Scaling analysis and model estimation of solar corona index |
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Authors: | Samujjwal Ray Rajdeep Ray Mofazzal Hossain Khondekar Koushik Ghosh |
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Affiliation: | 1. Department of Electronics & Instrumentation Engineering, Dr. B. C. Roy Engineering College, Durgapur 713206, West Bengal, India;2. Department of Electronics & Communication Engineering, Dr. B. C. Roy Engineering College, Durgapur 713206, West Bengal, India;3. Department of Mathematics, University Institute of Technology, Burdwan 713104, West Bengal, India |
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Abstract: | A monthly average solar green coronal index time series for the period from January 1939 to December 2008 collected from NOAA (The National Oceanic and Atmospheric Administration) has been analysed in this paper in perspective of scaling analysis and modelling. Smoothed and de-noising have been done using suitable mother wavelet as a pre-requisite. The Finite Variance Scaling Method (FVSM), Higuchi method, rescaled range (R/S) and a generalized method have been applied to calculate the scaling exponents and fractal dimensions of the time series. Autocorrelation function (ACF) is used to find autoregressive (AR) process and Partial autocorrelation function (PACF) has been used to get the order of AR model. Finally a best fit model has been proposed using Yule-Walker Method with supporting results of goodness of fit and wavelet spectrum. The results reveal an anti-persistent, Short Range Dependent (SRD), self-similar property with signatures of non-causality, non-stationarity and nonlinearity in the data series. The model shows the best fit to the data under observation. |
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Keywords: | Corona Solar Hurst FVSM Fractal Higuchi Autocorrelation Wavelets PACF Yule-walker |
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