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.

Cosmic Ray Electron and Positron Spectrum with the PAMELA Experiment / Mikhailov V.V.; Adriani O.; Barbarino G.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bruno A.; Cafagna F.S.; Campana D.; Carlson P.; Casolino M.; Castellini G.; De Santis C.; Di Felice V.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobsky S.A.; Kvashnin A.A.; Kvashnin A.N.; Leonov A.A.; Malakhov V.V.; Marcelli L.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mocchiutti E.; Monaco A.; Mori N.; Munini R.; Osteria G.; Papini P.; Panico B.; Pearce M.; Picozza P.; Ricci M.; Ricciarini S.B.; Simon M.; Sparvoli R.; Spillantini P.; Stozhkov Yu.I.; Vacchi A.; Vannuccini E.; Vasiliev G.I.; Voronov S.A.; Yurkin Yu.T.; Zampa G.; Zampa N.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - ELETTRONICO. - 358:(2021), pp. 108.0-108.5.

Cosmic Ray Electron and Positron Spectrum with the PAMELA Experiment

Adriani O.;Bongi M.;Mori N.;Ricciarini S. B.;Vannuccini E.;
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.
2021
358
0
5
Mikhailov V.V.; Adriani O.; Barbarino G.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bruno A.; Cafagna F.S.; Campana D.; Carlson P.; Casolino M.; Castellini G.; De Santis C.; Di Felice V.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobsky S.A.; Kvashnin A.A.; Kvashnin A.N.; Leonov A.A.; Malakhov V.V.; Marcelli L.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mocchiutti E.; Monaco A.; Mori N.; Munini R.; Osteria G.; Papini P.; Panico B.; Pearce M.; Picozza P.; Ricci M.; Ricciarini S.B.; Simon M.; Sparvoli R.; Spillantini P.; Stozhkov Yu.I.; Vacchi A.; Vannuccini E.; Vasiliev G.I.; Voronov S.A.; Yurkin Yu.T.; Zampa G.; Zampa N.
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1285650
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