Prediction Based on Convolutional Neural Networks and Vision Transformer for GOES-XRS Solar Flare Time Series

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Abstract

Solar flare is a type of solar activity that occurs at active regions at the surface of the sun. The emission of solar flares has numerous consequences, including the dis- turbances of magnetic fields, disruptions from energetic particles, and geomagnetic explosions. All those consequences have numerous impacts on human civilization, including the degradation of communication systems, power grids, space navigation, and even natural disasters. Thus, those minor or catastrophic consequences are al- ways threatening to the normal operation of society and decision-makers of those systems always seek a precise and accurate prediction of hazardous solar flares. This paper aims to develop a forecast model that can accurately decide whether solar flares would happen in the future. The data is extracted from the NOAA (National Oceanic and Atmospheric Administration) GOES-16 X-Ray Sensor that monitors solar activity by measuring the flux intensity of X-Ray. The original data is in the form of time series. Markov Transition Field is applied to the time series data, transforming the data into the form of 3-dimensional images. Therefore, the data undergone pre-processing could be applied to computer vision models. The aim of these models is to accurately recognize the Markov Transition Field images that symbolize there would be solar flare emission one hour later through a binary classification. Deep learning architects are the major components to accomplish this forecast task. Convolutional Neural Network (CNN) is a common approach in doing clas- sification tasks, which is also frequently used in recent studies that aim to predict flare emission through X-Ray images of the active regions. There are several classic CNN undergone training and testing, including LeNet-5, AlexNet, VGGNet 16 and 19, and ResNet-18, that utilizes the residue block structure. These CNN architects provide fascinating reliability and accuracy in this prediction task of solar flares, with multiple structures providing accuracy greater than 80%. Furthermore, Vision Transformer, a deep learning architect also used in classification based on trans- former structure is applied to the flare task. It is comprised of the core structure of multiple-head self-attention, residue blocks, layer normalization, and multilayer perceptron. Vision Transformer has shown outstanding accuracy (89.89%) while making predictions of solar flare emissions.
基于卷积神经网络和视觉变压器的GOES-XRS太阳耀斑时间序列预测
太阳耀斑是一种发生在太阳表面活跃区域的太阳活动。太阳耀斑的发射有许多后果,包括磁场的紊乱、高能粒子的破坏和地磁爆炸。所有这些后果都对人类文明产生了许多影响,包括通信系统、电网、空间导航的退化,甚至自然灾害。因此,这些轻微或灾难性的后果总是威胁到社会的正常运行,这些系统的决策者总是寻求对危险太阳耀斑的精确和准确预测。本文旨在建立一个能够准确判断未来太阳耀斑是否会发生的预报模型。这些数据是从NOAA(美国国家海洋和大气管理局)GOES-16 x射线传感器提取的,该传感器通过测量x射线的通量强度来监测太阳活动。原始数据采用时间序列的形式。将马尔可夫过渡场应用于时间序列数据,将数据转换成三维图像的形式。因此,经过预处理的数据可以应用于计算机视觉模型。这些模型的目的是通过二元分类准确识别马尔科夫过渡场图像,这些图像象征着一小时后太阳耀斑的发射。深度学习架构师是完成这项预测任务的主要组成部分。卷积神经网络(CNN)是进行分类任务的常用方法,也经常用于最近的研究,旨在通过活动区域的x射线图像预测耀斑发射。有几个经典的CNN经过训练和测试,包括LeNet-5, AlexNet, VGGNet 16和19,ResNet-18,使用了残馀块结构。这些CNN架构师在预测太阳耀斑的任务中提供了令人着迷的可靠性和准确性,多个结构提供的精度超过80%。此外,将基于变换结构分类的深度学习架构Vision Transformer应用于火炬任务。它由多头自注意、残差块、层归一化和多层感知器等核心结构组成。Vision Transformer在预测太阳耀斑辐射时显示出出色的准确性(89.89%)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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