CORDIS Project
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This project investigates the emergence of magnetic fields in astrophysical environments, focusing on their role in solar phenomena such as jets and coronal mass ejections. It aims to enhance understanding of the dynamics of these magnetic processes.
Magnetic fields are produced in differentially rotating and convecting environments, such as in the interior of the sun, other convective stars and also in accretion disks.
The produced magnetic fields emerge in the outer atmospheric layers because of magnetic buoyancy producing a plethora of explosive events.
This Emergence of Magnetic Flux (EMF) is a fundamental astrophysical phenomenon and the possible driver of the observed, ubiquitous activity in astrophysical plasmas.
In the case of the Su…
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