HiSAXy: A fast methodology for solar wind structure identification in millions of time series
Authors
Hala Lamdouar
Sairam Sundaresan
Anna Jungbluth
Sudeshna Boro Saikia
Amanda Joy Camarata
Nathan Miles
Marcella Scoczynski
Mavis Stone
Andrés Muñoz-Jaramillo
Ayris Narock
Adam Szabo
Abstract
We present a hybridized unsupervised clustering algorithm Hisaxy as a novel way to identify frequently occurring magnetic structures embedded in the interplanetary magnetic field (IMF) carried by the solar wind. The Hisaxy algorithm utilizes a combination of indexable Symbolic Aggregate approXimation (iSAX) and Hierarchical Density-Based Spatial Clustering of Applications with Noise (HDBSCAN) to efficiently identify clusters of patterns embedded in time series data. We utilized Hisaxy to identify small-scale structures, known as discontinuities, embedded in time series measurements of the IMF. In doing so, we demonstrate the capability of the algorithm to significantly reduce the amount of human analysis hours required to identify these structures, all the while maintaining a high degree of self similarity within a given cluster of time series data.
