Dataset: MultiFractal Detrented Fluctuations Analysis on Cosmic Rays Time Series

Published: 25 July 2022| Version 3 | DOI: 10.17632/kkk7ckvhcw.3
Contributor:
David Sierra Porta

Description

The following dataset corresponds to the application of MultiFractal Detrented Fluctuations Analysis (MFDFA) for the Cosmic Ray case using the Izmiran network detectors (http://cr0.izmiran.ru/common/links.htm). The data sets are: 1. a Table of the neutron monitors with their corresponding properties and characteristics; 2. a Table of the neutron monitors with their corresponding properties and characteristics. 2. A table for Hurst exponents in the context of MFDFA for all the monitors and stations considered. 3. Three files corresponding to the calculated values of the analysis parameters for the Moscow station (http://cr0.izmiran.ru/mosc/main.htm). 4. A dataset corresponding to the counts of the monitoring stations in hourly resolution. Each column contains information for the normalized counts and also for a filter using the median for the smoothed curve. These data have been used for the manuscript: Linking cosmic ray intensities to cutoff rigidity through Multifractal Detrended Fluctuation Analysis. D. Sierra-Porta (orcid=0000-0003-3461-1347) and A. Domínguez-Monterroza (orcid=0000-0002-5274-7443). Submitted to Physica A: Statistical Mechanics and its Applications - Elsevier (2022). https://papers.ssrn.com/sol3/papers.cfm?abstract_id=4143311

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Institutions

Universidad Tecnologica de Bolivar

Categories

Astrophysics, Time Series, Particle Astrophysics, Cosmic Ray, High-Energy Astrophysics

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