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Measuring fluxes of the protons and helium nuclei of high-energy cosmic rays
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: 66
2011 (English)In: Bulletin of the Russian Academy of Sciences: Physics, ISSN 1062-8738, Vol. 75, no 3, 327-330 p.Article in journal (Refereed) Published
Abstract [en]

Techniques for measuring helium nuclei and proton energy spectra in circumterrestrial space were developed on the basis of simulated data and data from the position-sensitive silicon-tungsten calorimeter in the PAMELA satellite experiment. The thickness of the calorimeter is 0.6 nuclear interaction lengths. In this work, the experimental results for the measured energy spectra of the protons and helium nuclei of cosmic rays with energies above 50 GeV are presented.

Place, publisher, year, edition, pages
2011. Vol. 75, no 3, 327-330 p.
Keyword [en]
Energy spectra, Helium nuclei, High-energy cosmic rays, Nuclear interaction, Position sensitive, Proton energy spectra, Simulated data, Calorimetry, Cosmic rays, Protons, Spectroscopy, Tungsten, Helium
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-151236DOI: 10.3103/S1062873811030208Scopus ID: 2-s2.0-79955823455OAI: oai:DiVA.org:kth-151236DiVA: diva2:747247
Note

QC 20140916

Available from: 2014-09-16 Created: 2014-09-15 Last updated: 2016-12-23Bibliographically approved

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