Automated Detection of Accelerating Solar Eruptions Using Parabolic Hough Transform
Solar eruptions such as coronal mass ejections (CMEs) observed in the inner solar corona (up to 4 R ⊙) show acceleration profiles that appear as parabolic ridges in height-time plots. Inspired by the white-light automated detection algorithms Computer Aided CME Tracking System (CACTus) and Solar Eruptive Events Detection System (SEEDS), we employ
Patel, Ritesh et al.
Fecha de publicación:
2
2021