PoS - Proceedings of Science
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, N. Zampa
*corresponding author
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Pre-published on: July 22, 2019
Published on:
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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