A Universal Method for Solar Filament Detection from H-alpha Observations using Semi-supervised Deep Learning
Filaments are omnipresent features in the solar atmosphere. Their location, properties and
time evolution can provide information about changes in solar activity and assist the …
time evolution can provide information about changes in solar activity and assist the …
The Plasma in quiet Sun Regions: Multi-Instrument View
JM Rodríguez-Gómez, C Kuckein… - arXiv preprint arXiv …, 2024 - arxiv.org
A joint campaign of several space-borne and ground-based observatories, such as the
GREGOR solar telescope, the Extreme-ultraviolet Imaging Spectrometer (EIS), and the …
GREGOR solar telescope, the Extreme-ultraviolet Imaging Spectrometer (EIS), and the …