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my_history_columns_full.list
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109 lines (90 loc) · 3.85 KB
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! some general info about the model
star_age ! elapsed simulated time in years since the start of the run
star_mass ! in Msun units
star_mdot ! d(star_mass)/dt (in msolar per year)
! information about abundance transitions
he_core_mass ! h1 boundary is outermost location where h1 mass fraction is < 0.01
c_core_mass ! he4 boundary is outermost location where h1 mass fraction is < 0.01
o_core_mass ! c12 boundary is outermost location where h1 mass fraction is < 0.01
! conditions near surface
log_L ! log10 luminosity in Lsun units
log_L_div_Ledd ! log10 (luminosity/Eddington luminosity)
log_LH ! log10 power_h_burn
log_LHe ! log10 power_he_burn
log_LZ !log10 total burning power excluding LH and LHe and photodisintegrations
log_Teff ! log10 effective temperature
log_abs_Lgrav !log10 abs(eps_grav_integral) (in Lsun units)
log_R ! log10 radius in Rsun units
log_g ! log10 gravity
log_surf_z ! surface mass fraction in metals
surf_avg_omega ! surf_v_rot/R
surf_avg_v_rot ! km/sec rotational velocity at equator
surf_num_c12_div_num_o16 ! ratio of number fractions, >1 for C star
v_wind_Km_per_s ! wind velocity
! just for massive rotating stars
surf_avg_omega_crit ! critical angular rotational frequency at equator
surf_avg_omega_div_omega_crit ! ratio of angular rotational frequency to critical rotational frequency
surf_avg_v_crit ! critical rotational velocity at equator
surf_avg_v_div_v_crit ! ratio of rotational velocity to critical rotational velocity
surf_avg_Lrad_div_Ledd ! ratio of surface radiative luminosity to eddington luminosity
v_div_csound_surf ! velocity divided by sound speed at outermost grid point
! mass fractions near surface (averaged over the outer 1e−6% of the total stellar mass)
surface h1
surface he3
surface he4
surface li7
surface be9
surface b11
surface c12
surface c13
surface n14
surface o16
surface f19
surface ne20
surface na23
surface mg24
surface si28
surface s32
surface ca40
surface ti48
surface fe56
! conditions near center
log_center_T ! temperature
log_center_Rho ! density
center_degeneracy ! the electron chemical potential in units of k*T
center_omega ! angular frequency of rotation
center_gamma ! plasma interaction parameter
mass_conv_core ! mass of the convective core
! mass fractions near center (averaged over the inner 1e−6% of the total stellar mass)
center h1
center he4
center c12
center n14
center o16
center ne20
center mg24
center si28
! log10 total luminosity for reaction categories (Lsun units)
pp
cno
tri_alfa
burn_c
burn_n
burn_o
c12_c12
!asteroseismic properties
delta_nu ! large frequency separation for p-modes (microHz)
! 1e6/(seconds for sound to cross diameter of star)
delta_Pg ! g-mode period spacing for l=1 (seconds)
! sqrt(2) pi^2/(integral of brunt_N/r dr)
nu_max ! estimate from scaling relation (microHz)
! nu_max = nu_max_sun * M/Msun / ((R/Rsun)^3 (Teff/Teff_sun)^0.5)
! with nu_max_sun = 3100 microHz, Teff_sun = 5777
acoustic_cutoff ! 0.5*g*sqrt(gamma1*rho/P) at surface
! misc
max_conv_vel_div_csound ! maximum value of the ratio of convective vel. to local sound speed
max_gradT_div_grada ! maximum value of superadiabaticity
gradT_excess_alpha ! between 0 and 1; 0 means no MLT++, 1 means MLT++ fully on
min_Pgas_div_P ! beta to check stability
max_L_rad_div_Ledd ! lambda to check stability
e_thermal ! sum over all zones of Cp*T*dm