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Behaviour of 27-Day and 13.5-Day Periodicities in Galactic Cosmic Particles as Observed by Spacecraft and Neutron Monitors During Different Solar Polarity Cycles
Recurrence of galactic cosmic-ray intensity and anisotropy in solar minima 23/24 and 24/25 observed by ACE/CRIS, STEREO, SOHO/EPHIN and neutron monitors
Study of the 27 Day Variations in GCR Fluxes during 2007–2008 Based on PAMELA and ARINA Observations
R. Modzelewska, G. A. Bazilevskaya, M. Boezio, S. V. Koldashov, M. B. Krainev, N. Marcelli, A. G. Mayorov, M. A. Mayorova, R. Munini, I. K. Troitskaya, R. F. Yulbarisov, X. Luo, M. S. Potgieter and O. P. M. Aslam The Astrophysical Journal 904(1) 3 (2020) https://doi.org/10.3847/1538-4357/abbdac
27-day variation of galactic cosmic ray intensity by PAMELA experiment. Relationship with heliospheric parameters