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Time dependence of the helium flux measured by PAMELA
Ist Nazl Fis Nucl, Sez Rome Tor Vergata, I-00133 Rome, Italy.;Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy..
KTH, School of Biotechnology (BIO), Centres, Albanova VinnExcellence Center for Protein Technology, ProNova. KTH, School of Engineering Sciences (SCI), Physics.
KTH, School of Engineering Sciences (SCI), Physics. KTH, School of Biotechnology (BIO), Centres, Albanova VinnExcellence Center for Protein Technology, ProNova.ORCID iD: 0000-0001-7011-7229
North West Univ, Ctr Space Res, ZA-2520 Potchefstroom, South Africa..
2019 (English)In: 7TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS (RICAP18) / [ed] DeVincenzi, M Capone, A Morselli, A, E D P SCIENCES , 2019, article id UNSP 01004Conference paper, Published paper (Refereed)
Abstract [en]

Precision measurements of the Z = 2 component in cosmic radiation provide crucial information about the origin and propagation of the second most abundant cosmic ray species in the Galaxy (9% of the total). These measurements, acquired with the PAMELA space experiment orbiting Earth, allow to study solar modulation in details. Helium modulation is compared to the modulation of protons to study possible dependencies on charge and mass. The time dependence of helium fluxes on a monthly basis measured by PAMELA has been studied for the period between July 2006 to January 2016 in the energy range from 800 MeV/n to similar to 20 GeV/n.

Place, publisher, year, edition, pages
E D P SCIENCES , 2019. article id UNSP 01004
Series
EPJ Web of Conferences, ISSN 2100-014X ; 209
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-267196DOI: 10.1051/epjconf/201920901004ISI: 000507538900004OAI: oai:DiVA.org:kth-267196DiVA, id: diva2:1391206
Conference
7th Roma International Conference on Astroparticle Physics (RICAP), SEP 04-07, 2018, Roma Tre Univ, Roma, ITALY
Note

QC 20200204

Available from: 2020-02-04 Created: 2020-02-04 Last updated: 2020-02-04Bibliographically approved

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