Solar Flare Short-term Forecast Model Based on Long and Short-term Memory Neural Network

Q4 Physics and Astronomy
He Xin-ran , Zhong Qiu-zhen , Cui Yan-mei , Liu Si-qing , Shi Yu-rong , Yan Xiao-hui , Wang Zi-si-yu
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引用次数: 2

Abstract

Solar flares are a kind of violent solar eruptive activity phenomenon and an important warning device of space weather disturbance. In space weather forecasting, flare forecasting is an important forecast content. This paper proposes a flare prediction model based on long and short-term memory neural network, which uses the time sequence of magnetic field changes in the solar active region in the past 24 h to construct samples, and analyzes the time series evolution of magnetic field characteristics through the long and short-term memory neural network to predict whether M-level flares will occur in the next 48 h. This paper uses a data set for all active region samples from May 2010 to May 2017, and selects 10 magnetic field characteristic parameters of SDO/HMI SHARP. In the modeling process, six feature parameters with high weight, gain rate, and coverage rate were selected as input parameters through XGBoost method. Through test comparison, the false report rate and accuracy rate of the model are similar to the traditional machine learning model, and the accuracy rate and critical success index are better than the traditional machine learning model, which are 0.7483 and 0.7402, respectively. The overall effect of the model is better than that of the traditional machine learning model.

基于长短期记忆神经网络的太阳耀斑短期预报模型
太阳耀斑是一种强烈的太阳喷发活动现象,是空间天气扰动的重要预警装置。在空间天气预报中,耀斑预报是一项重要的预报内容。提出了一种耀斑基于长期和短期记忆神经网络预测模型,利用时间序列太阳活跃区域的磁场变化在过去24小时构造样本,并分析磁场特征的时间序列演化通过长期和短期记忆神经网络来预测是否≥M-level耀斑将发生在未来48 h。本文使用一个数据集所有活跃区域样品从2010年5月到2017年5月,选取了10个SDO/HMI SHARP的磁场特征参数。在建模过程中,通过XGBoost方法选取权重、增益率、覆盖率较高的6个特征参数作为输入参数。通过测试对比,该模型的误报率和准确率与传统机器学习模型相近,准确率和临界成功指数优于传统机器学习模型,分别为0.7483和0.7402。该模型的整体效果优于传统的机器学习模型。
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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来源期刊
Chinese Astronomy and Astrophysics
Chinese Astronomy and Astrophysics Physics and Astronomy-Astronomy and Astrophysics
CiteScore
0.70
自引率
0.00%
发文量
20
期刊介绍: The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.
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