Abstract
Solar Radio Flux (SRF) is the significant index in easily evaluating everyday solar activities. From the statistical analysis of SRF at 2800 MHz, 1415 MHz and 610 MHz from 1976 to 1994, and only 111 Solar Proton Events (SPEs) occurring in the same period, we have given the statistical relation between them. In fact, there occurred a total of 131 SPEs in the same period, but we dealt with only 111 SPEs of them, because of lack of SRF data in SGD (2800 MHz, 1415 MHz and 610 MHz). We also discussed the possible parameters of SRF at 2800 MHz, 1415 MHz and 610 MHz for prediction of SPEs by statistical analysis, Artificial Neural Network (ANN) and Genetic Algorithm (GA) using MATLAB. In this study, we used some parameters: the daily total SRF, the overall rate of increase of SRF and SPEs.
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Kim, K.N., Sin, S.A., Song, K.A. et al. A technique for prediction of SPEs from solar radio flux by statistical analysis, ANN and GA. Astrophys Space Sci 363, 170 (2018). https://doi.org/10.1007/s10509-018-3263-8
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DOI: https://doi.org/10.1007/s10509-018-3263-8