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Study of the 27-day variations in the GCR fluxes in 2007-2008 based on PAMELA and ARINA observations

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dc.contributor.authorModzelewska, R.
dc.contributor.authorBazilevskaya, G. A.
dc.contributor.authorBoezio, M.
dc.contributor.authorKrainev, M. B.
dc.contributor.authorKoldashov, S. V.
dc.contributor.authorMayorov, A. G.
dc.contributor.authorMayorov,A.G.
dc.contributor.authorMayorova, M. A.
dc.contributor.authorTroitskaya, I. K.
dc.contributor.authorМайоров, Андрей Георгиевич
dc.contributor.authorЮлбарисов, Рустам Фаритович
dc.date.accessioned2024-11-21T18:39:33Z
dc.date.available2024-11-21T18:39:33Z
dc.date.issued2019
dc.description.abstract© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).We have investigated the energy and time dependences of the amplitude of the proton galactic cosmic ray intensity 27-days oscillations in 2007-2008 from the data of the PAMELA and ARIN? spectrometers on board the RESURS DK-1 satellite. We have used different types of harmonic analysis, such as Fourier and wavelet analysis. The time profiles and amplitude dependences for the rigidities of cosmic ray particles from ~300 MV to tens of GV were obtained. It is shown that the amplitude-rigidity dependence cannot be described by a power law at low energies, the amplitude decreases with decreasing rigidity starting from ~ 1 GV. For a physical interpretation, we have studied the relationship between the 27-day variations of GCR and heliospheric parameters: solar wind velocity and heliospheric magnetic field.
dc.identifier.citationStudy of the 27-day variations in the GCR fluxes in 2007-2008 based on PAMELA and ARINA observations / Modzelewska, R. [et al.] // Proceedings of Science. - 2019. - 358
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85086242466&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19548
dc.relation.ispartofProceedings of Science
dc.titleStudy of the 27-day variations in the GCR fluxes in 2007-2008 based on PAMELA and ARINA observations
dc.typeConference Paper
dspace.entity.typePublication
oaire.citation.volume358
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