[mesa-users] Zero Brunt-Vaisala freq. in outer regions of GYRE output files
Richard Townsend
townsend at astro.wisc.edu
Tue Jun 10 16:07:45 EDT 2014
On Jun 10, 2014, at 3:03 PM, Bill Paxton <paxton at kitp.ucsb.edu> wrote:
>
> On Jun 10, 2014, at 12:40 PM, Richard Townsend wrote:
>
>> Is there a good reason why the Brunt can’t be calculated in the atmosphere? Since the acoustic cutoff frequency depends on the Brunt, this issue is quite important.
>
> Confusion alert.... try setting this in your &controls inlist:
>
> add_atmosphere_to_pulse_info = .true.
>
> see star/private/create_atm.f and pulsation_info.f for details.
>
> -b
>
>
>
Still confused — in store1_gyre_point (inside pulsation_info.f) the BV is explicitly set to zero. That doesn’t seem right.
cheers
R
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20140610/e6e916b0/attachment.html>
More information about the Mesa-users
mailing list