From: Gabriel-Dominique M. <gab...@ma...> - 2011-07-12 03:58:42
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Dear MESA/star users, With in mind the modeling of giant gas planets (which seems to be garnering a healthy amount of attention in this mailing list), would someone know how to: 1. Print log*.data files of the "on-the-side" models calculated while adding a core with relax_M_center and relax_R_center on (as explained in star/public/run_star_defaults.dek)? 2. Add to the log files the composition in terms of the H, H_2, He mass fractions, i.e. track their dissociation and ionisation fractions within the star? I could not find a relevant column name in mesa/data/star_data/profile_columns.list but I may be missing something simple. 3. Get the following columns to print? - chiY ! dlnP/dlnY used in calculate of brunt_B term - dlnY_dlnP ! the actual dlnY/dlnP in the model as used in brunt_B - dlnmu_dr ! for salt-finger mixing - semiconvection_criterion ! positive means stable Including them in profile_columns.list with "use_Ledoux_criterion = .true." and values for alpha_semiconvection and thermo_haline_coeff yields for each a "failed to recognize item" error. Thank you for any help, Gabriel-Dominique Marleau Department of Physics McGill University |