[mesa-users] Question

Tue May 31 13:39:47 EDT 2016

:)

fxt


> On May 31, 2016, at 10:16 AM, Aaron Dotter <aaron.dotter at gmail.com> wrote:
> 
> The most useful single thing I've ever found for reading MESA history files and profiles in the terminal:
> 
> less -S history.data
> 
> from the less manual 
> 
>        -S or --chop-long-lines
>               Causes  lines  longer than the screen width to be chopped (trun‐
>               cated) rather than wrapped.  That is, the portion of a long line
>               that does not fit in the screen width is not shown.  The default
>               is to wrap long lines; that is, display  the  remainder  on  the
>               next line.
> 
> And from there you can use the arrow left and right keys to browse horizontally through the file.  Changed my life!
> 
> Aaron
> 
> 
> On Tue, May 31, 2016 at 12:02 PM, Bill Paxton <paxton at kitp.ucsb.edu> wrote:
> Hi Abel,
> 
>> If the problem is that the output file is hard to read because a row with many elements continues on a new line
> 
> Excellent new take on what might be the problem (I have to admit that I don't know what the actual problem is!).   I didn't even think of that since I never look at the text files (I make plots plots and more plots).  But in the rare cases where I do check something in the editor, I can set it so that it doesn't break lines of the file onto separate lines on the screen (same as your nowrap).  Then I simply use horizontal scrolling.   Or if I want to get several values from a row, I'll copy it to a separate file and replace spaces by CR's.  then do the same for the line with the column names and match up names with values.   It might be useful to have a script that would do that automatically, but I don't resort to doing it enough to be motivated to create such a script!
> 
> Perhaps someone else has a trick for doing this.  But unless you need many digits of output, making plots is the better solution in my experience.
> 
> Cheers,
> Bill
> 
> 
> 
> 
> 
> 
> On May 31, 2016, at 7:22 AM, Abel Schootemeijer wrote:
> 
>> Hello,
>> 
>> (Disclaimer: it is very well possible that I completely misunderstood the problem, in that case please accept my apologies :) )
>> 
>> 
>> If the problem is that the output file is hard to read because a row with many elements continues on a new line (instead of a one row per line format), you can for example do
>> 
>> :set nowrap
>> 
>> if you are using vim, to display the file with one row per line, so the elements of one column are displayed right below one another.
>> 
>> Kind regards,
>> Abel
>> 
>> 
>> 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
>> Hi,
>> 
>> The final model file contains only the minimum information needed to specify the structure and abundance.
>> 
>> The final profile model will have the basics and much more.  So you probably should be getting the information you need from that.
>> 
>> Most of the test cases have lines like the following in the inlist &star_job section:
>> 
>> 
>>       save_model_when_terminate = .true.
>>       save_model_filename = 'final.mod'
>> 
>>       write_profile_when_terminate = .true.
>>       filename_for_profile_when_terminate = 'final_profile.data'
>> 
>> The "final.mod" has what is needed to start a new run.
>> The "final_profile.data" has lots of information about that model.
>> 
>> Add to your "profile_columns.list" to add things to the profile.
>> See star/defaults/profile_columns.list for options you can add.
>> For things not built-in, use your run_star_extras to add your own.
>> 
>> e.g., you might pick from these
>> 
>>    ! average charge from ionization module
>>       !avg_charge_H
>>       !avg_charge_He
>>       !avg_charge_C
>>       !avg_charge_N
>>       !avg_charge_O
>>       !avg_charge_Ne
>>       !avg_charge_Mg
>>       !avg_charge_Si
>>       !avg_charge_Fe
>> 
>>    ! average neutral fraction from ionization module
>>       !neutral_fraction_H
>>       !neutral_fraction_He
>>       !neutral_fraction_C
>>       !neutral_fraction_N
>>       !neutral_fraction_O
>>       !neutral_fraction_Ne
>>       !neutral_fraction_Mg
>>       !neutral_fraction_Si
>>       !neutral_fraction_Fe
>> 
>> 
>> b
>> 
>> 
>> 
>> 
>> 
>> 
>> On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
>> 
>> > Sorry for my late reply. I need to extract the abundances and ionizations of the several chemical elements from the final model. I am trying to understand where it is saved and how it is organized. But am unable to find it. I can't understand where one starts and the other ends.
>> 
>> 
>> ------------------------------------------------------------------------------
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>> consuming the most bandwidth. Provides multi-vendor support for NetFlow, 
>> J-Flow, sFlow and other flows. Make informed decisions using capacity 
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> 
> 
> ------------------------------------------------------------------------------
> What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> patterns at an interface-level. Reveals which users, apps, and protocols are
> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> J-Flow, sFlow and other flows. Make informed decisions using capacity
> planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
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> 
> 
> ------------------------------------------------------------------------------
> What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> patterns at an interface-level. Reveals which users, apps, and protocols are 
> consuming the most bandwidth. Provides multi-vendor support for NetFlow, 
> J-Flow, sFlow and other flows. Make informed decisions using capacity 
> planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e_______________________________________________
> mesa-users mailing list
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