CORDIS Project
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This project focuses on understanding the magnetic structure of solar filaments, which are dense plasma structures in the sun's atmosphere. By using advanced observational techniques, it aims to determine their formation and evolution, which is crucial for space weather forecasting.
Solar filaments are prominent cold and dense structures of plasma suspended in the hot corona.
They are called prominences when observed above the solar limb.
Despite they were probably the first solar features to be observed, the magnetic structure of solar filaments is still largely unknown, being their determination a fundamental problem for Solar Physics.
The reason is the lack of chromospheric observables able to provide binding information for the magnetic field.
Therefore, though there ar…
INSTITUTO DE ASTROFISICA DE CANARIAS
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