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


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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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E. Bogomolov

Ioffe Physical-Technical Institute

编辑信件的主要联系方式.
Email: Edward.Bogomolov@mail.ioffe.ru
俄罗斯联邦, Politekhnicheskaya ul. 26, St. Petersburg, 194021

G. Vasilyev

Ioffe Physical-Technical Institute

Email: Edward.Bogomolov@mail.ioffe.ru
俄罗斯联邦, Politekhnicheskaya ul. 26, St. Petersburg, 194021

W. Menn

Universität Siegen

Email: Edward.Bogomolov@mail.ioffe.ru
德国, Adolf-Reichwein-Straße 2, Siegen, 57068

Email: Edward.Bogomolov@mail.ioffe.ru

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