Comparison Between Gramian Angular Fields (GAF) and Markov Transition Field (MTF) Images Data by Using them as Input to the Deep Learning Neural Network Solar Flare Production Platform

Tarek A. M. Nagem, Sohil F. Alshareef, Abdel-rahman Mohamed, Akram Gihedan, S. Albargathe
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引用次数: 1

Abstract

The prediction of solar storms from real-time satellites data is an essential to protect various aviation, power, and communication infrastructures. For this reason, current research interest is focusing on creating systems that can predict solar fare accurately. This paper combers Gramian Angular Fields (GAF) images and Markov Transition Field (MTF) images that have been generated by converting pre-flare Geostationary Operational Environmental Satellite (GOES) data from 2010 to 2016. After that, the deep learning neural network for the solar flare production platform accepts both MTF and GAF images as input to generate the predictions. Furthermore, this paper; investigated using MTF and GAF images spritely as input to the solar flare production platform. After that, the results of MTF and GAF images were compared using various prediction verification measures.
用Gramian角场(GAF)和Markov过渡场(MTF)图像数据作为输入到深度学习神经网络太阳耀斑生成平台的比较
从实时卫星数据预测太阳风暴对保护各种航空、电力和通信基础设施至关重要。由于这个原因,目前的研究兴趣集中在创造能够准确预测太阳能票价的系统上。本文对2010年至2016年地球静止运行环境卫星(GOES)数据转换生成的格拉曼角场(GAF)图像和马尔可夫过渡场(MTF)图像进行了梳理。之后,用于太阳耀斑产生平台的深度学习神经网络接受MTF和GAF图像作为输入来生成预测。进一步,本文;利用MTF和GAF图像进行了研究,并将其作为太阳耀斑产生平台的输入。然后,使用各种预测验证措施对MTF和GAF图像的结果进行比较。
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