Improvements on coronal hole detection in SDO/AIA images using supervised classification
Martin A. Reiss, Stefan J. Hofmeister, Ruben De Visscher, Manuela, Temmer, Astrid M. Veronig, V\'eronique Delouille, Benjamin Mampaey, Helmut, Ahammer

TL;DR
This paper presents a machine learning approach combining segmentation and classification techniques to improve coronal hole detection in solar EUV images, achieving high accuracy and real-time applicability.
Contribution
The study introduces a supervised classification framework that enhances coronal hole detection accuracy over traditional methods using magnetic and shape features.
Findings
Linear SVM achieved the highest true skill statistic (~0.90).
Magnetic field data improved classification performance.
Approach is computationally efficient for real-time applications.
Abstract
We demonstrate the use of machine learning algorithms in combination with segmentation techniques in order to distinguish coronal holes and filaments in SDO/AIA EUV images of the Sun. Based on two coronal hole detection techniques (intensity-based thresholding, SPoCA), we prepared data sets of manually labeled coronal hole and filament channel regions present on the Sun during the time range 2011 - 2013. By mapping the extracted regions from EUV observations onto HMI line-of-sight magnetograms we also include their magnetic characteristics. We computed shape measures from the segmented binary maps as well as first order and second order texture statistics from the segmented regions in the EUV images and magnetograms. These attributes were used for data mining investigations to identify the most performant rule to differentiate between coronal holes and filament channels. We applied…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Solar Radiation and Photovoltaics · Ionosphere and magnetosphere dynamics
