D.7 Example: A model with hydrogen and helium

T = 100000 K, log g = 7 and number fractions H = 0.9 and He = 0.1
Basic H and He model atoms are provided by TMAD ( http://astro.uni-tuebingen.de/~TMAD). These are combined then in ${AA}/H+He.

D.7.1 ATOMS2


Table 5: Example for the atoms2.job in the case of LTE and NLTE model atmosphere calculations




LTE model NLTE model


#!/bin/sh #!/bin/sh
set +x;. ${HOME}/.jobstart set +x;. ${HOME}/.jobstart
# #
cat > options <<eos cat > options <<eos
AUTO ION H    I   16  16  16 AUTO ION H    I   16  16  16
AUTO ION HE  II   14  32 -14 AUTO ION HE  II   14  32 -14
CBB-AUTO-FILL CBB-AUTO-FILL
CBF-AUTO-FILL CBF-AUTO-FILL
CBX-AUTO-FILL CBX-AUTO-FILL
RBB-AUTO-FILL ( NONE) .RBB-AUTO-FILL ( NONE)
RBF-AUTO-FILL ( NOOP) RBF-AUTO-FILL
RDI-AUTO-FILL ( NONE) RDI-AUTO-FILL ( NONE)
END OPTIONS END OPTIONS
eos eos
# #
cp ${AA}/H+He PROATOM cp ${AA}/H+He PROATOM
expand options PROATOM > SOURCE expand options PROATOM > SOURCE
${BI}/atoms2${sys} ${BI}/atoms2${sys}
ls -l ATOMS ls -l ATOMS
# #
cp ATOMS ${AA}/H+He_lte.atoms2 cp ATOMS ${AA}/H+He.atoms2
# #
set +x; ${HOME}/.jobend ${TMPDIR}set +x; ${HOME}/.jobend ${TMPDIR}



D.7.2 SETF2

D.7.3 Parameter files

D.7.4 LTE2


#!/ bin/sh
set   + x ; .  ${ HOME }/. jobstart
#  do not  edit   the   beginning   of   this   f i l e
# #######################
# #  own  job   following   ##
# #######################
#
#   ------------
#  common  paths
#   ------------
GRP =/ home/rauch/group
#   ---------
#   user   part
#   ---------
#
#   directories   etc .
#
code=lte2
mod = H + He
type=’_lte
#
jobdir= ${JO}/ l t e
f l x d i r= ${JO}/ l t e
#
#  model parameters
H=0.900
HE=0.100
#
GGM =7.00
TTM =0100000
#
name = ${ TTM }_${ GGM }
fn= ${mod}
#
aa = ${ AA }/${fn}${type }. atoms2
f f= ${FF}/${fn}_${ TTM }${type }. setf2
#
if  test  !   -s ${ f f }
then
echo  ${ TTM }   >   SDATEN
echo  PRINT   CHECK   >>   SDATEN
echo  ’1.30E+16’  >>   SDATEN
echo  ’1 ’  >>   SDATEN
echo  ’20 10 ’  >>   SDATEN
cp ${aa}  ATOMS
${BI}/ setf2$ { sys }  <   SDATEN  1>&1
if  test  -f   FGRID
then
cp  FGRID  ${ f f }
chmod 600 ${ f f }
echo  new frequency  grid  created
l s   -l  ${ f f }
else
echo  no new frequency  grid  created
break
fi
rm *
fi
#
MO = ${ MO }/${mod}/ l t e /${name}_${ H }_${ HE }
#
if  test  !   -s ${ MO }
then
#
echo  ’2 1 ${ H } ${ HE}   >  normH
echo  ’2 2 ${ H } ${ HE}   >  normHE
#
HN =‘/home/rauch/bimod/normalize${ sys }  <  normH  2>/dev/ null  1>&1‘
HEN =‘/home/rauch/bimod/normalize${ sys }  <  normHE 2>/dev/ null  1>&1‘
#
cat  >   LDATEN   <<  eos
T   EFF  ${ TTM }
LOG   G  ${ GGM }
DAMP =0.1
ITMAX =100
EPS=1.0E -6
TAU   SCALE   86 90  -2
PRINT   INTEGRATED   EDDINGTON   FLUX,ITERATION:LAST
PRINT   TEMPERATURE   CORRECTIONS,ITERATION:LAST,ALL   DEPTHS
PRINT   MODEL   ATOMS  ( OVERVIEW )
ABUNDANCE   H   ${ HN }
ABUNDANCE   HE  ${ HEN }
eos
#
cp ${aa}  ATOMS
cp ${ f f }  FGRID
#
${BI}/${code}${ sys }  <   LDATEN
#
if  test  -s  MODELL
then
cp  MODELL  ${ MO }
chmod 600 ${ MO }
fi
fi
#
#  do not  edit   the   rest   of   this   f i l e
# ####################
set   + x ;  ${ HOME }/. jobend ${ TMPDIR }

D.7.5 PRO2


#!/ bin/sh
set   + x ; .  ${ HOME }/. jobstart
#  do not  edit   the   beginning   of   this   f i l e
# #######################
# #  own  job   following   ##
# #######################
#
#   ------------
#  common  paths
#   ------------
GRP =/ home/rauch/group
#   ---------
#   user   part
#   ---------
#
#   directories   etc .
#
code=pro2
mod = H + He
#
type =’’
#
jobdir= ${ HOME }/ jobs /pro2
f l x d i r= ${ HOME }/ jobs /pro2
#
IONFRAC = HE
#
# ---  model parameters
#
fn= ${mod}
#
GGM =7.00
#
TTM =0140000
#
H=0.900
HE=0.100
#
name = ${ TTM }_${ GGM }
#
#
aa = ${ AA }/${fn}${type }. atoms2
f f= ${FF}/${fn}_${ TTM }${type }. setf2
#
if  test  !   -s ${ f f }
then
/home/rauch/prep_conts_man${ sys }  >   noCONTS_MAN   <<  eos
5.0  2000.1  0.1
eos
echo  ${ TTM }   >   SDATEN
echo  PRINT   CHECK   >>   SDATEN
echo  ’1.30E+16’  >>   SDATEN
echo  ’1 ’  >>   SDATEN
echo  ’4 10 ’  >>   SDATEN
cp ${aa}  ATOMS
${BI}/ setf2$ { sys }  <   SDATEN  2>/dev/ null  1>&1
if  test  -f   FGRID
then
cp  FGRID  ${ f f }
chmod 600 ${ f f }
echo  new frequency  grid  created
l s   -l  ${ f f }
else
echo  no new frequency  grid  created
break
fi
rm *
fi
#
name = ${name}_${ H }_${ HE }
#
MI = ${ HOME }/models/${mod}/0100000_7 .00 _0 .900 _0 .100 _pro2
MO = ${ HOME }/models/${mod}/${name}_pro2
#
if  test  -s ${MI}
then
#
if  test  -s ${ MO }
then
MI = ${ MO }
fi
#
cat  >   DATEN   <<  eos
COMMENT:  test 4  TMAP
.
.CHANGE   ABUNDANCE   H   ${ H }  MASS   FRACTION
.CHANGE   ABUNDANCE   HE  ${ HE }  MASS   FRACTION
.
.CHANGE   LOGG   $GGM
.CHANGE   EFFECTIVE   TEMPERATURE  $TT
.
LAMBDA =4
.
OCCUPATION   PROBABILITY   FORMALISM   FOR  H1
OCCUPATION   PROBABILITY   FORMALISM   FOR  HE1
OCCUPATION   PROBABILITY   FORMALISM   FOR  HE2
.
OPACITY   PROJECT   RBF   DATA:   START   AT   EDGE
OPACITY   PROJECT   RBF   DATA:  MISSING  HYDROGENIC
.
.STEP   UP  F - VALUES:   MODEL - START:  H1  1.0E -03  1.5  1
.STEP   UP  F - VALUES:   MODEL - START:  HE1  1.0E -04  1.5  1
.STEP   UP  F - VALUES:   MODEL - START:  HE2  1.0E -03  1.5  1
.
ITMAX =20
.ERRSCH =1.0E -4
NEWMAX =2
.ERRNEW =1.E -8
.
RADIATIVE  EQUILIBRIUM:   DIFFERENTIAL/ INTEGRAL   FORM
.INNER   BOUNDARY:   LAMBDA - ITERATION
.LINEARIZE  HYDROSTATIC   EQUATION
.
SKIP  OCCDRVF   AFTER  1ST LINEARIZATION
.
NO   NEGATIVE   POPULATION   NUMBERS  (LTE)
.
.SWITCH   OFF  LINES
.
DEPTH   DEPENDENT  LINE PROFILES,  LINEARIZATION:  FIRST
.
KANTOROVICH =2,  SWITCH  LIMITS  0-->1, 1-->2,  2-->1   :   0.1  0.01  0.5
.SOLVE  STATISTICAL  EQUATIONS   ONLY   RE - SOLVE   PARTICLE   CONSERVATION
.
.NO   TEMPERATURE   CORRECTION
.UNSOELD - LUCY   TEMPERATURE   CORRECTION   DAMP =0.1  0.1   0.1
.UNSOELD - LUCY   PARAMETERS   PRINT  LIMIT  0.1   TAU - WTS   0.1   1.
.
.REDUCE   LOG   CVEC   -1
.
.PRINT   OPTIONS
PRINT   MODEL   ATOMS  ( OVERVIEW )
PRINT   ABUNDANCES
PRINT   MAX.   REL.   CORRECTIONS   EVERY  1  ITERATIONS
PRINT   INTEGRATED   SURFACE   FLUX,ITERATION:EACH
PRINT   CP - TIME /ITERATION,EACH
PLOT   EMERGENT   FLUX,ITERATION:LAST
PRINT   OUTPUT   MODEL ,ITERATION:LAST,DEPTH   INCREMENT:1   (STRUCTURE   ONLY)
PRINT   CORRECTIONS   OF   LAST  LINEARIZATION,ITERATION:LAST,DEPTH   INCREMENT:1
LP - PLOT   OPTICALLY   THICK /THIN,ITERATION:LAST, FILE  ONLY
PLOT  IONIZATION  FRACTIONS  ${ IONFRAC }  -8.5  2.5  -10.0  0.5
.
MACHINE   hostname
eos
#
cp ${MI}  MODIN;  chmod 600  MODIN
cp ${aa}  ATOMS
cp ${ f f }  FGRID
/home/rauch/data/get_OP  >  /dev/ null
#
${BI}/${code}_${mod}${type}${ sys }  <   DATEN
#
if  test  -s  MODOUT
then
echo new_NLTE_ _model _${ MO } created
cp ${MI} ${MI}_ date  +% y -% m -% d}_ % H :% M :%S
cp  MODOUT  ${ MO
chmod 600 ${ MO
l s   -l  ${ MO
if  test  -s  STOP
then
cp  STOP  ${ MO }. converged
fi
else
echo no _new_model _${ MO } created   >  ${ MO }. f a i l e d
touch ${ MO }.failed@$HOSTNAME
echo no _new_model _${ MO } created
if  test  -s  MODTMP
then
echo model _ found _from _ i t e r a t i o n _ before _ f a i l u r e
cp ${MI} ${MI}_ date  +% y -% m -% d_ % H :% M :%S
cp  MODTMP  ${ MO }_tmp
l s   -l  ${ MO }_tmp
fi
fi
#
if  test  -s  IONPLOT
then
cp  IONPLOT  ${ jobdir }/${name}. ${ IONFRAC }_ion
fi
if  test  -s  PLLP
then
cp  PLLP  ${ jobdir }/${name}. lp
fi
if  test  -s  PLOTCORR
then
cp  PLOTCORR  ${ jobdir }/${name}. corr
fi
if  test  -s  PRFLUX
then
cp  PRFLUX  ${ f l x d i r }/${name}. flux
fi
if  test  -s  STRUCTURE
then
cp  STRUCTURE  ${ jobdir }/${name}.T -structure
fi
#
fi
#
#  do not  edit   the   rest   of   this   f i l e
# ####################
set   + x ;  ${ HOME }/. jobend ${ TMPDIR }