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Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.
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Number of Authors: 62
2011 (English)In: Bulletin of the Russian Academy of Sciences: Physics, ISSN 1062-8738, Vol. 75, no 6, 779-781 p.Article in journal (Refereed) Published
Abstract [en]

We present the energy spectra of protons and helium nuclei of cosmic rays obtained in the PAMELA experiment on board the satellite RESURS-DK1 for the period from August 2006 to December 2009. The spectra were measured in the energy range of 100 MeV/nucleon to 100 GeV/nucleon using a magnetic spectrometer within the apparatus. Variations in the solar modulation potential for protons and helium nuclei were calculated on the basis of the monthly mean particle fluxes. A force field model was used to compare the modulation with measurements from balloon experiments, and with measurements from a network of neutron monitors.

Place, publisher, year, edition, pages
2011. Vol. 75, no 6, 779-781 p.
Keyword [en]
Balloon experiment, Energy ranges, Energy spectra, Force field models, Helium nuclei, Magnetic spectrometers, Neutron monitors, Particle fluxes, Solar modulation, Experiments, Helium, Modulation, Protons, Spectroscopy, Solar energy
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-151216DOI: 10.3103/S1062873811060293Scopus ID: 2-s2.0-79960531173OAI: oai:DiVA.org:kth-151216DiVA: diva2:748344
Note

QC 20140919

Available from: 2014-09-19 Created: 2014-09-15 Last updated: 2016-12-23Bibliographically approved

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