742 USA
[37] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[38] Chinese Acad Sci, Ctr Space Sci & Applicat, Beijing 100080, Peoples R China
[39] Russian Acad Sci, Inst Nucl Phys, St Petersburg, Russia
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2002年 / 366卷 / 06期
关键词
D O I
10.1016/S0370-1573(02)00013-3
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7degrees 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 x 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) x 10(-3)(m(2) s sr)(-1). Over 90 percent of the helium flux was determined to be He-3 at the 90% confidence level. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:331 / 405
页数:75
相关论文
共 179 条
  • [11] Leptons in near earth orbit
    Alcaraz, 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, C
    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
    Buenerd, 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
    Chuang, YL
    Cindolo, F
    Commichau, V
    [J]. PHYSICS LETTERS B, 2000, 484 (1-2) : 10 - 22
  • [12] Helium in near Earth orbit
    Alcaraz, 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
    Buenerd, 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
    Chuang, YL
    Cindolo, F
    Commichau, V
    [J]. PHYSICS LETTERS B, 2000, 494 (3-4) : 193 - 202
  • [13] ELASTIC AND INELASTIC-SCATTERING OF 1.37 GEV ALPHA-PARTICLES FROM CA-40, CA-42, CA-44, CA-48
    ALKHAZOV, GD
    BAUER, T
    BERTINI, R
    BIMBOT, L
    BING, O
    BOUDARD, A
    BRUGE, G
    CATZ, H
    CHAUMEAUX, A
    COUVERT, P
    FONTAINE, JM
    HIBOU, F
    IGO, GJ
    LUGOL, JC
    MATOBA, M
    [J]. NUCLEAR PHYSICS A, 1977, 280 (02) : 365 - 376
  • [14] A high resolution, low power time-of-flight system for the space experiment AMS
    Alvisi, D
    Anselmo, F
    Baldini, L
    Bari, G
    Basile, M
    Bellagamba, L
    Bruni, A
    Bruni, G
    Boscherini, D
    Casadei, D
    Romeo, GC
    Castellini, G
    Cifarelli, L
    Cindolo, F
    Contin, A
    De Pasquale, S
    Giusti, P
    Iacobucci, G
    Laurenti, G
    Levi, G
    Margotti, A
    Massam, T
    Nania, R
    Palmonari, F
    Polini, A
    Recupero, S
    Sartorelli, G
    Williams, C
    Zichichi, A
    [J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1999, 437 (2-3) : 212 - 221
  • [15] ANDREEV IV, 1978, SOV J NUCL PHYS+, V28, P243
  • [16] Apparao K.M.V., 1973, P INT COSM RAY C DEN, V1, P126
  • [17] Cosmic-ray proton and helium spectra: Results from the JACEE experiment
    Asakimori, K
    Burnett, TH
    Cherry, ML
    Chevli, K
    Christ, MJ
    Dake, S
    Derrickson, JH
    Fountain, WF
    Fuki, M
    Gregory, JC
    Hayashi, T
    Holynski, R
    Iwai, J
    Iyono, A
    Johnson, J
    Kobayashi, M
    Lord, J
    Miyamura, O
    Moon, KH
    Nilsen, BS
    Oda, H
    Ogata, T
    Olson, ED
    Parnell, TA
    Roberts, FE
    Sengupta, K
    Shiina, T
    Strausz, SC
    Sugitate, T
    Takahashi, Y
    Tominaga, T
    Watts, JW
    Wefel, JP
    Wilczynska, B
    Wilczynski, H
    Wilkes, RJ
    Wolter, W
    Yokomi, H
    Zager, E
    [J]. ASTROPHYSICAL JOURNAL, 1998, 502 (01) : 278 - 283
  • [18] ASAKIMORI K, 1993, 23RD P INT COSM RAY, V2, P25
  • [19] AZHGIREI LS, 1979, SOV J NUCL PHYS+, V30, P818
  • [20] Cherenkov detectors in the alpha magnetic spectrometer
    Barao, F
    [J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2000, 454 (01) : 174 - 179