CORDIS Project
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This project conducts simulations of convection and heat transport in Sun-like stars, focusing on the tachocline region. By using advanced modeling techniques, it aims to improve our understanding of stellar magnetic fields and their impact on solar phenomena.
Stars like our Sun are complex systems in which hydrogen fusion occurs in the radiative core, and heat is transported by convection in the outer part.
The two most important regions in Sun-like stars are the optical surface and the transition region between the radiative core and the convective envelop, called the tachocline.
The tachocline, which is believed to be responsible for generating stellar global magnetic fields (also related to the 11-year solar cycle), is a complicated region where t…
UNIVERSITETET I OSLO
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