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arXiv 2108.06394astro-ph.SRastro-ph.IMcs.LGphysics.space-phstat.ML
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A Machine-Learning-Ready Dataset Prepared from the Solar and Heliospheric Observatory Mission

Center for Mathematics and Computer Science(数学与计算机科学中心);W.W. Hansen Experimental Physics Laboratory, Stanford University(斯坦福大学W.W.汉森实验物理实验室);US Naval Research Laboratory(美国海军研究实验室);CIRES, University of Colorado, Boulder(科罗拉多大学博尔德分校CIRES);NOAA, Space Weather Prediction Center(美国国家海洋和大气管理局空间天气预测中心)

Carl Shneider, Andong Hu, Ajay K. Tiwari, Monica G. Bobra, Karl Battams, Jannis Teunissen, Enrico Camporeale

英文摘要:

We present a Python tool to generate a standard dataset from solar images that allows for user-defined selection criteria and a range of pre-processing steps. Our Python tool works with all image products from both the Solar and Heliospheric Observatory (SoHO) and Solar Dynamics Observatory (SDO) missions. We discuss a dataset produced from the SoHO mission's multi-spectral images which is free of missing or corrupt data as well as planetary transits in coronagraph images, and is temporally synced making it ready for input to a machine learning system. Machine-learning-ready images are a valuable resource for the community because they can be used, for example, for forecasting space weather parameters. We illustrate the use of this data with a 3-5 day-ahead forecast of the north-south component of the interplanetary magnetic field (IMF) observed at Lagrange point one (L1). For this use case, we apply a deep convolutional neural network (CNN) to a subset of the full SoHO dataset and compare with baseline results from a Gaussian Naive Bayes classifier.

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