Speaker
Yori Fournier
(Leibniz Institute for Astrophysics)
Description
We would like to introduce a robust but still under work
method to probe the existence of flux tubes in low mass
stars. This method is based on the ability of numerical
simulations to predict a magnetic-field--rotation relation
for solar-like stars. Thanks to the observations compiled up
to the present day, this theoretical relation can be
compared with the corresponding observed relation.
Investigating and developing such a method could help
disregarding or confirming the the rise of magnetic
flux-tubes from a tachocline.
Primary author
Yori Fournier
(Leibniz Institute for Astrophysics)
