Modulation of electrons and positrons in 2006–2015 in the PAMELA experiment

V. V. Mikhailov; O. Adriani; G. A. Bazilevskaya; G. C. Barbarino; R. Bellotti; E. A. Bogomolov; M. Boezio; V. Bonvicini; M. Bongi; S. Bottai; A. Bruno; A. Vacchi; E. Vannuccini; G. I. Vasilyev; S. A. Voronov; A. M. Galper; C. De Santis; V. Di Felice; G. Zampa; N. Zampa; M. Casolino; D. Campana; A. V. Karelin; P. Carlson; G. Castellini; F. Cafagna; A. A. Kvashnin; A. N. Kvashnin; S. V. Koldashov; S. A. Koldobskiy; S. Y. Krutkov; A. A. Leonov; A. G. Mayorov; V. V. Malakhov; M. Martucci; L. Marcelli; W. Menn; M. Merge; E. Mocchiutti; A. Monaco; N. Mori; R. Munini; G. Osteria; B. Panico; P. Papini; P. Picozza; M. Pearce; M. Ricci; S. B. Ricciarini; M. F. Runtso; M. Simon; R. Sparvoli; P. Spillantini; Y. I. Stozhkov; Y. T. Yurkin

doi:10.3103/S1062873817020277

Modulation of electrons and positrons in 2006–2015 in the PAMELA experiment

Authors: Mikhailov V.V.¹, Adriani O.²^,3, Bazilevskaya G.A.⁴, Barbarino G.C.²^,5, Bellotti R.²^,6, Bogomolov E.A.⁷, Boezio M.⁸, Bonvicini V.⁸, Bongi M.²^,3, Bottai S.³, Bruno A.²^,6, Vacchi A.⁸^,9, Vannuccini E.³, Vasilyev G.I.⁷, Voronov S.A.¹, Galper A.M.¹, De Santis C.¹⁰^,2, Di Felice V.¹⁰^,11, Zampa G.⁸, Zampa N.⁸, Casolino M.¹⁰, Campana D.⁵, Karelin A.V.¹, Carlson P.²^,12, Castellini G.¹³, Cafagna F.⁶, Kvashnin A.A.⁴, Kvashnin A.N.⁴, Koldashov S.V.¹, Koldobskiy S.A.¹, Krutkov S.Y.⁷, Leonov A.A.¹, Mayorov A.G.¹, Malakhov V.V.¹, Martucci M.²^,14, Marcelli L.², Menn W.², Merge M.¹⁰^,2, Mocchiutti E.⁸, Monaco A.²^,6, Mori N.³, Munini R.⁸^,2, Osteria G.⁵, Panico B.⁵, Papini P.³, Picozza P.¹⁰^,2, Pearce M.²^,12, Ricci M.¹⁴, Ricciarini S.B.³, Runtso M.F.¹, Simon M.², Sparvoli R.¹⁰^,2, Spillantini P.¹, Stozhkov Y.I.⁴, Yurkin Y.T.¹
Affiliations:
1. National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
2. Department of Physics
3. INFN, Sezione di Florence
4. Lebedev Physical Institute
5. INFN, Sezione di Naples
6. INFN, Sezione di Bari
7. Ioffe Institute
8. INFN, Sezione di Trieste
9. Department of Mathematics and Informatics
10. INFN, Sezione di Rome Tor Vergata
11. Agenzia Spaziale Italiana (ASI) Science Data Center
12. Oskar Klein Centre for Cosmoparticle Physics
13. IFAC
14. Laboratori Nazionali di Frascati
Issue: Vol 81, No 2 (2017)
Pages: 154-156
Section: Proceedings of the 34th All-Russian Conference on Cosmic Rays
URL: https://journals.rcsi.science/1062-8738/article/view/184955
DOI: https://doi.org/10.3103/S1062873817020277
ID: 184955

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The PAMELA magnetic spectrometer was launched aboard the Resurs DK-1 satellite into a nearpolar circumterrestrial orbit with an altitude of 350–600 km to study fluxes of the particles and antiparticles of cosmic rays in the wide energy range of ~80 MeV to several hundred gigaelectronvolts. The results from observations of temporal variations in electron and positron fluxes in 2006–2015 are presented. The ratio of electron and positron fluxes measured in this time interval reveals a dependence on the rigidity of particles, the solar activity, and the polarity of the solar magnetic field.

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Modulation of electrons and positrons in 2006–2015 in the PAMELA experiment

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Abstract

About the authors

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