L. Quadrani
University of Bologna
15 Papers
54 Citations
L. Quadrani is an academic researcher from University of Bologna. The author has contributed to research in topics: Cosmic ray & Heliosphere. The author has an hindex of 13, co-authored 15 publications.
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Papers
Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station
M. Aguilar,D. Aisa,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,Gabriele 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,F. Cervelli,M. J. Chae,Yuan-Hann Chang,A. I. Chen,Huan Chen,G. M. Cheng,H. S. Chen,Lin Cheng,A. Chikanian,H. Y. Chou,E. Choumilov,V. Choutko,C. H. Chung,C. Clark,R. Clavero,G. Coignet,C. Consolandi,A. Contin,Claudio Corti,B. Coste,Z. Cui,M. Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,L. Di Masso,F. Dimiccoli,C. Díaz,P. von Doetinchem,W. J. Du,M. Duranti,D. D'Urso,A. Eline,Fj Eppling,T. Eronen,Y. Y. Fan,L. Farnesini,J. Feng,E. Fiandrini,A. Fiasson,E. Finch,Peter H. Fisher,Yu. Galaktionov,G. Gallucci,B. García,R. J. García-López,H. Gast,I. Gebauer,Massimo Gervasi,A. Ghelfi,W. Gillard,F. Giovacchini,P. Goglov,J. Gong,Corinne Goy,Varlen Grabski,D. Grandi,M. Graziani,C. Guandalini,I. Guerri,K. H. Guo,M. Habiby,Sadakazu Haino,K. C. Han,Z. H. He,Michael Heil,J. Hoffman,Timothy H. Hsieh,Zhiqi Huang,Changgi Huh,M. Incagli,M. Ionica,W. Y. Jang,H. Jinchi,K. Kanishev,Gui Nyun Kim,Kwangsoo Kim,T. Kirn,R. Kossakowski,O. Kounina,Andrei Kounine,V. Koutsenko,M. S. Krafczyk,S. Kunz,G. La Vacca,Elisa Laudi,G. Laurenti,Ignazio Lazzizzera,A. Lebedev,H. T. Lee,Shih-Chang Lee,C. Leluc,Haifeng Li,Jinglai Li,Qiang Li,T. X. Li,Wei Li,Yongyao Li,Z. H. Li,Z. Y. Li,S. Lim,Chia-Hui Lin,P. Lipari,Thomas Lippert,Dong Liu,Hengchang Liu,Teimuraz Lomtadze,M. J. Lu,Ying Lu,K. Luebelsmeyer,F. Luo,J. Z. Luo,S. S. Lv,R. D. Majka,Alexander Malinin,C. Maña,J. C. Marin,Tim Martin,German 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,Alberto Papi,E. Pedreschi,S. Pensotti,Rodrigo Araujo Pereira,Fabrizio Giulio Luca Pilo,A. Piluso,C. Pizzolotto,V. Plyaskin,M. Pohl,V. Poireau,E. Postaci,Antje Putze,L. Quadrani,X. M. Qi,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,Stefan Schael,S. M. Schmidt,D. Schuckardt,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,Wei 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,M. Velasco,J. P. Vialle,Liqiu Wang,Q. L. Wang,Ruiguang Wang,Xiaoping Wang,Zheng Wang,Z. L. Weng,K. Whitman,J. Wienkenhöver,H. Wu,X. Xia,M. Xie,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. H. Zhang,M. T. Zhang,X. B. Zhang,Zhen Zhang,Z. M. Zheng,H. L. Zhuang,V. Zhukov,A. Zichichi,N. Zimmermann,Paolo Zuccon,C. Zurbach +279 more
TL;DR: In this paper, the Alpha Magnetic Spectrometer on the International Space Station was used to measure the primary cosmic-ray electron flux in the range 0.5 to 700 GeV and the positron flux in a range of 0.1 to 500 GeV.
The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II - Results from the first seven years
M. Aguilar,L. Ali Cavasonza,G. Ambrosi,Luísa Arruda,N. Attig,F. Barao,L. Barrin,A. Bartoloni,S. Başeğmez-du Pree,J. Bates,Roberto Battiston,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,Veronica Bindi,W. De Boer,K. Bollweg,B. Borgia,Matteo Boschini,M. Bourquin,E F Bueno,J. D. Burger,W. J. Burger,S. Burmeister,X. D. Cai,M. Capell,J. Casaus,G. Castellini,F. Cervelli,Yung Huang Chang,Yung Huang Chang,Guo-Ming Chen,H. S. Chen,Y. Chen,Lin Cheng,H. Y. Chou,S. Chouridou,V. Choutko,C. H. Chung,C. Clark,G. Coignet,C. Consolandi,Andrea Contin,Claudio Corti,Z. Cui,K. Dadzie,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,V. Di Felice,Carlos Díaz,F. Dimiccoli,P. von Doetinchem,F. Dong,F. Donnini,M. Duranti,A. Egorov,A. Eline,Jonathan L. Feng,E. Fiandrini,P. H. Fisher,V. Formato,C. Freeman,Yu. Galaktionov,C. Gámez,R. J. García-López,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,Massimo Gervasi,F. Giovacchini,D M Gómez-Coral,J. Gong,Corinne Goy,Varlen Grabski,D. Grandi,D. Grandi,M. Graziani,K. H. Guo,Sadakazu Haino,K. C. Han,R. K. Hashmani,Z. H. He,Bernd Heber,Timothy H. Hsieh,Jun Hu,Zhiqi Huang,W. Hungerford,M. Incagli,W. Y. Jang,Yi Jia,H. Jinchi,K. Kanishev,B. Khiali,G. N. Kim,T. Kirn,M. Konyushikhin,O. Kounina,Andrei Kounine,V. Koutsenko,A. Kuhlman,A. Kulemzin,G. La Vacca,G. La Vacca,Elisa Laudi,G. Laurenti,Ignazio Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,J. Q. Li,M. Li,Qiang Li,S. Li,T. X. Li,Z. H. Li,C. Light,Chia-Hui Lin,Thomas Lippert,Z Liu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,J. Z. Luo,S. S. Lyu,F. Machate,C. Mañá,Julio C. Marín,J. Marquardt,T. Martin,G. Martinez,N. Masi,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,D. C. Mo,M. Molero,P. Mott,L Mussolin,J. Q. Ni,N. Nikonov,F. Nozzoli,A.I. Oliva,M. Orcinha,M. Palermo,F. Palmonari,M. Paniccia,A. Pashnin,M. Pauluzzi,S. Pensotti,S. Pensotti,H. D. Phan,V. Plyaskin,M. Pohl,S. Porter,X. M. Qi,X. Qin,Z. Y. Qu,L. Quadrani,Pier-Giorgio Rancoita,D. Rapin,A. Reina Conde,A. Reina Conde,S. Rosier-Lees,A. Rozhkov,D. Rozza,D. 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,C. Solano,J. W. Song,R. Sonnabend,Qie Sun,Zhen Sun,Mauro Tacconi,Mauro Tacconi,X. W. Tang,Zhixiang Tang,J Tian,Samuel C.C. Ting,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Tüysüz,T. Urban,Ilya Usoskin,V Vagelli,Rami Vainio,E. Valente,Eino Valtonen,M. Vazquez Acosta,M. Vazquez Acosta,M. Vecchi,Mayda Velasco,J. P. Vialle,Liqiu Wang,Naihua Wang,Q. L. Wang,S Wang,Xiaoqun Wang,Zhao Wang,J Wei,Z. L. Weng,H. Wu,R. Q. Xiong,W Xu,Q. Yan,Y. Yang,H. Yi,Y. J. Yu,Z. Q. Yu,Mario Zannoni,Mario Zannoni,Chuanguo Zhang,Fan Zhang,Fajun Zhang,J. H. Zhang,Zhihua Zhang,F. Zhao,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,P. Zuccon +239 more
TL;DR: The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on the International Space Station (ISS) conducting a unique, long-duration mission of fundamental physics research in space as mentioned in this paper.
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Towards Understanding the Origin of Cosmic-Ray Electrons.
M. Aguilar,L. Ali Cavasonza,G. Ambrosi,Luísa Arruda,N. Attig,P. Azzarello,A. Bachlechner,F. Barao,A. Barrau,L. Barrin,A. Bartoloni,L. Basara,S. Başeğmez-du Pree,Roberto Battiston,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,Veronica Bindi,W. De Boer,K. Bollweg,B. Borgia,Matteo Boschini,M. Bourquin,E. F. Bueno,J. D. Burger,W. J. Burger,X. D. Cai,M. Capell,S. Caroff,J. Casaus,G. Castellini,F. Cervelli,Y. H. Chang,Guo-Ming Chen,H. S. Chen,Y. Chen,Lin Cheng,H. Y. Chou,V. Choutko,C. H. Chung,C. Clark,G. Coignet,C. Consolandi,Andrea Contin,Claudio Corti,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,A. Egorov,A. Eline,T. Eronen,Jonathan L. Feng,E. Fiandrini,P. H. Fisher,Valerio Formato,Yu. Galaktionov,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,Massimo Gervasi,F. Giovacchini,D. M. Gómez-Coral,J. Gong,Corinne Goy,Varlen Grabski,D. Grandi,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,M. Incagli,Yi Jia,H. Jinchi,K. Kanishev,B. Khiali,T. Kirn,C. Konak,O. Kounina,Andrei Kounine,V. Koutsenko,A. Kulemzin,G. La Vacca,G. La Vacca,Elisa Laudi,G. Laurenti,Ignazio Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,C. Leluc,J. Q. Li,Qiang Li,T. X. Li,Z. H. Li,C. Light,Chia-Hui Lin,Thomas Lippert,Frank Liu,Hu Liu,Hu Liu,Z Liu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,F. Luo,J. Z. Luo,Xi 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,D. C. Mo,M Molero,P. Mott,L Mussolin,T. J. N. Nelson,J. Q. Ni,N. Nikonov,F. Nozzoli,A. Oliva,M. Orcinha,M. Palermo,F. Palmonari,M. Paniccia,A. Pashnin,M. Pauluzzi,S. Pensotti,S. Pensotti,C. Perrina,H. D. Phan,N. Picot-Clemente,V. Plyaskin,M. Pohl,V. Poireau,A. Popkow,L. Quadrani,X. M. Qi,X. Qin,Z. Y. Qu,P. G. Rancoita,D. Rapin,A. Reina Conde,S. Rosier-Lees,A. Rozhkov,D. Rozza,D. Rozza,Roald Z. Sagdeev,C. Solano,S. Schael,S. M. Schmidt,A. Schulz von Dratzig,G. Schwering,Eun-Suk Seo,B. S. Shan,J. Y. Shi,T. Siedenburg,J. W. Song,Zhen Sun,Mauro Tacconi,Mauro Tacconi,X. W. Tang,Zhixiang Tang,J Tian,Samuel C.C. Ting,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,T. Urban,V Vagelli,E. Valente,Eino Valtonen,M. Vazquez Acosta,M. Vecchi,M. Vecchi,Mayda Velasco,J. P. Vialle,J Vizán,Liqiu Wang,Naihua Wang,Q. L. Wang,Xiaoqun Wang,X. Q. Wang,Zhao Wang,J Wei,Z. L. Weng,H. Wu,R. Q. Xiong,W. Xu,Q. Yan,Yang Yang,H. Yi,Y. J. Yu,Z. Q. Yu,Mario Zannoni,Mario Zannoni,S. Zeissler,Chuanguo Zhang,Fan Zhang,J. H. Zhang,Zhihua Zhang,F. Zhao,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,P. Zuccon +236 more
TL;DR: In this article, the authors presented precision results on cosmic-ray electrons in the energy range from 0.5 to 1.4, based on 28.1×106 electrons collected by the Alpha Magnetic Spectrometer on the International Space Station.
Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer
M. Aguilar,L. Ali Cavasonza,G. Ambrosi,Luísa Arruda,N. Attig,F. Barao,L. Barrin,A. Bartoloni,S. Başeğmez-du Pree,Roberto Battiston,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,Veronica Bindi,W. De Boer,K. Bollweg,B. Borgia,Matteo Boschini,M. Bourquin,E F Bueno,J. D. Burger,W. J. Burger,S. Burmeister,X. D. Cai,M. Capell,J. Casaus,G. Castellini,F. Cervelli,Yung Huang Chang,Guo-Ming Chen,H. S. Chen,Y. Chen,Lin Cheng,H. Y. Chou,S. Chouridou,V. Choutko,C. H. Chung,C. Clark,G. Coignet,C. Consolandi,Andrea Contin,Claudio Corti,Z. Cui,K. Dadzie,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,V. Di Felice,Carlos Díaz,F. Dimiccoli,P. von Doetinchem,F. Dong,F. Donnini,M. Duranti,A. Egorov,A. Eline,Jonathan L. Feng,E. Fiandrini,P. H. Fisher,V. Formato,C. Freeman,Yu. Galaktionov,C. Gámez,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,F. Giovacchini,D M Gómez-Coral,J. Gong,Corinne Goy,Varlen Grabski,D. Grandi,M. Graziani,K. H. Guo,Sadakazu Haino,K. C. Han,R. K. Hashmani,Z. H. He,Bernd Heber,Timothy H. Hsieh,Jun Hu,Zhiqi Huang,M. Incagli,W. Y. Jang,Yi Jia,H. Jinchi,K. Kanishev,B. Khiali,G. N. Kim,T. Kirn,M. Konyushikhin,O. Kounina,Andrei Kounine,V. Koutsenko,A. Kuhlman,A. Kulemzin,G. La Vacca,Elisa Laudi,G. Laurenti,Ignazio Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,J. Q. Li,M. Li,Qiang Li,S. Li,T. X. Li,Z. H. Li,C. Light,Chia-Hui Lin,Thomas Lippert,Z Liu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,J. Z. Luo,S. S. Lyu,F. Machate,C. Mañá,Julio C. Marín,J. Marquardt,T. Martin,G. Martinez,N. Masi,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,D. C. Mo,M. Molero,P. Mott,L Mussolin,J. Q. Ni,N. Nikonov,F. Nozzoli,A.I. Oliva,M. Orcinha,M. Palermo,F. Palmonari,M. Paniccia,A. Pashnin,M. Pauluzzi,S. Pensotti,H. D. Phan,R Piandani,V. Plyaskin,Stepan Poluianov,X. M. Qi,X. Qin,Z. Y. Qu,L. Quadrani,Pier-Giorgio Rancoita,D. Rapin,A. Reina Conde,S. Rosier-Lees,A. Rozhkov,D. 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,C. Solano,R. Sonnabend,J. W. Song,Qie Sun,Zhen Sun,Mauro Tacconi,X. W. Tang,Zhixiang Tang,J Tian,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Tüysüz,T. Urban,Ilya Usoskin,V Vagelli,Rami Vainio,E. Valente,Eino Valtonen,M. Vazquez Acosta,M. Vecchi,Mayda Velasco,J. P. Vialle,C. Wallmann,Liqiu Wang,Naihua Wang,Q. L. Wang,S Wang,Xiaoqun Wang,Zhao Wang,J Wei,Z. L. Weng,H. Wu,R. Q. Xiong,W. Xu,Q. Yan,Yuh-Shyong Yang,H. Yi,Y. J. Yu,Z. Q. Yu,Mario Zannoni,Chuanguo Zhang,Fan Zhang,Fajun Zhang,J. H. Zhang,Zhihua Zhang,F. Zhao,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,Paolo Zuccon +226 more
TL;DR: The observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.65 GV shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary Cosmic rays.
Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ⩽ 28 with the GalProp-HelMod Framework.
Matteo Boschini,S. Della Torre,Massimo Gervasi,D. Grandi,G. Jóhannesson,G. La Vacca,N. Masi,Igor V. Moskalenko,S. Pensotti,Troy A. Porter,L. Quadrani,Pier-Giorgio Rancoita,D. Rozza,Mauro Tacconi +13 more
TL;DR: In this article, a fraction of HEAO-3-C2 data was used together with ACE-CRIS data to make predictions for the local interstellar spectra (LIS) of nuclei that are not yet released by AMS-02.
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