[Mesa-users] perturbation due to magnetic field

[Alex Serebryanskiy]

Dear MESA users,

Is there any way in MESA to introduce magnetic fields of a particular amplitude at the BCZ and the surface in the S-model of the Sun? 
So far what I'm doing is simply introduce \Gamma_1 perturbations at these locations but I'm looking for a more elaborated method to get 
"self-consistent" model. 
 
I will very much appreciate it if someone can give me some hints. 

Sincerely,

Alex

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Aleksander Serebryanskiy, PhD
Fesenkov Astrophysical Institute,
Observatory 23, 050020 Almaty, Kazakhstan 
tel: 8(747)9393892
e-mail: alex at aphi.kz, aserebryanskiy at yahoo.com