[mesa-users] mesa release to synch with new MESA SDK release

[Pablo Marchant]

Warrick, did you update to the new repo? Sourceforge went through some
changes and the address of the mesa repo changed:

http://mesastar.org/documentation/frequently-asked-questions#the-sourceforge-repository-change


On Fri, Mar 22, 2013 at 9:53 AM, Warrick Ball <
wball at astro.physik.uni-goettingen.de> wrote:

> Hi,
>
> I just tried to update to revision 4849 with
>
>  svn co -r 4849
>>
>
> and I get the error
>
> Updating '.':
> svn: E160006: No such revision 4849
>
> I tried pinging mesa.svn.sourceforge.net and that worked fine.  I tried
> updating to the current version and that seemed okay (but might not involve
> checking anything online).
>
>  svn up -r 4798
>>
> Updating '.':
> At revision 4798.
>
> I Googled the error number but didn't find anything useful.
>
> Cheers,
> Warrick
>
>
> ------------
> Warrick Ball
> Postdoc, Institut für Astrophysik Göttingen
> wball at astro.physik.uni-**goettingen.de<wball at astro.physik.uni-goettingen.de>
> +49 (0) 551 39 5069
>
>
>
>
> --
> Date: Thu, 21 Mar 2013 09:48:16 -0700
> From: Bill Paxton <paxton at kitp.ucsb.edu>
> To: "mesa-users at lists.sourceforge.**net <mesa-users at lists.sourceforge.net>[mesa-users at lists.sourceforge"
> <mesa-users at lists.sourceforge.**net <mesa-users at lists.sourceforge.net>>
> Subject: [mesa-users] mesa release to synch with new MESA SDK release
>
>
> Hi,
>
> This new mesa version (4849) has the few small changes to makefile_header
> required to make it work with the new MESA SDK.
>
> There is also a fix provided by Josiah Schwab to allow relax composition
> to work from an arbitrary starting model number rather than only from model
> number 1.
>
> We've added control parameters to set lower limits for rotational
> distortion corrections factors FP and FT.  The old hard-wired limits were
> 0.6 for each; now the defaults are higher (corresponding to less geometric
> distortion):
>
>             FP_min = 0.75
>             FT_min = 0.95
>
> I'm working on element diffusion using the beautiful work of Haili Hu and
> collaborators as a guide. Hopefully this will let us support radiative
> levitation in a future release, but we already have an option to use atomic
> diffusion coefficients according to Paquette et al. (1986) instead of
> assuming pure Coulomb.   The default is still to use pure Coulomb, but you
> can try using the Paquette coeffs by setting diffusion_use_pure_Coulomb =
> .false.
>
> For a preview of where we are headed with element  diffusion, take a look
> at this 2011 paper
>
>   Haili Hu, C. A. Tout, E. Glebbeek and M.-A. Dupret,
>   "Slowing down atomic diffusion in subdwarf B stars: mass loss or
> turbulence?",
>   Mon. Not. R. Astron. Soc. 418, 195–205 (2011)
>
>
>
>     [ Part 3.5.2, Application/PDF (Name: "Hu_11.pdf") 2 MB. ]
>     [ Cannot display this part. Press "V" then "S" to save in a file. ]
>
>
>     [ Part 3.5.3: "Attached Text" ]
>
>
>
>
> Cheers,
> Bill
>
>
>
>
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-- 
Pablo Marchant Campos
M.Sc on Astrophysics, Universidad Católica de Chile
PhD student, Argelander-Institut für Astronomie
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