! Options for Atmospheric Structure 1.298668E+04 [RSTAR] !Stellar radius (in 10^10 cm) - ME: Updated !9.083631E+03 [RSTAR] !Stellar radius (in 10^10 cm) - ME: Updated 20.42964 [RMAX] !Maximum radius (in R*) - ME: Updated 11 [VEL_LAW] !Velocity Law to be used - ME: Updated 10108.97 [VINF] !Terminal velocity (km/s) - ME: Updated - km/s? 0.0 [LSTAR] !Stellar luminosity (Lsun) - ME: Updated 9.28497 [MASS] !Stellar mass (Msun) - ME: Updated but set to du F [DO_CL] !Calculate a model with clumping? NONE [CL_LAW] !Which clumping law is being utilized? 0 [N_CL_PAR] !Number of clumping parameters 9.999515D-01 [HYD/X] !H/X abundance (by number) 8.13D-03 [HE/X] !He/X abundance (by number) 8.13D-03 [IRON/X] !Fe/X abundance (by number) 8.13D-03 [COB/X] !Co/X abundance (by number) 8.13D-03 [NICK/X] !Ni/X abundance (by number) ! Options for continuum freqency grid F [RD_CF_FILE] !Read in continuum frequencies from file 0.00149897 [MIN_CF] !Minimum continuum frequency if calculating NU - 50.000D0 [MAX_CF] !Maximum continuum frequency if calculating NU - 1.10D0 [FRAC_SP] !Fractional spacing for small frequencies 1.05D0 [AMP_FAC] !Amplification factor for large frequency ranges 0.10D0 [MAX_BF] !Maximum frequency spacing close to bf edge T [DO_DIS] !Allow for level dissolution 200.0D0 [dV_LEV] !Spacing in km/s on low side of bf edge. 1.4 [AMP_DIS] !Amplification factor on low side of bf edge. 0.1 [MIN_DIS] !Minimum frequency for level disolution. F [CROSS] !Compute all photoionization cross-sections? 750.0 [V_CROSS] !Max. vel. sep. (km/s) between evaluations of all phot. 750.0 [SIG_GAU_KMS] !Sigma of Gaussian used to smooth photoionizatio 0.5 [EXT_LINE_VAR] !Extent of variation region beyond resonance zon 0.01 [ZNET_VAR_LIM] !Iterate on net rates when ABS(ZNET-1) < ZNET_VA T [WNET] !Iterate on net rates for weak lines. 0.10 [WK_LIM] !Weak line opacity limit ! Computation of radiation field T [USE_J_REL] !Use MOM_J_REL_VN to solve the moment equations ? T [INCL_REL] !Include relativistic terms in the transfer equaton ? T [INCL_ADV_TRANS] !Include advection terms in the transfer equaton ? F [INCL_DJDT] F [USE_DJDT_RTE] T [JC_W_EDD] !Compute continuum intensity using Eddington fac T [JBAR_W_EDD] !Compute line continuum intensity using Eddingto T [DIF] !Diffusion approx. DIFFUSION [IB_METH] T [COH_ES] !Assume coherent electorn scattering? F [OLD_J] !Obsolete F [MIX_COH] !Mix coherencies in variation of J 0.1 [ES_FAC] !How close RJ and RJ_ES to use COH N_ON_J [N_TYPE] !How to handle N in MOM_J_CMF !MIXED [N_TYPE] !How to handle N in MOM_J_CMF INT/INS [FG_OPT] !Solution options for FG ! Accuracy options LOGMON [METHOD] !Use log interp to compute chi.LOGLOG 20000.0D0 [VFRAC_FG] !Maximum velocity spacing along ray in FG_J_CMF_ 20000.0D0 [VFRAC_MOM] !Maximum velocity spacing along ray in MOM_J_CMF T [THK_CONT] !Thick boundary condition for continuum ? T [TRAP_J] !Use trapazoidal wights to compute J ? ! Line options 4.0D0 [TDOP] !Temperature for Doppler profile 4.0D0 [AMASS_DOP] !Atomic mass for Doppler profile 50.0D0 [VTURB] !Turbulent Velocity 6.0 [MAX_DOP] !Max. half-width of resonace zone 1.0 [FRAC_DOP] !Spacing in CMF resonace zone [in Doppler widths 200.0 [dV_CMF_PROF] !Spacing (in km/s) across CMF profile. 300.0 [dV_CMF_WING] !Spacing in e.s. line wings of CMF profile. 2500.0 [ES_WING_EXT] !Ext. of non-coh e.s. wings beyond res. zone (in 3.0 [R_CMF_WING_EXT] !Ext. of coh. e.s. wings beyond res. zone (in Vi ! Options for calculation of spectrum in observers frame 1.1 [OBS_EXT_RAT] !Half-Width of Observed profile in Vinf (>= 1.0) 100.0 [dV_OBS_PROF] !Spacing (in km/s) across observed profile (km/s 400.0 [dV_OBS_WING] !Spacing in e.s. line wings (km/s). 2000.0 [dV_OBS_BIG] !Spacing between lines (km/s). F [FLUX_CAL_ONLY] !Do a flux calculation only? F [EXT_FRM_SOL] !Extend formal solutiona factor of 10 in R T [INS_F_FRM_SOL] !Insert extra frequencies in the formal sol? INT [FRM_OPT] !Methot for formal solution? F [DO_SOB_LINES] !Compute rates for SObolev transitions in flux m F [SOB_FREQ_IN_OBS] !Allow for SOB & CMF lines in defining observers T [LAM_SET] !Swith to SOB for long wavelengths? 5.0E+01 [F_LAM_BEG] !Lambda to begin flux calculation. 5.0E+04 [F_LAM_END] !Lambda to end flux calculation. ! Options controlling the treamnent of bound-bound transitions BLANK [GLOBAL_LINE] !Global switch to indicate handeling of line - M 1.0D-3 [GF_CUT] !Omit lines with gf < GFCUT and lower level 9 [GF_LEV_CUT] !> GF_LEV_CUT 22 [AT_CUT] !Only cut if Atomic # >= AT_CUT 10 [MIN_TRANS] !Minimum # of trans from level before cut. T [THK_LINE] !Thk line boundary condition ? T [CHK_L_POS] !Check for negative line opacity? ESEC_CHK [NEG_OPAC_OPT] !Method for negative opacities in BLANKETING mod F [He2_RES=0] !Set rates in He2 resonance lines to zero? F [ALLOW_OL] !Include line overlap? 50.0 [OL_DIF] !Max velocity dif for overlap (km/s)? ! Physical processes to be included F [INC_CHG] !Include charge exchange reactions? F [INC_TWO] !Include two photon transitions? F [INC_PEN] !Include Penning ionization? - ME: Added F [INC_RAY] !Include opacity due to Rayleigh scattering? - ME: Added F [INC_AD] !Include adiabatic cooling? F [INC_ADV] !Include advection terms in rate equations? - ME: Added T [SCL_LN] !Scale line cooling/heating rates? 0.5 [SCL_LN_FAC] !Factor for determining when to scale H/C rates. ! X-ray options F [INC_XRAYS] !Include X-ray emission ! Options for beginning a NEW model F [RD_IN_R_GRID] !Read in a predetermined R grid ? F [LIN_INT] !Use direct linear interpolation if new model? - T [POP_SCALE] !Scale pops to satisfy abundance Eq. F [IT_ON_T] !Improve initial T estimate by iteration? - ME: 1.0 [T_INIT_TAU] !Tau above which T is set exactly to T(spherical 1.0 [GREY_TAU] !Specify Tau above which T is set to TGREY in it ! Options specifying method of handling lines BLANK [TRANS_HI] !Method for treating Hydrogen lines ? BLANK [TRANS_HeI] !Method for treating He I lines ? BLANK [TRANS_He2] !Method for treating He II lines ? BLANK [TRANS_FeI] !Method for treating Fe I lines ? BLANK [TRANS_Fe2] !Method for treating Fe II lines ? BLANK [TRANS_Co2] !Method for treating Co II lines ? BLANK [TRANS_Nk2] !Method for treating Ni II lines ? F [DIE_AS_LINE] !Treat dielectronic as non-overlapping lines 1000.0D0 [VSM_DIE] !Smoothing velocity (km/s) F,F [DIE_HI] !Include LTDR for HI (Use WI calcs?) F,F [DIE_HeI] !Include LTDR for HeI (Use WI calcs?) F,F [DIE_He2] !Include LTDR for HeII (Use WI calcs?) F,F [DIE_FeI] !Include LTDR for FeI (Use WI calcs?) F,F [DIE_Fe2] !Include LTDR for FeII (Use WI calcs?) F,F [DIE_Co2] !Include LTDR for CoII (Use WI calcs?) F,F [DIE_Nk2] !Include LTDR for NiII (Use WI calcs?) ! Options for assisting convergence F [FIX_NE] !Fixed Electron density ? F [FIX_IMP] !Fix impurity species automatically ? T [FIX_T] !Fixed T ? - ME: Changed F [FIX_T_AUTO] !Automatic variable T - ME: Changed F [FIX_INB_T] !Fix the Temperature at the inner boundary ? 0.0 [TAU_SCL_T] !Fix T for this optical depth. 1.0? ! Options for controlling the linearization TRIDIAG [SOL_METH] !Which Method To solve Matrix Equations (DIAG, T MAJOR [SCALE_OPT] !Scale option (MAJOR, LOCAL, GLOBAL or NONE) ? 1.0D-02 [EPS_TERM] !If maximum fractional % change < EPS terminate 10.0D0 [MAX_LIN] !Maximum fractional change allowed for linearization. 1.0D+05 [MAX_LAM] !Maximum fractional change allowed for LAMBDA iteration. 1.0D+40 [MAX_CHNG] !If maximum % fractional change > MAX_CHNG termi F [COMP_BA] !Compute BA matrix ? T [STORE_BA_INV] !Store the INVERSE of the BA matrix on each iter T [WR_PRT_INV] !Store part of the INVERSE to reduce storage (TR 2 [N_FIX_BA] !Number of iterations to hold BA fixed: T [STORE_BA] !Store the BA matrix for/during each iteration ? 1.0D-04 [BA_CHK_FAC] !If dJ < BA_CHK_FAC*RJ, ignore correction to BA 15.0D0 [FIX_BA] !Switch off BA computation if MAXCH< VAL_FIX_BA 400.0D0 [LAM_VAL] !Do Lambda iterations if MAXCH > VAL_DO_LAM 2 [NUM_LAM] !Number of Lambda iterations if MAXCH > VAL_DO_L F [RD_SOL] !RD in solution vector to update populations ! Options for and enhanced spatial grid F [INC_GRID] !Increase grid size to improve accuracy ? F [ALL_FREQ] !Increase accuracy for all frequencies ? 3.19 [ACC_END] !Increase accuracy for all frequencies < ACC_END 2 [N_INS] !Number of points to be inserted in higher accur 1 [ST_INT] !Interpolate from ? 30 [END_INT] !Interpolate to ? 50 [ND_QUAD] !Quadratic interpolation from ND-? to ND LOG [INTERP_TYPE] !Perform interpolations in LOG or LIN plane 200 [N_PAR] !Rate of BA incrementation by BA_PAR in cont. lo F [COMP_F] !Compute new Eddington factors (f) 1.0D-04 [ACC_F] !Accuracy with which to compute the eddington fa ! Parameters to control Ng acceleration F [DO_NG] !Perform NG acceleration when applicable ? 5.0D0 [BEG_NG] !Percentage accuracy at which to begin NG accele 20 [IBEG_NG] !Iteration at which to begin NG acceleration 60 [BW_NG] !Depth band width for NG acceleration 8 [ITS/NG] !Number of iterations between NG accelerations ( ! SN model options 1 [TS_NO] 3.037652E+01 [SN_AGE] !Age of SN in days - ME: Udated USE_HYDRO [SN_T_OPT] !Method to get T with non-GRID option (USE_T_IN or USE_ F [DO_DDT] T [INC_RAD_DECAYS] !Allow for radiactive decays - ME: Updated - Set to true T [REL_OBS] !Include all reltivistic terms in observer''s frame solution T [REL_CMF] !Include all reltivistic terms in CMF solution for observed i !LOCAL [GAMRAY_TRANS] !NONLOCAL or LOCAL gamma-ray enegry transport - ME: ABS_TRANS [GAMRAY_TRANS] !NONLOCAL or LOCAL gamma-ray enegry transport - ME: ! Additional options for beginning a NEW SN model T [PURE_HUB] !Force a pre hubble flow using age and radii of T [LTE_EST] !Use LTE for the initial estimates - ME: Updated 0.0 [T_EXC] !Minimum temp. when using LTE option - ME: Updated ! Non-thermal model options F [TRT_NON_TE] !Treat non-thermal electrons ! ME test options F [ME_TEST] !ME test run ?