Output of the model atmosphere - file MODELO.DAT

This file is a main result of a model atmosphere calculation. following lines only for LNLTE=.TRUE. (NLTE model atmosphere) and NLBG>0 (background atoms are included into model atmosphere calculation) following lines only for LNLTE=.TRUE. (NLTE model atmosphere)
XLUM
stellar luminosity (in ergs)
RADIUS
stellar radius (in cm)
XMSTAR
stellar mass (in g)
TAUMIN
minimum optical depth
TAUMAX
maximum optical depth
LNLTE
T - output of the NLTE model atmosphere
F - output of the LTE model atmosphere
ITER
number of iterations that was necessary for the calculation of the model
LSPHER
T - spherically symmetric model atmosphere
F - plane-parallel model atmosphere

ND
number of depth points of the model

ND lines, for each depth point 1:
(all values are in CGS units)
ID
index of the depth point
DM(ID)
column mass depth (g.cm-2)
DR(ID)
radius (in cm); for a plane-parallel atmosphere 0
TEMP(ID)
temperature (K)
ELEC(ID)
electron density (cm-3)
DENS(ID)
density (g.cm-3)
TAUR(ID)
Rosseland optical depth

this output is only for LNLTE=.TRUE. and NLBG>0
NLBG
number of backgound NLTE levels
LT
T - has no meaning for output, will be used in future model atmosphere input (in the possible next run of the code)
LT
T - has no meaning for output

this output is only for LNLTE=.TRUE. and only for NLBG>0; NLBG/5+1 times ND lines
ID
index of the depth point
BFAC(ID,IL)
departure coefficients (b-factors) for each background NLTE energy level considered

this output is only for LNLTE=.TRUE. and for NL>0
NL
number of NLTE levels
LF
F - has no meaning for output, will be used in future input
LF
F - has no meaning for output, will be used in future input

this output is only for LNLTE=.TRUE. and only for NL>0; NL/5+1 times ND lines

ID
index of the depth point
BFAC(ID,IL)
departure coefficients (b-factors) for each NLTE energy level considered

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Last update: 27.8.2001