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 and N. Zampaet al. (click to show)
Full text: pdf
Pre-published on: July 22, 2019
Published on: July 02, 2021
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
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.