dc.creatorSierra-Porta, D.
dc.date.accessioned2023-07-25T12:10:22Z
dc.date.accessioned2023-09-06T15:42:58Z
dc.date.available2023-07-25T12:10:22Z
dc.date.available2023-09-06T15:42:58Z
dc.date.created2023-07-25T12:10:22Z
dc.date.issued2022
dc.identifierSierra-Porta, D. (2022). On the fractal properties of cosmic rays and Sun dynamics cross-correlations. Astrophysics and Space Science, 367(12), 116.
dc.identifierhttps://hdl.handle.net/20.500.12585/12428
dc.identifier10.1007/s10509-022-04151-5
dc.identifierUniversidad Tecnológica de Bolívar
dc.identifierRepositorio Universidad Tecnológica de Bolívar
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8682528
dc.description.abstractWe investigate the cosmic rays and ten physical parameters of heliosphere behavior considering the scaling features of their temporal evolution. Our analysis start with the cosmic rays measurements by a neutron monitor station located in Moscow, as well sunspot, Ap index, Na/Np, Alfven mach number, DST index, Kp index, Plasma beta (β ), Proton temperature, F10.7 index and Field magnitude |B| (Interplanetary Magnetic Field, IMF), for the period 1976 to early 2020. Each of these datasets was analyzed by using the Multifractal Detrended Fluctuation Analysis and Multifractal Detrended Cross-Correlation Analysis in order to investigate intrinsic properties, like self-similarity and the spectrum of singularities. The main result obtained is that the cosmic rays time series as well the 10 heliospheric parameters exhibit positive long-range correlations with multifractal behavior.
dc.languageeng
dc.publisherCartagena de Indias
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional
dc.sourceAstrophysics and Space Science
dc.titleOn the fractal properties of cosmic rays and Sun dynamics cross-correlations


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