Mayorov, A. G.A. G.MayorovAdriani, O.O.AdrianiAleksandrin, S. Y.S. Y.AleksandrinDi Felice, ValeriaValeriaDi FelicePicozza, P.P.PicozzaRicci, M.M.Ricci2020-09-172020-09-172017-01-01https://hdl.handle.net/20.500.13025/5281Journal of Physics Conference Series, Volume 798, Issue 1, article id. 012042 (2017).Solar modulation of galactic protons with energies from 50 MeV up to dozens of GeV during July `06 - January `16 studied based on a data of the magnetic spectrometer PAMELA and scintillation spectrometer ARINA. This period is interesting because it covers the end of 23<SUP>rd</SUP> and current 24<SUP>th</SUP> cycles of solar activity, including the abnormally long transient period and change of the polarity of solar magnetic field.Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data10.1088/1742-6596/798/1/012042http://adsabs.harvard.edu/abs/2017JPhCS.798a2042M2017JPhCS.798a2042M