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 23rd and current 24th cycles of solar activity, including the abnormally long transient period and change of the polarity of solar magnetic field. © Published under licence by IOP Publishing Ltd.

Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

Castellini G;Ricciarini SB;
2017

Abstract

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 23rd and current 24th cycles of solar activity, including the abnormally long transient period and change of the polarity of solar magnetic field. © Published under licence by IOP Publishing Ltd.
2017
Istituto di Fisica Applicata - IFAC
Cosmic rays; Cosmology; Magnetic polarity; Modulation; Solar energy; Spectrometers Galactic cosmic rays; Magnetic spectrometers; Solar activity; Solar magnetic fields; Solar modulation; Transient periods
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/328455
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