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A series of solar physics seminars streamed to several European institutes
Site URL: espos.stream/
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Effects of Plasma Composition Variations on the Radiative Cooling of Solar Flare Loops
http://espos.stream/2026/05/21/Mihailescu/
Published: May 21, 2026 11:00
Abstract The plasma composition in the solar corona is variable, with a strong dependency on the first ionisation potential (FIP) of elements. In flaring regions, plasma composition has been shown to have significant spatial and temporal variations, likely…
Modelling Magnetohydrodynamic Waves in Streamers: First Comparison with Metis Observations
http://espos.stream/2026/05/07/Kumar/
Published: May 7, 2026 11:00
Abstract Magnetohydrodynamic waves are often regarded as efficient pathways for magnetic energy transfer from the solar interior. Consequently, they are key to not only understand the physical processes behind coronal heating and/or solar wind acceleration…