From: Aaron D. <aar...@gm...> - 2010-03-18 14:13:30
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Hi Zahra, If you want to know where the base of the surface convection zone is in the output, you can look for conv_mx1_top, conv_mx1_bot, etc. in the log file. See the file mesa/data/star_data/log_columns.list for more option. In the profiles, you can use conv_mixing_type where the different values are defined in mesa/mlt/public/mlt_def.f. If that doesn't answer your question, please provide more information about what you want to do and we'll try again. Best wishes, Aaron On Thu, Mar 18, 2010 at 12:45 AM, zahra altaha motahar <zam...@ya...>wrote: > Hi, > I am using the Mesa for study the stellar evolution of low mass stars. > Actually, I have run the code for 1 solar mass and I need to find the base > of convective zone and remove the results for larger radius. > How can I do that ? > I wanted to add my own code but it doesn't work. > Thank you > Zahra > > > ------------------------------ > New Email addresses available on Yahoo! > <http://sg.rd.yahoo.com/aa/mail/domainchoice/mail/signature/*http://mail.promotions.yahoo.com/newdomains/aa/> > Get the Email name you've always wanted on the new @ymail and @rocketmail. > Hurry before someone else does! > > > ------------------------------------------------------------------------------ > Download Intel® Parallel Studio Eval > Try the new software tools for yourself. Speed compiling, find bugs > proactively, and fine-tune applications for parallel performance. > See why Intel Parallel Studio got high marks during beta. > http://p.sf.net/sfu/intel-sw-dev > _______________________________________________ > mesa-users mailing list > mes...@li... > https://lists.sourceforge.net/lists/listinfo/mesa-users > > |