Visualizing and Interpreting Unsupervised Solar Wind Classifications

Astronomy Geophysics. Cosmic physics FOS: Physical sciences QB1-991 Astronomy & Astrophysics 7. Clean energy 01 natural sciences Physics - Space Physics 0103 physical sciences unsupervised SPACE CYCLE ACE Solar and Stellar Astrophysics (astro-ph.SR) Self-Organizing Maps 0105 earth and related environmental sciences autoencoder COROTATING INTERACTION REGIONS PCA Science & Technology QC801-809 ENERGETIC PARTICLES Space Physics (physics.space-ph) CORONAL MASS EJECTIONS machine learning SLOW solar wind Astrophysics - Solar and Stellar Astrophysics 13. Climate action Physical Sciences SHOCK clustering
DOI: 10.3389/fspas.2020.553207 Publication Date: 2020-09-25T16:02:42Z
ABSTRACT
One of the goals machine learning is to eliminate tedious and arduous repetitive work. The manual semi-automatic classification millions hours solar wind data from multiple missions can be replaced by automatic algorithms that discover, in mountains multi-dimensional data, real differences properties. In this paper we present how unsupervised clustering techniques used segregate different types wind. We propose use advanced reduction methods pre-process introduce Self-Organizing Maps visualize interpret 14 years ACE data. Finally, show these potentially uncover hidden information, they compare with previous categorizations.
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