Cosmic Ray Electron and Positron Spectrum with the PAMELA Experiment

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

doi:10.22323/1.358.0108

Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - CRD - Cosmic Ray Direct

Cosmic Ray Electron and Positron Spectrum with the PAMELA Experiment

V. Mikhailov*, O. Adriani, G. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, M. Bongi, V. Bonvicini, A. Bruno, F. S. Cafagna, D. Campana, P. Carlson, M. Casolino, G. Castellini, C. De Santis, V. Di Felice, A. M. Galper, A. V. Karelin, S. V. Koldashov, S. A. Koldobsky, A. A. Kvashnin, A. N. Kvashnin, A. A. Leonov, V. V. Malakhov, L. Marcell, M. Martucci, A. G. Mayorov, W. Menn, M. Mergé, E. Mocchiutti, A. Monaco, N. Mori, R. Munin, G. Osteria, P. Papini, B. Panico, M. Pearce, P. Picozza, M. Ricci, S. B. Ricciarini, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, I. Vasilyev, S. A. Voronov, Y. T. Yurkin, G. Zampa and N. Zampaet al. (click to show)

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Pre-published on: July 22, 2019

Published on: July 02, 2021

Abstract

The PAMELA magnetic spectrometer, located on board the Resurs-DK1 satellite on Earth polar orbit with altitude of 350-600 km, measured the fluxes of cosmic ray particles and antiparticles in a wide energy range from ~ 50 MeV to several TeVs. In this paper new results on the "all-electron" (sum electrons and positrons) spectrum are presented. New improved analysis on the full data set from 2006 to 2016 allows a significant increase in statistic compared to previously published results and an extension of energy interval up to ~1 TeV

DOI: https://doi.org/10.22323/1.358.0108

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