Analysis of cosmic ray variations recorded in October–December 2013
Tipo
Artigo
Data de publicação
2015
Periódico
Bulletin of the Russian Academy of Sciences: Physics
Citações (Scopus)
6
Autores
Makhmutov V.S.
Bazilevskaya G.A.
Stozhkov Y.I.
Raulin J.-P.
Philippov M.V.
Bazilevskaya G.A.
Stozhkov Y.I.
Raulin J.-P.
Philippov M.V.
Orientador
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Título de Volume
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Resumo
© 2015, Allerton Press, Inc.Results from analyzing variations in cosmic ray and solar activities in October–November 2013 are described. Data from observations using a Kover/GCR cosmic ray detector (CERN, Switzerland) and the neutron monitor worldwide network are used. Solar flare activity is analyzed using results on H<inf>α</inf>, X-ray, gamma, and radio emissions observed at ground-based installations and on board spacecraft (e.g., GOES and FERMI). Attention is focused on the cosmic ray increases detected by the Kover/GCR detector on October 15 and November 19, 2013. Features of these events are similar to increases detected earlier on March 7, 2011, and January 23, 2012, by the Kover/CASLEO detector at the CASLEO astronomical complex in Argentina. Possible correlations between the observed cosmic ray intensity increases and flare solar activity or processes in the Earth’s atmosphere are considered.
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Assuntos Scopus
Cosmic ray intensity , Ground based , Neutron monitors , On-board spacecrafts , Radio emission , Solar activity , Solar flare , World-wide networks