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

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

doi:10.3103/s1062873817020277

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

V V Mikhailov, M F Runtso + Show 53 more

https://doi.org/10.3103/s1062873817020277

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#Rigidity Of Particles #PAMELA Experiment + Show 8 more

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Abstract

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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