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The NeoCon project investigates the discrepancies between solar observations and existing models of stellar convection. By developing a new model that incorporates entropy rain and magnetic effects, it aims to provide a more accurate representation of convection in stars, which could enhance our understanding of stella…
Tension between solar observations and theoretical and numericalmodels is shifting the paradigm of stellar convection: simulationsproduce dominant large-scale flows that are absent in the Sun and thesupergranulation scale which according to helioseismology is dominantin the Sun is not captured by simulations.
This discrepancy, named theconvective conundrum, is the most likely reason why solar differentialrotation and global dynamo cannot be reproduced by currentsimulations.
Canonical theory of c…
UNIVERSITAET GRAZ
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