News
A new explanation for the high temperatures of the solar corona
An international scientific team, including researchers from the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL), have...
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TalkArch Filament Systems and their evolution through the layers of the solar atmosphereEmerging flux regions (EFRs) are seen as magnetic concentrations in the photosphere of the Sun. From a theoretical point of view, the EFRs are formed in the...
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TalkAre chromospheric fibrils tracing the magnetic field?Fibrils are thin elongated features visible in the solar chromosphere in and around magnetized regions. Because of their visual appearance they have been...
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TalkFlares: highly energetic explosions on the SunFlares are among the most energetic magnetic solar phenomena. They are often accompanied by ejections of charged particles, which have a direct influence on the...
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PublicationLarge-amplitude Prominence Oscillations following Impact by a Coronal JetObservational evidence shows that coronal jets can hit prominences and set them in motion. The impact leads to large-amplitude oscillations (LAOs) in the...