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Solar Modulation of 2H/1H and 3He/4He according to Data Obtained in the PAMELA Satellite-Borne Experiment between 2006 and 2014

  • Elementary Particles and Fields
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Abstract

Preliminary results of measurements of the solar modulation of the isotopic hydrogen and helium content in galactic cosmic rays are presented for the first time. These data were obtained between 2006 and 2014 in the PAMELA international orbital experiment via measuring the time of flight of nuclei in the Pamela scintillation telescope and via analyzing, in the multilayered calorimeter of the PAMELA magnetic spectrometer, ionization losses of nuclei whose rigidity was known from trajectory measurements and which traversed the instrument without undergoing nuclear interactions. The results of these measurements are compared with existing experimental and calculated data, which are quite scanty.

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Authors and Affiliations

  1. Ioffe Physical-Technical Institute, Russian Academy of Sciences, Politekhnicheskaya ul. 26, St. Petersburg, 194021, Russia

    E. A. Bogomolov & G. I. Vasilyev

  2. Universität Siegen, Adolf-Reichwein-Straße 2, Siegen, 57068, Germany

    W. Menn

Authors
  1. E. A. Bogomolov
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  2. G. I. Vasilyev
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  3. W. Menn
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PAMELA Collaboration

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Correspondence to E. A. Bogomolov.

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Original Russian Text © E.A. Bogomolov, G.I. Vasilyev, W. Menn, 2018, published in Yadernaya Fizika, 2018, Vol. 81, No. 3, pp. 377–382.

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Bogomolov, E.A., Vasilyev, G.I., Menn, W. et al. Solar Modulation of 2H/1H and 3He/4He according to Data Obtained in the PAMELA Satellite-Borne Experiment between 2006 and 2014. Phys. Atom. Nuclei 81, 390–395 (2018). https://doi.org/10.1134/S1063778818030067

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  • DOI: https://doi.org/10.1134/S1063778818030067

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