论文标题
太阳耀斑预测的基于形状的功能工程
Shape-based Feature Engineering for Solar Flare Prediction
论文作者
论文摘要
太阳耀斑是由太阳表面的活动区域(AR)磁性喷发引起的。这些事件可能会对人类活动产生重大影响,其中许多事件可以通过良好预测的足够预先警告来减轻许多事件。迄今为止,基于机器学习的耀斑预测方法已采用基于物理的AR图像作为特征。最近,有一些工作使用深度学习方法自动推导的功能(例如卷积神经网络)。我们使用计算拓扑和计算几何形状的工具描述了从太阳的磁图图像中提取的一系列新型基于形状的特征。我们在多层感知器(MLP)神经网络的背景下评估了这些功能,并将其性能与传统物理属性进行比较。我们表明,这些基于抽象形状的特征优于人类专家选择的功能,而两个功能集的组合则进一步提高了预测能力。
Solar flares are caused by magnetic eruptions in active regions (ARs) on the surface of the sun. These events can have significant impacts on human activity, many of which can be mitigated with enough advance warning from good forecasts. To date, machine learning-based flare-prediction methods have employed physics-based attributes of the AR images as features; more recently, there has been some work that uses features deduced automatically by deep learning methods (such as convolutional neural networks). We describe a suite of novel shape-based features extracted from magnetogram images of the Sun using the tools of computational topology and computational geometry. We evaluate these features in the context of a multi-layer perceptron (MLP) neural network and compare their performance against the traditional physics-based attributes. We show that these abstract shape-based features outperform the features chosen by the human experts, and that a combination of the two feature sets improves the forecasting capability even further.