[mesa-users] Zero Brunt-Vaisala freq. in outer regions of GYRE output files

Richard Townsend townsend at astro.wisc.edu
Tue Jun 10 15:40:30 EDT 2014


Thanks!

I was hoping that adding an atmosphere would fix that — but from Josiah’s post, it seems it won’t.

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.

cheers,

Rich

On Jun 10, 2014, at 2:37 PM, Bill Paxton <paxton at kitp.ucsb.edu> wrote:

> <Convection.pdf>
> BV zero because there's a tiny convection zone at the surface.
> 
> 
> 
> 
> On Jun 10, 2014, at 12:13 PM, Richard Townsend wrote:
> 
>> Hi folks —
>> 
>> I’ve been calculating a set of massive main-sequence models using MESA r6596 (inlists attached), and saving the models in GYRE format for some post-processing.
>> 
>> Looking at these models, it appears that the BV frequency is identically zero in the outer ~40 zones (example attached — see column 9 for N^2). Has anyone else encountered this — and is there a fix?
>> 
>> cheers,
>> 
>> Rich
>> 
>> <profile74.data.GYRE><inlist><inlist_massive><inlist_massive_defaults>
>> 
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