The PAMELA experiment had operated almost ten years on board of the Resurs DK1 satellite. The satellite was launched on the 15tℎ of June 2006 and placed in orbit with an inclination of 70° and an altitude of 350 to 610 km. The experiment had continuously measured electron and positron fluxes of Galactic cosmic rays in a wide energy range from about 50 MeV to hundreds of GeV. The spectra of electrons have been analysed from the end of 23rd until the beginning of 24tℎ solar cycle including the prolonged deep solar minimum period from 2006 to the end of 2009 and the solar magnetic polarity reversal period in 2012-2014. Here, we present updated annual electron spectra from 2006 to 2015.
Study of the modulation of Galactic positrons and electrons in 2006-2016 with the PAMELA Experiment / Mikhailov V.V.; Aleksandrin S.Y.; Koldobskiy S.A.; Boezio M.; Munini R.; Aslam O.P.M.; Bisschoff D.; Ngobeni M.D.; Potgieter M.S.; Adriani O.; Barbarino G.; Bazilevskaya G.A.; Bellotti R.; 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.; Koldashov S.V.; Koldobskiy S.A.; Kvashnin A.N.; Leonov A.; Malakhov V.V.; Marcelli L.; Marcelli N.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mikhailov V.V.; Mocchiutti E.; Monaco A.; Mori N.; Lenni A.; 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. - 395:(2022), pp. 1307.1-1307.8.
Study of the modulation of Galactic positrons and electrons in 2006-2016 with the PAMELA Experiment
Adriani O.;Bongi M.;
2022
Abstract
The PAMELA experiment had operated almost ten years on board of the Resurs DK1 satellite. The satellite was launched on the 15tℎ of June 2006 and placed in orbit with an inclination of 70° and an altitude of 350 to 610 km. The experiment had continuously measured electron and positron fluxes of Galactic cosmic rays in a wide energy range from about 50 MeV to hundreds of GeV. The spectra of electrons have been analysed from the end of 23rd until the beginning of 24tℎ solar cycle including the prolonged deep solar minimum period from 2006 to the end of 2009 and the solar magnetic polarity reversal period in 2012-2014. Here, we present updated annual electron spectra from 2006 to 2015.
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