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Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

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

in Astrophysics / Cosmic rays / Cosmology / Earth polar orbit / Electron flux / Electrons / Magnetic polarity / Magnetic spectrometers / Orbits / Physics / Polar orbits / Positrons / Solar magnetic field / Solar magnetic fields / Temporal variation / Wide energy range

2017

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Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

2017

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Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

2017

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Journal Article

Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

Marcelli, L,

De Santis, C,

Kvashnin, A N,

Bogomolov, E A,

Mikhailov, V V,

Vacchi, A,

Galper, A M,

Boezio, M,

Leonov, A A,

Casolino, M,

Picozza, P,

Vannuccini, E,

Panico, B,

Koldobsky, S,

Bellotti, R,

Krutkov, S Yu,

Mayorov, A G,

Menn, W,

Palma, F,

Di Felice, V.,

Merge, M,

Bottai, S,

De Simone, N,

Zampa, N,

Zampa, G,

Bongi, M,

Martucci, M,

Voronov, S A,

Barbarino, G,

Ricciarini, S B,

Malakhov, V V,

Bazilevskaya, G A,

Stozhkov, Yu I,

Bonvicini, V,

Mocchiutti, E,

Carlson, P,

Vasiliev, G I,

Campana, D,

Koldashov, S V,

Yurkin, Yu T,

Monaco, A,

Sparvoli, R,

Adriani, O,

Ricci, M,

Papini, P,

Pearce, M,

Spillantini, P,

Munini, R,

Bruno, A,

Cafagna, F S,

Osteria, G,

Castellini, G,

Simon, M,

De Donato, C.,

Karelin, A V,

Mori, N.

2017

Overview

Magnetic spectrometer PAMELA was launched onboard a satellite Resurs-DK1 into low-Earth polar orbit with altitude 350-600 km to study cosmic ray antiparticle fluxes in a wide energy range from ∼ 100 MeV to hundreds GeV. This paper presents the results of observations of temporal variations of the positron and electron fluxes in the 2006-2015. The ratio of the positron and electron fluxes below 2 GV shows sharp increasing since 2014 due to changing of the polarity of the solar magnetic field.

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