[Mesa-users] Mixing types

[Pablo Marchant]

This also depends, for instance, on whether you consider things as an
overshooting region as being radiative. If you just want to check if the
criteria for convection is satisfied you have the following profile output
options

    !sch_stable ! 1 if grada > gradr, 0 otherwise
    !ledoux_stable ! 1 if gradL > gradr, 0 otherwise

On Mon, Jun 15, 2020 at 8:43 AM Francis Timmes via Mesa-users <
mesa-users at lists.mesastar.org> wrote:

> no_mixing = radiative.
>
> fxt
>
>
>
> > On Jun 14, 2020, at 8:10 AM, Roque Caballero via Mesa-users <
> mesa-users at lists.mesastar.org> wrote:
> >
> > Dear all,
> >
> > I've a question concerning the mixing types reported in the history
> file. According to the const_def.f90 file, the possible types are:
> >
> >       ! mixing types
> >       ! NOTE: some packages may depend on the order
> >       integer, parameter :: no_mixing = 0
> >       integer, parameter :: convective_mixing = 1
> >       integer, parameter :: softened_convective_mixing = 2
> >          ! for modified D_mix near convective boundary
> >       integer, parameter :: overshoot_mixing = 3
> >       integer, parameter :: semiconvective_mixing = 4
> >       integer, parameter :: thermohaline_mixing = 5
> >       integer, parameter :: rotation_mixing = 6
> >       integer, parameter :: rayleigh_taylor_mixing = 7
> >       integer, parameter :: minimum_mixing = 8
> >       integer, parameter :: anonymous_mixing = 9
> >
> > Is the "no_mixing" type reported for a particular zone equivalent to
> assume a radiative zone? If that weren't the case, how could I figure out
> which zone/s is/are radiative?
> >
> > Many thanks in advance for your help.
> >
> > Kind regards,
> >
> > Roque
> >
> >
> > _______________________________________________
> > mesa-users at lists.mesastar.org
> > https://lists.mesastar.org/mailman/listinfo/mesa-users
> >
>
> _______________________________________________
> mesa-users at lists.mesastar.org
> https://lists.mesastar.org/mailman/listinfo/mesa-users
>
>

-- 
Pablo Marchant Campos
M.Sc on Astrophysics, Universidad Católica de Chile
PhD on Astrophysics, Argelander-Institut für Astronomie, Universität Bonn
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