Journal ArticleDOI
Leptons in near earth orbit
J. Alcaraz,Behcet Alpat,Giovanni Ambrosi,H. Anderhub,L. Ao,A. Arefiev,P. Azzarello,E. Babucci,L. Baldini,M. Basile,D. Barancourt,F. Barao,G. Barbier,G.P. Barreira,Roberto Battiston,R. Becker,U. Becker,L. Bellagamba,P. Bene,J. Berdugo,P. Berges,B. Bertucci,Adrian Biland,S. Bizzaglia,S. Blasko,G. Boella,M. J. Boschini,M. Bourquin,L. Brocco,Giovanna Bruni,M. Buenerd,J. D. Burger,W. J. Burger,X. D. Cai,C. Camps,P. Cannarsa,M. Capell,Diego Casadei,J. Casaus,G. Castellini,Claudia Cecchi,Y. H. Chang,H. F. Chen,H. S. Chen,Z.G. Chen,N.A. Chernoplekov,Tzihong Chiueh,Y.L. Chuang,Federico Cindolo,V. Commichau,A. Contin,P. Crespo,Markus Cristinziani,J. P. Da Cunha,T. S. Dai,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,Peter H. Fisher,G. Fluegge,N. Fouque,Yu. Galaktionov,Massimo Gervasi,P. Giusti,D. Grandi,O. Grimm,W.Q. Gu,K. Hangarter,A. Hasan,V. Hermel,H. Hofer,M. A. Huang,W. Hungerford,M. Ionica,R. Ionica,M. Jongmanns,K. Karlamaa,Waclaw Karpinski,G. Kenney,Jose Maria Kenny,W. Kim,A. Klimentov,R. Kossakowski,V. Koutsenko,M. Kraeber,G. Laborie,Timo Laitinen,G. Lamanna,G. Laurenti,A. Lebedev,S.C. Lee,Giuseppe Levi,P. Levtchenko,C.L. Liu,H. T. Liu,I. Lopes,G. Lu,Lu Yuzhang,K. Lübelsmeyer,D. Luckey,Werner Lustermann,C. Maña,Anselmo Margotti,F. Mayet,R. R. McNeil,B. Meillon,Mauro Menichelli,A. Mihul,A. Mourao,Ari Mujunen,F. Palmonari,A. Papi,Inkyu Park,M. Pauluzzi,Felicitas Pauss,E. Perrin,A. Pesci,A. Pevsner,M. Pimenta,V. Plyaskin,V. Pojidaev,V. Postolache,N. Produit,P. G. Rancoita,D. Rapin,Frank Raupach,D. Ren,Z. L. Ren,M. Ribordy,J.P. Richeux,E. Riihonen,J. Ritakari,U. Roeser,C. Roissin,Roald Z. Sagdeev,G. Sartorelli,A. Schultz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,V. Shoutko,E. Shoumilov,R. Siedling,Dong-Chul Son,Tengfei Song,M. Steuer,G.S. Sun,H. Suter,Xiao-Dong Tang,Samuel C.C. Ting,S. M. Ting,Merja Tornikoski,J. J. Torsti,J. Trümper,J. Ulbricht,S. Urpo,Ilya Usoskin,Eino Valtonen,J. Vandenhirtz,F. Velcea,E. P. 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,Jing Wang,Yun Wang,K. Wiik,Ciaran Williams,S. X. Wu,S. X. Wu,P.C. Xia,J.L. Yan,L.G. Yan,Changgen Yang,Mao-Zhi Yang,S.W. Ye,P. Yeh,Z. Z. Xu,Hao Zhang,Zhenyu Zhang,Dawei Zhao,Guohuai Zhu,W.Z. Zhu,H.L. Zhuang,Antonino Zichichi,B. Zimmermann +202 more
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TLDR
The lepton kinetic energy ranges from 0.2 to 40 GeV for e − and from 3 GeV to 6 GeVs for e + were measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at altitudes near 380 km.About:
This article is published in Physics Letters B.The article was published on 2000-06-29. It has received 248 citations till now. The article focuses on the topics: Lepton & Cosmic ray.read more
Citations
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Journal ArticleDOI
An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,G. De Rosa,N. De Simone,V. Di Felice,A. M. Galper,L. A. Grishantseva,Petter Hofverberg,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,Silvio Orsi,G. Osteria,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,M. Simon,Roberta Sparvoli,Piero Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +50 more
TL;DR: It is found that the positron fraction increases sharply over much of that range, in a way that appears to be completely inconsistent with secondary sources, and is concluded that a primary source, be it an astrophysical object or dark matter annihilation, is necessary.
Journal ArticleDOI
An excess of cosmic ray electrons at energies of 300-800 GeV
Jin Chang,James H. Adams,H. S. Ahn,G. L. Bashindzhagyan,M. Christl,O. Ganel,T. G. Guzik,Joachim Isbert,K. C. Kim,E. N. Kuznetsov,M. I. Panasyuk,Alexander D. Panov,Wolfgang Schmidt,Eun-Suk Seo,N. V. Sokolskaya,John W. Watts,John P. Wefel,J. Wu,V. I. Zatsepin +18 more
TL;DR: An excess of galactic cosmic-ray electrons at energies of ∼300–800 GeV is reported, which indicates a nearby source of energetic electrons, or the electrons could arise from the annihilation of dark matter particles.
Journal ArticleDOI
Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
M. Aguilar,D. Aisa,Behcet Alpat,A. Alvino,G. Ambrosi,K. Andeen,Luísa Arruda,N. Attig,Philipp Azzarello,A. Bachlechner,Fernando Barão,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,Markus Battarbee,Roberto Battiston,J. Bazo,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,G. Bigongiari,Veronica Bindi,S. Bizzaglia,M. Bizzarri,G. Boella,W. De Boer,K. Bollweg,V. Bonnivard,B. Borgia,S. Borsini,Matteo Boschini,M. Bourquin,J. D. Burger,Franck Cadoux,X. D. Cai,M. Capell,S. Caroff,J. Casaus,V. Cascioli,G. Castellini,I. Cernuda,D. Cerreta,F. Cervelli,M. J. Chae,Yuan-Hann Chang,A. I. Chen,H. S. Chen,G. M. Cheng,H. S. Chen,Lin Cheng,H. Y. Chou,E. Choumilov,V. Choutko,C. H. Chung,C. Clark,R. Clavero,G. Coignet,C. Consolandi,A. Contin,Claudio Corti,E. Cortina Gil,B. Coste,W. Creus,M. Crispoltoni,Z. Cui,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,L. Di Masso,F. Dimiccoli,Carlos Díaz,P. von Doetinchem,F. Donnini,W. J. Du,M. Duranti,D. D'Urso,A. Eline,F. J. Eppling,T. Eronen,Y. Y. Fan,L. Farnesini,J. Feng,E. Fiandrini,A. Fiasson,E. Finch,Peter H. Fisher,Yu. Galaktionov,G. Gallucci,Bruce Rafael Mellado Garcia,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,W. Gillard,F. Giovacchini,P. Goglov,J. Gong,C. Goy,Varlen Grabski,D. Grandi,M. Graziani,C. Guandalini,I. Guerri,K. H. Guo,D. Haas,M. Habiby,Sadakazu Haino,K. C. Han,Z. H. He,Matthias Heil,J. Hoffman,Timothy H. Hsieh,Zhiqi Huang,Changgi Huh,M. Incagli,Maria Ionica,W. Y. Jang,H. Jinchi,K. Kanishev,G. N. Kim,Kwangsoo Kim,T. Kirn,R. Kossakowski,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,G. La Vacca,E. Laudi,G. Laurenti,I. Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,Giuseppe Levi,H. L. Li,J. Q. Li,Qiang Li,T. X. Li,Wei Li,Y. Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,Dong Liu,Hengchang Liu,M. Lolli,Teimuraz Lomtadze,M. J. Lu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,J. Z. Luo,S. S. Lv,R. D. Majka,C. Mañá,J. C. Marin,Tim Martin,G. Martinez,N. Masi,David Maurin,A. Menchaca-Rocha,Q. Meng,D. C. Mo,Luca Morescalchi,P. Mott,M. Müller,J. Q. Ni,N. Nikonov,F. Nozzoli,P. Nunes,A. Obermeier,A. Oliva,M. Orcinha,F. Palmonari,C. Palomares,M. Paniccia,A. Papi,M. Pauluzzi,E. Pedreschi,S. Pensotti,R. Pereira,N. Picot-Clemente,Fabrizio Giulio Luca Pilo,A. Piluso,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,E. Postaci,Antje Putze,Lucio Quadrani,X. M. Qi,Xubo Qin,Z. Y. Qu,T. Räihä,Pier-Giorgio Rancoita,D. Rapin,J. S. Ricol,I. Rodríguez,S. Rosier-Lees,A. Rozhkov,Davide Rozza,Roald Z. Sagdeev,J. Sandweiss,P. Saouter,C. Sbarra,S. Schael,S. M. Schmidt,A. Schulz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,B. S. Shan,Y. H. Shan,J. Y. Shi,X. Y. Shi,Yun Shi,T. Siedenburg,Dong-Chul Son,F. Spada,F. Spinella,Won Kyu Calvin Sun,W. H. Sun,Mauro Tacconi,C. P. Tang,X. W. Tang,Zhixiang Tang,L. Tao,D. Tescaro,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Türkoğlu,T. Urban,V. Vagelli,E. Valente,C. Vannini,Eino Valtonen,S. S. Vaurynovich,M. Vecchi,Mayda Velasco,J. P. Vialle,V. Vitale,S. Vitillo,Liqiu Wang,Naihua Wang,Q. L. Wang,Ruiguang Wang,Xiaoping Wang,Zheng Wang,Z. L. Weng,K. Whitman,J. Wienkenhöver,H. Wu,Xin Wu,X. Xia,M. Xie,S. Xie,R. Q. Xiong,Gongming Xin,Ningsheng Xu,W. Xu,Qing-Bo Yan,J. Yang,Mingming Yang,Q. H. Ye,H. Yi,Y. J. Yu,Z. Q. Yu,S. Zeissler,J. H. Zhang,M. T. Zhang,X. B. Zhang,Zhijun Zhang,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,A. Zichichi,N. Zimmermann,Paolo Zuccon,C. Zurbach +294 more
TL;DR: In this paper, a precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1.GV to 1.8TV is presented based on 300 million events.
Journal ArticleDOI
Diffuse Galactic continuum gamma rays. A model compatible with EGRET data and cosmic-ray measurements
TL;DR: In this article, the compatibility of current models of the diffuse Galactic continuum gamma-rays with EGRET data is studied. But the results are limited to a set of regions sampling the whole sky.
Journal ArticleDOI
Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station
M. Aguilar,L. Ali Cavasonza,Behcet Alpat,G. Ambrosi,L. Arruda,N. Attig,S. Aupetit,Philipp Azzarello,A. Bachlechner,F. Barao,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,S. Başeǧmez-Du Pree,Markus Battarbee,Roberto Battiston,Roberto Battiston,J. Bazo,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,Veronica Bindi,G. Boella,W. De Boer,K. Bollweg,V. Bonnivard,B. Borgia,M. J. Boschini,M. Bourquin,E. f. Bueno,J. D. Burger,Franck Cadoux,X. D. Cai,M. Capell,S. Caroff,J. Casaus,G. Castellini,I. Cernuda,F. Cervelli,M. J. Chae,Y. H. Chang,A. I. Chen,Guo-Ming Chen,H. S. Chen,Lin Cheng,H. Y. Chou,E. Choumilov,V. Choutko,C. H. Chung,C. Clark,R. Clavero,G. Coignet,C. Consolandi,Andrea Contin,Claudio Corti,B. Coste,W. Creus,M. Crispoltoni,Z. Cui,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,F. Dimiccoli,Carlos Díaz,P. von Doetinchem,F. Dong,F. Donnini,M. Duranti,D. D'Urso,A. Egorov,A. Eline,T. Eronen,J. Feng,E. Fiandrini,E. Finch,P. H. Fisher,V. Formato,Yu. Galaktionov,G. Gallucci,Bruce Rafael Mellado Garcia,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,F. Giovacchini,P. Goglov,D. M. Gómez-Coral,J. Gong,C. Goy,Varlen Grabski,D. Grandi,M. Graziani,I. Guerri,K. H. Guo,M. Habiby,Sadakazu Haino,K. C. Han,Z. H. He,Matthias Heil,J. Hoffman,Timothy H. Hsieh,H. P. Huang,Zhiqi Huang,Changgi Huh,M. Incagli,Maria Ionica,W. Y. Jang,H. Jinchi,S. C. Kang,K. Kanishev,G. N. Kim,Kwangsoo Kim,T. Kirn,C. Konak,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,G. La Vacca,Elisa Laudi,G. Laurenti,I. Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,Hui Li,Jinglai Li,Qiang Li,T. X. Li,Wei Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,D. Liu,Hu Liu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,F. Luo,J. Z. Luo,S. S. Lv,R. D. Majka,C. Mañá,J. C. Marin,T. Martin,G. Martinez,N. Masi,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,D. C. Mo,Luca Morescalchi,P. Mott,T. J. N. Nelson,J. Q. Ni,N. Nikonov,F. Nozzoli,P. Nunes,A.I. Oliva,M. Orcinha,F. Palmonari,C. Palomares,M. Paniccia,M. Pauluzzi,S. Pensotti,R. Pereira,N. Picot-Clemente,Fabrizio Giulio Luca Pilo,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,Antje Putze,Lucio Quadrani,X. M. Qi,Xubo Qin,Z. Y. Qu,T. Räihä,P. G. Rancoita,D. Rapin,J. S. Ricol,I. Rodríguez,S. Rosier-Lees,A. Rozhkov,Davide Rozza,Roald Z. Sagdeev,J. Sandweiss,P. Saouter,S. Schael,S. M. Schmidt,A. Schulz von Dratzig,G. Schwering,Eun-Suk Seo,B. S. Shan,J. Y. Shi,T. Siedenburg,Dong-Chul Son,J. W. Song,W. H. Sun,Mauro Tacconi,X. W. Tang,Zhixiang Tang,L. Tao,D. Tescaro,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Türkoğlu,T. Urban,V. Vagelli,E. Valente,C. Vannini,Eino Valtonen,M. Vazquez Acosta,Manuela Vecchi,Mayda Velasco,J. P. Vialle,V. Vitale,S. Vitillo,Liqiu Wang,Naihua Wang,Q. L. Wang,Xiaoqun Wang,X. Q. Wang,Zhao Wang,C. C. Wei,Z. L. Weng,K. Whitman,J. Wienkenhöver,M. Willenbrock,H. Wu,Xin Wu,X. Xia,R. Q. Xiong,W. Xu,Q. Yan,J. Yang,Mingming Yang,Yang Yang,H. Yi,Y. J. Yu,Z. Q. Yu,S. Zeissler,Chuanguo Zhang,J. Zhang,J. H. Zhang,S. Zhang,Shihao Zhang,Zhiqing Zhang,Z. M. Zheng,Zhihai Zhu,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,Paolo Zuccon +268 more
TL;DR: In the absolute rigidity range ∼60 to ∼500 GV, the antiproton p[over ¯], proton p, and positron e^{+} fluxes are found to have nearly identical rigidity dependence and the electron e^{-} flux exhibits a different rigidity dependent.
References
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Journal ArticleDOI
Protons in near earth orbit
J. Alcaraz,D. Alvisi,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.P. Barreira,Roberto 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,G. Bruni,M. Buenerd,J. D. Burger,W. J. Burger,X. D. Cai,R. Cavalletti,C. Camps,P. Cannarsa,M. Capell,D. Casadei,J. Casaus,G. Castellini,Y. H. Chang,H. F. Chen,H. S. Chen,Z. G. Chen,N. A. Chernoplekov,A. Chiarini,Tzihong Chiueh,Y. L. Chuang,F. Cindolo,V. Commichau,A. Contin,A. CottaRamusino,P. Crespo,Markus Cristinziani,J. P. Da Cunha +55 more
TL;DR: The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at an altitude of 380km as discussed by the authors.
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Physics of the upper polar atmosphere
TL;DR: In this paper, the authors present a model of the Earth's magnetic field and magnetosphere and show that the magnetic field can be represented as a permutation of the permutation.
Journal ArticleDOI
An Antimatter spectrometer in space
S. P. Ahlen,V. M. Balebanov,Roberto Battiston,U. Becker,J. D. Burger,M. Capell,H. F. Chen,H. S. Chen,Mingshui Chen,N. Chernoplekov,Robert Clare,T.S. Dai,A. De Rujula,Ph Fisher,Yu. Galaktionov,A. Gougas,Gu Wen-Qi,M. He,V. Koutsenko,A. Lebedev,Taosheng Li,Yunpeng Lu,D. Luckey,Ma Yuhua,R. McNeil,R. Orava,A. Prevsner,V. Plyaskine,H. Rubinstein,R. Sagdeev,M. H. Salamon,H. W. Tang,Samuel C.C. Ting,I. Vetlitsky,Y. F. Wang,Xia Ping-Chou,Zhenghao Xu,J. P. Wefel,Zhongming Zhang,B. Zhou,Antonino Zichichi +40 more
TL;DR: In this article, a simple magnetic spectrometer to be installed on a satellite or space station is discussed, which is used to search for primordial antimatter to the level of antimatter/matter ≈10 − 9, improving the existing limits obtained with balloon flights by a factor of 10 4 to 10 5.
Journal ArticleDOI
A revised corrected geomagnetic coordinate system for Epochs 1985 and 1990.
TL;DR: In this paper, a new set of corrected geomagnetic coordinates (CGM) has been calculated from the magnetic field model DGRF for Epoch 1985 and the IGRF model for epoch 1990, which is based on the vertical projection on the Earth's surface of the B -minimum value point (apex) on each geOMagnetic field line.
Journal ArticleDOI
Search for antihelium in cosmic rays
J. Alcaraz,D. Alvisi,B. Alpat,G. Ambrosi,H. Anderhub,L. Ao,A. Arefiev,Philipp Azzarello,E. Babucci,L. Baldini,L. Baldini,M. Basile,D. Barancourt,F. Barao,G. Barbier,G.P. Barreira,Roberto Battiston,R. Becker,U. Becker,L. Bellagamba,P. Bene,J. Berdugo,P. Berges,B. Bertucci,Adrian Biland,S. Bizzaglia,S. Blasko,G. Boella,M. Bourquin,G. Bruni,M. Buenerd,J. D. Burger,W. J. Burger,X. D. Cai,R. Cavalletti,C. Camps,P. Cannarsa,M. Capell,D. Casadei,J. Casaus,G. Castellini,Y. H. Chang,H. S. Chen,Z.G. Chen,N.A. Chernoplekov,A. Chiarini,Tzihong Chiueh,Y.L. Chuang,Federico Cindolo,V. Commichau,A. Contin,A. Cotta-Ramusino,P. Crespo,Markus Cristinziani,J. P. Da Cunha,T. S. Dai,Jorge Dias de Deus,L.K. Ding,N. Dinu,L. Djambazov,I. D'Antone,Z.R. Dong,E. Emonet,F. J. Eppling,T. Eronen,G. Esposito,P. Extermann,J. Favier,C.C. Feng,E. Fiandrini,Fabio Finelli,Peter H. Fisher,R. Flaminio,G. Fluegge,N. Fouque,Yu. Galaktionov,Yu. Galaktionov,Massimo Gervasi,P. Giusti,W.K. Gu,T.G. Guzik,K. Hangarter,A. Hasan,V. Hermel,H. Hofer,M. A. Huang,W. Hungerford,M. Ionica,R. Ionica,J. Isbert,M. Jongmanns,W. Karpinski,G. Kenney,Jose Maria Kenny,W. Kim,A. Klimentov,A. Klimentov,J. Krieger,R. Kossakowski,V. Koutsenko,V. Koutsenko,G. Laborie,Timo Laitinen,G. Lamanna,G. Laurenti,A. Lebedev,S.C. Lee,Giuseppe Levi,P. Levtchenko,T.P. Li,C.L. Liu,H.T. Liu,M. Lolli,I. Lopes,G. Lu,Y. S. Lu,K. Luebelsmeyer,D. Luckey,Werner Lustermann,G. Maehlum,C. Maña,Anselmo Margotti,F. Massera,F. Mayet,R. R. McNeil,B. Meillon,Mauro Menichelli,F. Mezzanotte,Raffaele Mezzenga,A. Mihul,G. Molinari,A. Mourao,Ari Mujunen,F. Palmonari,G. Pancaldi,A. Papi,Inkyu Park,M. Pauluzzi,Felicitas Pauss,E. Perrin,A. Pesci,A. Pevsner,R. Pilastrini,M. Pimenta,V. Plyaskin,V. Pojidaev,H. Postema,E. Prati,Nicolas Produit,P. G. Rancoita,D. Rapin,F. Raupach,S. Recupero,D. Ren,Zhuoxiang Ren,M. Ribordy,J.P. Richeux,E. Riihonen,J. Ritakari,U. Roeser,C. Rossin,Roald Z. Sagdeev,D. Santos,G. Sartorelli,A. Schultz von Dratzig,G. Schwering,V. Shoutko,E. Shoumilov,R. Siedling,Dong-Chul Son,Tao Song,M. Steuer,G.S. Sun,H. Suter,X. W. Tang,Samuel C.C. Ting,S. M. Ting,F. Tenbusch,G. Torromeo,J. J. Torsti,J. Truemper,J. Ulbricht,S. Urpo,Ilya Usoskin,Eino Valtonen,J. Vandenhirtz,E. P. 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,Jing Wang,Yun Wang,J.P. Wefel,E.A. Werner,Ciaran Williams,S. X. Wu,S. X. Wu,P.C. Xia,J.L. Yan,L.G. Yan,C. G. Yang,M. Yang,P. Yeh,Hao Zhang,D.X. Zhao,G.Y. Zhu,W.Z. Zhu,H.L. Zhuang,Antonino Zichichi +215 more
TL;DR: The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km as mentioned in this paper.
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Production and propagation of cosmic ray positrons and electrons
An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,G. De Rosa,N. De Simone,V. Di Felice,A. M. Galper,L. A. Grishantseva,Petter Hofverberg,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,Silvio Orsi,G. Osteria,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,M. Simon,Roberta Sparvoli,Piero Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +50 more
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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