Thin flux tube models for star spots

Details Thin flux tube models for star spots Thin flux tube models for star spots

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..417g&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 5, p.417-423

Astronomy and Astrophysics

Astronomy

3

Stars: Activity, Stars: Individual (V410 Tau, Hd 283572, Par 1724, Ab Dor), Stars: Magnetic Fields, Stars: Pre-Main Sequence, Stars: Spots

Scientific paper

The possibility of understanding stellar activity as an up-scaled version of the activity of our Sun is investigated. A theoretical model to explain properties of sunspots is used for explaining observed latitudes of star spots. The model is based on thin-flux-tube simulations that study the path of magnetic flux tubes from their origin in a stellar overshoot layer to photospheric layers. A direct comparison of the simulation results with individual stars is given.

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