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arXiv · 1812.08976

Activity variation driven by flux emergence and transport on Sun-like stars

Emre Işık·Sami K. Solanki·Natalie A. Krivova·Alexander I. Shapiro
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Abstract

In G dwarfs, the surface distribution, coverage and lifetimes of starspots deviate from solar-like patterns as the rotation rate increases. We set up a numerical platform which includes the large-scale rotational and surface flow effects, aiming to simulate evolving surface patterns over an activity cycle for up to 8 times the solar rotation and flux emergence rates. At the base of the convection zone, we assume a solar projected butterfly diagram. We then follow the rotationally distorted trajectories of rising thin flux tubes to obtain latitudes and tilt angles. Using them as source distributions, we run a surface flux transport model with solar parameters. Our model predicts surface distributions of the signed radial fields and the starspots that qualitatively agree with observations.

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Emre Işık, Sami K. Solanki, Natalie A. Krivova, Alexander I. Shapiro. 2018-12-21. Activity variation driven by flux emergence and transport on Sun-like stars. https://arxiv.org/abs/1812.08976

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