From: Daniel K. <ka...@as...> - 2011-12-01 18:51:51
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I'm pleased to report that it works. Thanks, Daniel On Tue, 29 Nov 2011, Bill Paxton wrote: > Hi Daniel, > > Note that brunt_N2 is a standard output, but it is only calculated when calculate_Brunt_N2 is true. > So first check that you've set that flag true in your inlist. > > Then make a plot of the profile of burnt_N2 to see if you get negative values in the convective zone. > > If so, great! If not, please send me your inlist plus a starting model so I can give it a try. > > Good luck, > Bill > > > > On Nov 29, 2011, at 2:55 PM, Daniel Kagan wrote: > >> >> I am trying to calculate the value of N^2 in convective regions of a stellar >> model; while this will be negative, both of the formulas for the Brunt-Vaisala >> frequency ought to work there. However, Mesa doesn't seem to use these formulae >> in convective regions, and N^2 (as opposed to log(N^2)) >> is not a standard output. Is there a way to force Mesa to do this calculation? >> I have tried to do it manually (without success), but is there an easier way? >> >> Thanks, >> Daniel Kagan >> >> ------------------------------------------------------------------------------ >> All the data continuously generated in your IT infrastructure >> contains a definitive record of customers, application performance, >> security threats, fraudulent activity, and more. Splunk takes this >> data and makes sense of it. IT sense. And common sense. >> http://p.sf.net/sfu/splunk-novd2d >> _______________________________________________ >> mesa-users mailing list >> mes...@li... >> https://lists.sourceforge.net/lists/listinfo/mesa-users > |