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

Richard Townsend townsend at astro.wisc.edu
Tue Jun 10 15:13:24 EDT 2014


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

-------------- next part --------------
A non-text attachment was scrubbed...
Name: profile74.data.GYRE
Type: application/octet-stream
Size: 358977 bytes
Desc: not available
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20140610/543e59fb/attachment.obj>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: inlist
Type: application/octet-stream
Size: 722 bytes
Desc: not available
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20140610/543e59fb/attachment-0001.obj>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: inlist_massive
Type: application/octet-stream
Size: 1318 bytes
Desc: not available
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20140610/543e59fb/attachment-0002.obj>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: inlist_massive_defaults
Type: application/octet-stream
Size: 10355 bytes
Desc: not available
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20140610/543e59fb/attachment-0003.obj>
-------------- next part --------------




More information about the Mesa-users mailing list