The dynamics of a solar arch filament system from the chromosphere to the photosphere
We study the dynamics of plasma along the legs of an arch filament system (AFS) from the chromosphere to the photosphere, observed with high-cadence spectroscopic data from two ground-based solar telescopes: the GREGOR telescope (Tenerife) using the GREGOR Infrared Spectrograph in the He I 10830 Å range and the Swedish Solar Telescope (La Palma)
González Manrique, S. J. et al.
Fecha de publicación:
7
2020