For LINE1 most of the options described in Sect. 5.4 and 5.5 are valid. There are some further options. Their meaning should be clear ...
MISSING OCCUPATION NUMBERS FROM I MODELS
The occupation numbers of newly considered levels are read from I models (I = max i, see ABUNDi
and MODINi, above) in increasing order.
ITERATIONIN
DEPTHS ii jj kk
The the first kk iterations are carried out only between depth points ii - jj.
MATRIXINVERSION:
MINV
The matrix inversion for the solution of the statistical equations is carried out by the SCILIB routine
MINV. Attention: numerically instable for n > 200,..., 220.
MATRIXINVERSION:
INV
The matrix inversion is done by an own routine.
MATRIXINVERSION:
GIRL
The matrix inversion is done by routine GIRL (single precision). More stable than MINV in some
cases!
MATRIXINVERSION:
GIRLDP
The matrix inversion is done by routine GIRL (double precision).
MATRIXINVERSION:
SGETRF
+
SGETRI
The matrix inversion is done by the LAPACK routines SGETRF and SGETRI.
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
With this option, all C IV line transitions in the atomic data file ATOMS are calculated with the stark
broadening tables by Dimitrijévic (if found there).
If the Dimitrijévic tables shall be used only for selected lines, in ATOMS formula 5 instead of formula
3 or 4 has to be requested.(Sect. 3).
-- The tables (Sect. 8.1) have to be loaded in any case ... --
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
V
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
CPU-TIMETTTTT
maximum CPU time for the job, TTTTT given in seconds
CPU-TIME0.0
This card transfers the total cpu time (then: stop) to LINE1. There are load dependent
variations of the system cpu time which accounts to the user cpu time. These variations can
effect the security time needed by LINE1 in order to complete the iteration, write the model,
etc.
ACCEPTCHANGED
EFFECTIVE
TEMPERATURE
X
LINE1 generally takes Tefffrom the start model (MODIN). For very large models the change of Teff (in
small steps) takes much less times than the complete new calculation with mainly the same (!)
parameters. However, still some iterations are needed ...
ACCEPTCHANGED
ABUNDANCES
LINE1 generally takes the chemical composition from the start model (MODIN) and ignores
ABUNDANCE cards in them input file but for newly implemented elements. For very large models the
change of the abundances (in small steps) takes much less times than the complete new
calculation with mainly the same (!) parameters. However, also still some iterations are needed ...
DOPPLERPROFILES
This option sets the line broadening of all line transitions in the atomic data file ATOMS generally to
Doppler line broadening. This can be used for a quick overview about blends within a selected range.
FORCE USE OF LINE BROADENING TABLES
This option enables the use of line broadening tables instead of approximate formulae during the model
atmosphere calculation.
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
HE
I
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
LINEARIZATIONMODE:
BLOCK-MATRIX
ITERATION,
ION
analogously to LINERIZATIONMODE ... in Sect. 5.4. This card allows to select one single ion to iterate.
LINETEMPERATURE
FROM
FORMATION
DEPTH
The line temperature Tline is by defaults set to . Teff (Sect. 3). The different lines form in very
different depths, i.e. at different temperatures. This card allows to select the temperature at the
formation depth (
= 1) of the line core for every lines as line temperature, respectively.
MIKROTURBULENCE[KM/SEC]
0.0
analogously to Sect. 5.4. LINE1 considers the microturbulence also in the calculation of the line profiles.
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
N
V
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
NEWMAXB= 20*
maximum number of linearizations of the Broyden or Kantorovich iterations
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
O
IV
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
O
V
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
O
VI
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
SI
IV
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV.
USEDIMITRIJEVIC
BROADENING
TABLES
FOR
S
VI
like USEDIMITRIJEVIC
BROADENING
TABLES
FOR
C
IV.
PRINTEQUIVALENT
WIDTH
A small table with the equivalent widths of all selected lines is printed to STDOUT.
Attention: For the calculation of the equivalent widths of the selected lines, the interval
[CONT RED,CONT BLUE] (Sect. 3) is used -- with all included blends
In order to study the equivalent widths of selected lines in detail the blendrange has to be set to a
small-enough value that includes only the components of the multiplet or the atomic data file ATOMS
has to be created with only the requested line transition.
PRINTEQUIVALENT
WIDTH
(LONG)
like PRINTEQUIVALENT
WIDTH but this table includes all frequency points in the interval
[CONT RED,CONT BLUE] and gives additionally the accumulated equivalent widths.
PRINTATOMIC
DATA
FILE
ATOMS_2
print the internally created atomic data file (see above) for the line profile calculations
PRINTMULTIPLET
SPLITTING
LINE1 is able to split the NLTE occupation number of multiplets (see above). With this card all
multiplet splittings are reported.
PRINTVCS
TABLE
PRINTFORMATION
DEPTH
OF
LINES
AND
THRESHOLDS
PRINTFREQUENCY
GRID
FGRID_2
print the internally created frequency grid (see above) for the line profile calculations
PRINTSTATISTICS
OF
FGRID_2
PRINTLEVELS
WITH
LTE
START
VALUES
PRINTLINES
AND
BLENDS
PRINTPROFILE
TYPES
With this option, information about the used line broadening theories for all calculated lines is printed
to STDOUT. The same information is always included in the plot data file PLPRF as far as the
necessary plot option (see below) is active to create it.
PRINTWARNINGS
PLOTEMERGENT
FLUX
LOG
FNUE
/
LOG
NUE
PLOTEMERGENT
FLUX
FNUE
/
NUE
PLOTEMERGENT
FLUX
LOG
FLAM
/
LOG
LAM
PLOTEMERGENT
FLUX
FLAM
/
LAM
PLOTEMERGENT
FLUX
FLAM
/
LAM
INTERVAL: LAMBDAMIN LAMBDAMAX
PLOTLIMIT
TAU=1,ITERATION:EACH
With this option, a plot file PLLP is created which contains the geometrical depth (logarithmical) of the
limit = 1 for the complete frequency grid. It can be plotted with the program PLXY (Sect. 11).
PLOTLINES
PLOTTEMPERATURE
STRATIFICATION,ITERATION:LAST
PLOTTEMPERATURE
STRATIFICATION,ITERATION:EACH