Electron and positron fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the international space station.

@article{Aguilar2014ElectronAP,
  title={Electron and positron fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the international space station.},
  author={Miguel Aguilar and D. Aisa and Antonio Alvino and Giovanni Ambrosi and Karen Andeen and L. Arruda and Norbert Attig and Philipp Azzarello and Andreas Bachlechner and Fernando Bar{\~a}o and Aur{\'e}lien Barrau and Laurence Barrin and Alessandro Bartoloni and Laurent Basara and Markus Battarbee and Roberto Battiston and J. L. Bazo and Uwe Becker and Matthew Daniel Behlmann and Bastian Beischer and Javier Berdugo and B. Bertucci and Gabriele Bigongiari and Veronica Bindi and Sauro Bizzaglia and M. Bizzarri and Giuliano Boella and Wim de Boer and Ken Bollweg and Vincent Bonnivard and Bruno Borgia and Serena Borsini and M. J. Boschini and Maurice Bourquin and Joseph Burger and Franck Cadoux and X. D. Cai and Mireia Br{\`o}via Capell and S. Caroff and Jorge Casaus and Vincenzo Cascioli and Giovanni Castellini and Ignacio Cernuda and Franco Cervelli and M. J. Chae and Y. H. Chang and A. I. Chen and Hsieh Chen and G. M. Cheng and H S Chen and L. Cheng and Alexei Chikanian and H. Y. Chou and E. Choumilov and Vitali Choutko and C. H. Chung and Chris Clark and R. Clavero and Nicolas Produit and Cristina Consolandi and Andrea Contin and Claudio Corti and B. Coste and Z. Cui and M. Dai and Carlos Delgado and Stefano Della Torre and Melahat Bilge Demirk{\"o}z and L. Derome and S. Di Falco and L Di Masso and Francesco Dimiccoli and Carlos Diaz and Philip von Doetinchem and Wenyan Du and Matteo Duranti and Domenico D'urso and A. Eline and Frederic J. Eppling and T. Eronen and Y. Y. Fan and L. Farnesini and J. Feng and E. Fiandrini and A. Fiasson and Evan Finch and P. H. Fisher and Yu. K. Galaktionov and Giovanni Gallucci and Bruce Rafael Mellado Garcia and R. Garcia-Lopez and Henning Gast and Iris Gebauer and M. Gervasi and A. Ghelfi and William Gillard and Francesca Giovacchini and P. Goglov and J. Gong and C. Goy and Varlen Grabski and D. Grandi and Maura Graziani and Cristina Guandalini and Irene Guerri and K. H. Guo and M. Habiby and Sadakazu Haino and K. C. Han and Z. H. He and Matthias Heil and Julia Hoffman and Timothy H. Hsieh and Z. C. Huang and Changgi Huh and M. Incagli and Maria Ionica and Wooyoung Jang and H. Jinchi and K. A. Kanishev and G. N. Kim and K. S. Kim and Thomas J. Kirn and R. Kossakowski and O. Kounina and Andrei Kounine and Vladimir Koutsenko and Matthew Scott Krafczyk and Simon Kunz and G. La Vacca and Elisa Laudi and Giuliano Laurenti and Ignazio Lazzizzera and Alexei Lebedev and H. T. Lee and S. C. Lee and Catherine Leluc and H L Li and J. Q. Li and Q Li and Q Li and T. X. Li and Wenyue Li and Yong-yao Li and Zh. Li and Z. Y. Li and S. I. Lim and C. H. Lin and Paolo Lipari and Th. Lippert and D Liu and Hengchuan Liu and Teimuraz Lomtadze and M. J. Lu and Y. S. Lu and K. Luebelsmeyer and Feng Luo and J. Z. Luo and S. S. Lv and R. Majka and Alexander Malinin and Carlos Ma{\~n}{\'a} and J-C. Marin and T. A. Martin and German Martinez and N. Masi and David Maurin and Arturo Alejandro Menchaca-rocha and Q. Meng and D. C. Mo and Luca Morescalchi and P. Mott and M. M{\"u}ller and J. Q. Ni and N. N. Nikonov and Francesco Nozzoli and P. Nunes and Andreas Alexander Obermeier and Alberto Oliva and Miguel Orcinha and Federico Palmonari and Carmen Palomares and Mercedes Paniccia and A. Papi and Elena Pedreschi and Simonetta Pensotti and Rui Pereira and Federico Pilo and A. Piluso and C. Pizzolotto and V. I. Plyaskin and Martin Pohl and V. Poireau and E. Postaci and Antje Putze and Lucio Quadrani and X. M. Qi and P. G. Rancoita and Divic Rapin and J-S. Ricol and I. Rodr{\'i}guez and S. Rosier-Lees and A. Rozhkov and Davide Rozza and Roal'd. Z. Sagdeev and Jack H. Sandweiss and Pierre Saouter and C. Sbarra and Stefan Schael and S. M. Schmidt and D. Schuckardt and A. Schulz von Dratzig and Gregor Schwering and G. Scolieri and E-S. Seo and B. S. Shan and Y. H. Shan and J. Y. Shi and X. Y. Shi and Y. M. Shi and Thorsten Siedenburg and D C Son and Francesca R. Spada and Franco Spinella and W. H. Sun and W. H. Sun and M. Tacconi and C. P. Tang and X. W. Tang and Z. C. Tang and Lian Tao and Diego Tescaro and Samuel C. C. Ting and S. M. Ting and N. Tomassetti and Jarmo Torsti and C. T{\"u}rkoğlu and T. Urban and V. Vagelli and Enzo Valente and Cristina Vannini and Eino Valtonen and Siarhei Vaurynovich and Manuela Vecchi and Miguel Angel Velasco and J. P. Vialle and L Q Wang and Q. L. Wang and R. S. Wang and Xirui Wang and Z. X. Wang and Zhili Weng and Kathryn Whitman and Jens Wienkenh{\"o}ver and H. Wu and X. M. Xia and M. Xie and S Xie and Runqun Xiong and Gong-Ming Xin and Ning-sheng Xu and W. Xu and Q. Yan and Joo Yun Yang and M Yang and Q. H. Ye and Han Yi and Y. J. Yu and Z. Q. Yu and Stefan Zeissler and J. H. Zhang and M. T. Zhang and Xiaoling Zhang and Zhiling Zhang and Z. M. Zheng and H L Zhuang and Valery Zhukov and Antonino Zichichi and N. Zimmermann and Paolo Zuccon and Christine Zurbach},
  journal={Physical review letters},
  year={2014},
  volume={113 12},
  pages={
          121102
        }
}
Precision measurements by the Alpha Magnetic Spectrometer on the International Space Station of the primary cosmic-ray electron flux in the range 0.5 to 700 GeV and the positron flux in the range 0.5 to 500 GeV are presented. The electron flux and the positron flux each require a description beyond a single power-law spectrum. Both the electron flux and the positron flux change their behavior at ∼30  GeV but the fluxes are significantly different in their magnitude and energy dependence… Expand

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