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Study of the modulation of Galactic positrons and electrons in 2006-2016 with the PAMELA Experiment
National Research Nuclear University MEPhI, 31 Kashirskoe shosse, Moscow. Russia, 31 Kashirskoe shosse.
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, Sweden.ORCID iD: 0000-0003-2137-2922
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. The Oskar Klein Centre for Cosmoparticle Physics, Sweden.ORCID iD: 0000-0001-7011-7229
INFN, Sezione di Trieste, I-34149 Trieste, Italy.
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Number of Authors: 572022 (English)In: 37th International Cosmic Ray Conference, ICRC 2021, Sissa Medialab Srl , 2022, article id 1307Conference paper, Published paper (Refereed)
Abstract [en]

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.

Place, publisher, year, edition, pages
Sissa Medialab Srl , 2022. article id 1307
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-350638Scopus ID: 2-s2.0-85124969495OAI: oai:DiVA.org:kth-350638DiVA, id: diva2:1884515
Conference
37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, Germany, Jul 12 2021 - Jul 23 2021
Note

QC 20240717

Available from: 2024-07-17 Created: 2024-07-17 Last updated: 2024-07-17Bibliographically approved

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Carlson, PerPearce, Mark

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