Dataset: On the fractal properties of Cosmic Rays and Sun Dynamics Cross-Correlations

The following dataset corresponds to the application of MultiFractal Detrented Cross-Correlation Analysis (MFDCCA) for the Cosmic Ray case using the Izmiran network detectors (http://cr0.izmiran.ru/common/links.htm) and Solar Dynamics indexes (NASA: spacecraft interleaved near-Earth solar wind data, https://omniweb.gsfc.nasa.gov/ow_min.html). The data sets are: 1. 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. 2. A dataset corresponding to the Solar Dynamics indexes (NASA) 3. Codes (jupyter notebook) needed for replication and reproducibility. These data have been used for the manuscript: On the fractal properties of Cosmic Rays and Sun Dynamics Cross-Correlations. D. Sierra-Porta (orcid=0000-0003-3461-1347). Submitted to publication (2022).本数据集对应多重分形去趋势互相关分析（MultiFractal Detrented Cross-Correlation Analysis，MFDCCA）在宇宙射线场景中的应用，所用数据源自伊兹米兰（Izmiran）网络探测器（http://cr0.izmiran.ru/common/links.htm）与太阳动力学指数数据集（NASA：近地太阳风航天器交错观测数据，https://omniweb.gsfc.nasa.gov/ow_min.html）。本次提供的数据集包含以下三类： 1. 小时分辨率监测站计数数据集：每列均包含归一化计数信息，以及用于平滑曲线的中值滤波相关数据； 2. NASA发布的太阳动力学指数数据集； 3. 用于研究复现的Jupyter Notebook代码文件。 本数据集已应用于以下待刊论文：《宇宙射线与太阳动力学互相关的分形特性》，作者D. Sierra-Porta（ORCID：0000-0003-3461-1347），2022年提交待发表。