CORDIS Project
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CIRCE aims to model magnetic field generation in stars by exploring dynamo instability. The project focuses on identifying the conditions that lead to magnetic field amplification in stellar environments, which is crucial for understanding stellar evolution and dynamics.
Modeling magnetic field generation by dynamo instability in stellar objects is a long-standing challenge with far-reaching implications for stellar evolution theory.
Underlying motivations are exemplified by the need to understand stellar spin-down and accretion rates in protostellar discs, which are known to be dynamically impacted by magnetic fields.
The interest sparked by recurring discrepancies between predictive evolution models and rapidly-progressing observations drives the current resea…
INSTITUT NATIONAL DE RECHERCHE EN INFORMATIQUE ET AUTOMATIQUE
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