Journal ArticleDOI
The global modulation of cosmic rays during a quiet heliosphere: A modeling perspective
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In this paper, a perspective is given of the solar modulation of galactic cosmic rays in the heliosphere during the extraordinary quiet solar minimum period from 2006 to 2009, and the results from comprehensive modeling are discussed.About:
This article is published in Advances in Space Research.The article was published on 2017-08-15. It has received 53 citations till now. The article focuses on the topics: Cosmic ray & Heliosphere.read more
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In Situ Observations of Interstellar Plasma With Voyager 1 (Invited)
TL;DR: Electron densities detected by Voyager 1 show that the spacecraft is in the interstellar plasma, and other observations provide strong evidence that Voyager 1 has crossed the heliopause into the nearby interstellar plasma.
Journal ArticleDOI
Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station.
M. Aguilar,L. Ali Cavasonza,Giovanni Ambrosi,Luísa Arruda,N. Attig,S. Aupetit,P. Azzarello,A. Bachlechner,F. Barao,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,S. Başeğmez-du Pree,Markus Battarbee,Roberto Battiston,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,Bruna Bertucci,K. F. Bindel,Veronica Bindi,W. De Boer,K. Bollweg,V. Bonnivard,B. Borgia,Matteo Boschini,M. Bourquin,E. F. Bueno,J. D. Burger,Franck Cadoux,X. D. Cai,M. Capell,S. Caroff,J. Casaus,G. Castellini,F. Cervelli,M. J. Chae,Yuan-Hann Chang,A. I. Chen,Guo-Ming Chen,H. S. Chen,Y. 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,W. Creus,M. Crispoltoni,Z. Cui,K. Dadzie,Yaomin Dai,A. Datta,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,Jonathan L. Feng,E. Fiandrini,P. H. Fisher,Valerio Formato,Yu. Galaktionov,G. Gallucci,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,F. Giovacchini,D. M. Gómez-Coral,J. Gong,C. Goy,Varlen Grabski,D. Grandi,M. Graziani,K. H. Guo,Sadakazu Haino,K. C. Han,Z. H. He,Matthias Heil,Timothy H. Hsieh,H. P. Huang,Zhiqi Huang,Changgi Huh,M. Incagli,Maria Ionica,W. Y. Jang,Yi Jia,H. Jinchi,S. C. Kang,K. Kanishev,B. Khiali,G. N. Kim,Kwangsoo Kim,T. Kirn,C. Konak,O. Kounina,Andrei Kounine,V. Koutsenko,A. Kulemzin,G. La Vacca,Elisa Laudi,G. Laurenti,I. Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,Hui Li,J. Q. Li,Qiang Li,T. X. Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,D. Liu,Hu Liu,V. D. Lordello,S. Q. Lu,Ying Lu,K. Luebelsmeyer,F. Luo,J. Z. Luo,S. S. Lyu,F. Machate,C. Mañá,Julio C. Marín,T. Martin,G. Martinez,N. Masi,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,V. M. Mikuni,D. C. Mo,P. Mott,T. J. N. Nelson,J. Q. Ni,N. Nikonov,F. Nozzoli,A.I. Oliva,M. Orcinha,M. Palermo,F. Palmonari,C. Palomares,M. Paniccia,M. Pauluzzi,S. Pensotti,C. Perrina,H. D. Phan,N. Picot-Clemente,Fabrizio Giulio Luca Pilo,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,Lucio Quadrani,X. M. Qi,X. Qin,Z. Y. Qu,T. Räihä,P. G. Rancoita,D. Rapin,J. S. Ricol,S. Rosier-Lees,A. Rozhkov,Davide Rozza,Roald Z. Sagdeev,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,Mauro Tacconi,X. W. Tang,Zhixiang Tang,D. Tescaro,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Türkoğlu,T. Urban,Valerio Vagelli,E. Valente,Eino Valtonen,M. Vazquez Acosta,Manuela Vecchi,Mayda Velasco,J. P. Vialle,Liqiu Wang,Naihua Wang,Q. L. Wang,Xiaoqun Wang,X. Q. Wang,Zhao Wang,C. C. Wei,Z. L. Weng,K. Whitman,H. Wu,Xin Wu,R. Q. Xiong,W. Xu,Q. Yan,J. Yang,Mingming Yang,Yang Yang,H. Yi,Y. J. Yu,Z. Q. Yu,Mario Zannoni,S. Zeissler,Chuanguo Zhang,Fan Zhang,J. Zhang,J. H. Zhang,Shihao Zhang,Zhihua Zhang,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,Paolo Zuccon +251 more
TL;DR: High-statistics, precision measurements of the detailed time and energy dependence of the primary cosmic-ray electron flux and positron flux over 79 Bartels rotations from May 2011 to May 2017 in the energy range from 1 to 50 GeV show that the ratio exhibits a smooth transition over 830±30 days from one value to another.
Journal ArticleDOI
Proton fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for the 24th solar cycle
Matteo Martucci,Riccardo Munini,Mirko Boezio,V. Di Felice,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,P. Carlson,Marco Casolino,G. Castellini,C. De Santis,A. M. Galper,A. V. Karelin,S. V. Koldashov,Sergey Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,L. Marcelli,N. Marcelli,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti A. Monaco,Nicola Mori,G. Osteria,Beatrice Panico,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,M. Simon,R. Sparvoli,P. Spillantini,Y. I. Stozhkov,A. Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,M. S. Potgieter,Jan-Louis Raath +53 more
TL;DR: In this article, the PAMELA experiment was used to measure the time-dependent intensity of galactic cosmic ray proton spectra over a wide energy range (0.08-50 GeV) from a minimum to a maximum period of solar activity.
Journal ArticleDOI
Proton fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for solar cycle 24
Matteo Martucci,Riccardo Munini,Mirko Boezio,V. Di Felice,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,Per Carlson,Marco Casolino,G. Castellini,C. De Santis,A. M. Galper,A. V. Karelin,Sergey Koldashov,Sergey Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,L. Marcelli,N. Marcelli,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,G. Osteria,Beatrice Panico,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,M. Simon,R. Sparvoli,P. Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Yu. T. Yurkin,G. Zampa,N. Zampa,M. S. Potgieter,Jan-Louis Raath +54 more
TL;DR: In this paper, the time-dependent intensity of the low-energy (approximately 50 GeV) galactic cosmic rays (GCRs) was measured and the models that describe their propagation inside the galaxy were improved.
Journal ArticleDOI
New Very Local Interstellar Spectra for Electrons, Positrons, Protons, and Light Cosmic Ray Nuclei
TL;DR: In this article, the authors used the most comprehensive galactic propagation model (GALPROP) along with a sophisticated solar modulation model to compare the computed spectra with the observed PAMELA spectra over a wide energy range.
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The passage of energetic charged particles through interplanetary space
TL;DR: In this article, a general expression for the particle diffusion coefficient kij, including both scattering in magnetic irregularities and systematic pressure drifts, was derived from the condition that energetic solar particles in interplanetary space random walk in the irregularities in the large-scale inter-planetary magnetic field, and the observed fields show that the diffusion coefficient is of the order of 1021-1022 cm2/sec.
Journal ArticleDOI
First result from the Alpha Magnetic Spectrometer on the International Space Station: precision measurement of the positron fraction in primary cosmic rays of 0.5-350 GeV.
M. Aguilar,G Alberti,Behcet Alpat,A. Alvino,G. Ambrosi,K. Andeen,H. Anderhub,Luísa Arruda,Philipp Azzarello,A. Bachlechner,Fernando Barão,B. Baret,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,A. Basili,L Batalha,J. Bates,Roberto Battiston,J. Bazo,R. Becker,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,P. Berges,B. Bertucci,G. Bigongiari,Adrian Biland,Veronica Bindi,S. Bizzaglia,G. Boella,W. de Boer,K. Bollweg,J. Bolmont,B. Borgia,S. Borsini,Matteo Boschini,G. Boudoul,M. Bourquin,Pierre Brun,M Buénerd,J. D. Burger,W. J. Burger,Franck Cadoux,X. D. Cai,M. Capell,D. Casadei,J. Casaus,V. Cascioli,G. Castellini,I. Cernuda,F. Cervelli,M. J. Chae,Yuan-Hann Chang,A. I. Chen,C R Chen,H. S. Chen,G. M. Cheng,Huan Chen,Lin Cheng,N Chernoplyiokov,A. Chikanian,E. Choumilov,V. Choutko,C. H. Chung,C. Clark,R. Clavero,G. Coignet,V Commichau,C. Consolandi,Andrea Contin,Claudio Corti,M T Costado Dios,B. Coste,D. Crespo,Z. Cui,M. Dai,C. Delgado,S. Della Torre,B. Demirkoz,P. Dennett,L. Derome,S. Di Falco,X H Diao,A Diago,L. Djambazov,Carlos Díaz,P. von Doetinchem,W. J. Du,J.M. Dubois,R Duperay,M. Duranti,D D'Urso,A. Egorov,A. Eline,F. J. Eppling,T. Eronen,J. van Es,H. Esser,Alain Falvard,E. Fiandrini,A. Fiasson,E. Finch,Peter H. Fisher,K Flood,R Foglio,M Fohey,S Fopp,N. Fouque,Yu. Galaktionov,M. Gallilee,L Gallin-Martel,G. Gallucci,Bruce Rafael Mellado Garcia,Jmv Garcia,R. J. García-López,L García-Tabares,C Gargiulo,Henning Gast,I. Gebauer,Simonetta Gentile,Massimo Gervasi,W. Gillard,F. Giovacchini,L Girard,P. Goglov,J. Gong,C Goy-Henningsen,D. Grandi,M. Graziani,A Grechko,A Gross,I. Guerri,C. de la Guia,K. H. Guo,M. Habiby,Sadakazu Haino,F. Hauler,Z. H. He,Michael Heil,J Heilig,R. Hermel,H. Hofer,Zhiqi Huang,W Hungerford,M. Incagli,Maria Ionica,A. Jacholkowska,W. Y. Jang,H. Jinchi,M. Jongmanns,L Journet,L. Jungermann,Waclaw Karpinski,Gui Nyun Kim,Kwangsoo Kim,T. Kirn,R. Kossakowski,A. Koulemzine,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,E. Laudi,G. Laurenti,C Lauritzen,A. Lebedev,M W Lee,S. C. Lee,C. Leluc,H. León Vargas,V Lepareur,J. Q. Li,Qiang Li,T. X. Li,Wei Li,Z. H. Li,P. Lipari,Chia-Hui Lin,Dong Liu,Hengchang Liu,Teimuraz Lomtadze,Ying Lu,S Lucidi,K. Lübelsmeyer,J. Z. Luo,Werner Lustermann,S. S. Lv,Joseph R. Madsen,R. D. Majka,A. Malinin,C. Maña,J. C. Marin,Tim Martin,G. Martinez,F. Masciocchi,N. Masi,David Maurin,Al McInturff,Peter McIntyre,A. Menchaca-Rocha,Q. Meng,Mauro Menichelli,I Mereu,M Millinger,D. C. Mo,Marco Molina,P. Mott,Ari Mujunen,S Natale,P Nemeth,J. Q. Ni,N. Nikonov,F. Nozzoli,P. Nunes,A. Obermeier,S Oh,A. Oliva,F. Palmonari,C. Palomares,M. Paniccia,Alberto Papi,W H Park,M. Pauluzzi,Felicitas Pauss,A Pauw,E. Pedreschi,S. Pensotti,Rui Miguel Faisca Rodrigues Pereira,E. Perrin,G. Pessina,G. Pierschel,Fabrizio Giulio Luca Pilo,A. Piluso,C. Pizzolotto,V. Plyaskin,J Pochon,M. Pohl,V. Poireau,S. Porter,J Pouxe,Antje Putze,Lucio Quadrani,X N Qi,P. G. Rancoita,D. Rapin,Z. L. Ren,J. S. Ricol,E. Riihonen,I. Rodríguez,U. Roeser,S. Rosier-Lees,Leonardo Paolo Rossi,A. Rozhkov,Davide Rozza,A. Sabellek,Roald Z. Sagdeev,J. Sandweiss,B Santos,P. Saouter,M Sarchioni,Stefan Schael,D. Schinzel,M. Schmanau,G. Schwering,A. Schulz von Dratzig,G. Scolieri,Eun-Suk Seo,B. S. Shan,J. Y. Shi,Yun Shi,T. Siedenburg,R. Siedling,Dong-Chul Son,F. Spada,F. Spinella,M. Steuer,K Stiff,Won Kyu Calvin Sun,W. H. Sun,X H Sun,Mauro Tacconi,C. P. Tang,X. W. Tang,Zhixiang Tang,L. Tao,J Tassan-Viol,Samuel C.C. Ting,S. M. Ting,C Titus,Nicola Tomassetti,F Toral,J. J. Torsti,J R Tsai,J C Tutt,J. Ulbricht,T. Urban,V. Vagelli,E. Valente,C. Vannini,Eino Valtonen,M Vargas Trevino,S. S. Vaurynovich,M Vecchi,M. Vergain,B. Verlaat,C Vescovi,J. P. Vialle,G. Viertel,Giovanni Volpini,Dongfang Wang,Naihua Wang,Q. L. Wang,Ruiguang Wang,Xiaoping Wang,Zheng Wang,W. Wallraff,Z. L. Weng,M. Willenbrock,Michael Wlochal,H. Wu,K. Y. Wu,Z S Wu,Wenzhong Xiao,S. Xie,R. Q. Xiong,Gongming Xin,Ningsheng Xu,Wei Xu,Qing-Bo Yan,J. Yang,Mingming Yang,Q. H. Ye,H. Yi,Y. J. Yu,Z. Q. Yu,S. Zeissler,J G Zhang,Zhijun Zhang,M M Zhang,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,A. Zichichi,Paolo Zuccon,C. Zurbach +347 more
TL;DR: The very accurate data show that the positron fraction is steadily increasing from 10 to ∼ 250 GeV, but, from 20 to 250 GeV, the slope decreases by an order of magnitude, showing the existence of new physical phenomena.
Journal ArticleDOI
Solar modulation of galactic cosmic rays.
L. J. Gleeson,W. I. Axford +1 more
TL;DR: A brief description of the basic principles of and techniques which are used for describing the behavior of galactic cosmic rays in the solar wind is given in this article, where several numerical examples which illustrate features of the cosmic-ray behavior are presented.
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.
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