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Forbush Decreases in the Fluxes of Galactic Cosmic Rays, According to the PAMELA Experiment

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dc.contributor.authorLagoida, I. A.
dc.contributor.authorVoronov, S. A.
dc.contributor.authorMikhailov, V. V.
dc.contributor.authorЛагойда, Илья Алексеевич
dc.contributor.authorВоронов, Сергей Александрович
dc.contributor.authorМихайлов, Владимир Владимирович
dc.date.accessioned2024-11-22T06:39:48Z
dc.date.available2024-11-22T06:39:48Z
dc.date.issued2019
dc.description.abstract© 2019, Allerton Press, Inc.Abstract: Amplitudes of Forbush decreases registered in the PAMELA experiment from 2006 to 2014 were analyzed, depending on such characteristics of interplanetary space as the magnitude of the magnetic field modulus, the solar wind velocity, and the plasma temperature. The PAMELA telescope consists of a time-of-flight system, a magnetic spectrometer, anticoincidence systems, an electromagnetic calorimeter, and a neutron detector. It was launched into Earth orbit aboard the Resurs DK1 satellite in June 2006 and continued to work for 10 years.
dc.format.extentС. 971-973
dc.identifier.citationLagoida, I. A. Forbush Decreases in the Fluxes of Galactic Cosmic Rays, According to the PAMELA Experiment / Lagoida, I.A., Voronov, S.A., Mikhailov, V.V. // Bulletin of the Russian Academy of Sciences: Physics. - 2019. - 83. - № 8. - P. 971-973. - 10.3103/S1062873819080252
dc.identifier.doi10.3103/S1062873819080252
dc.identifier.urihttps://www.doi.org/10.3103/S1062873819080252
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85073242490&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19676
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleForbush Decreases in the Fluxes of Galactic Cosmic Rays, According to the PAMELA Experiment
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue8
oaire.citation.volume83
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