[Mesa-users] Evolution simulation questions

[Croxmor Moraga]

Greetings developers comunity.
You will see, the thing is that I am trying to simulate a red giant star in
order the study the mass loss process, following the reimers equations,
which is included between the parameters of MESA. But as it was redifined
by Schröder and  Cuntz; for this process.
I want to study if the presence of the red giant magnetic field, manifested
in MHD turbulences from subsurface convection zones which dissipates and
escape throught magnetic flux within the cool stellar winds; as it was
suggested by Cramer and Saar.
I want to know :in which version of the reimers equation is based the
standard mass loss relation used by MESA, and if is not the one I want to
use, how can I modify that equation in my version of MESA, to use it in my
simulations?

>From beforehand: Thank you and good afternoon.
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