1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
|
subroutine ewfind
c******************************************************************************
c This routine predicts equivalent widths for individual atomic lines
c******************************************************************************
implicit real*8 (a-h,o-z)
include 'Atmos.com'
include 'Linex.com'
include 'Mol.com'
include 'Pstuff.com'
include 'Dummy.com'
real*8 taunu0(100)
character*4 ion(3)
data ion/' I ', ' II ', ' III'/
c*****read the parameter file
call params
c*****open the files for standard output and summary curves-of-growth
nf1out = 20
lscreen = 4
array = 'STANDARD OUTPUT'
nchars = 15
call infile ('output ',nf1out,'formatted ',0,nchars,
. f1out,lscreen)
nf2out = 21
lscreen = lscreen + 2
array = 'SUMMARY PREDICTED EW OUTPUT'
nchars = 27
call infile ('output ',nf2out,'formatted ',0,nchars,
. f2out,lscreen)
c*****open and read the model atmosphere
nfmodel = 30
lscreen = lscreen + 2
array = 'THE MODEL ATMOSPHERE'
nchars = 20
call infile ('input ',nfmodel,'formatted ',0,nchars,
. fmodel,lscreen)
call inmodel
c*****open and read the line list file; get ready for the line calculations
nflines = 31
lscreen = lscreen + 2
array = 'THE LINE LIST'
nchars = 13
call infile ('input ',nflines,'formatted ',0,nchars,
. flines,lscreen)
call inlines (1)
call eqlib
call nearly (1)
c*****set some parameters and write header stuff to output
ewsynthopt = +1
mode = 1
call linlimit
lim1obs = lim1line
lim2obs = lim2line
istat = ivcleof (4,1)
write (nf2out,1002) linitle,moditle
c*****run single line computations once to predict the EW for each line
do lim1=lim1line,lim2line
array(1:40) = 'wavelength EP logGF ident'
array(41:60) = ' Abund EWcalc'
lscreen = lscreen + 2
c call prinfo (lscreen)
write (nf2out,1001)
ncurve = lim1
lim2 = lim1
gf1(ncurve) = gf(lim1)
call oneline (1)
widout(lim1) = w(ncurve)
iatom = atom1(lim1)
xab = dlog10(xabund(iatom)) + 12.
ich = idint(charge(lim1) + 0.1)
if (iatom < 100) then
write (array,1003) wave1(lim1), e(lim1,1),
. dlog10(gf(lim1)), names(iatom),
. ion(ich), xab, 1000.*widout(lim1)
lscreen = lscreen + 2
c call prinfo (lscreen)
write (nf2out,1003) wave1(lim1), e(lim1,1),
. dlog10(gf(lim1)), names(iatom),
. ion(ich) ,xab, 1000.*widout(lim1)
else
write (array,1004) wave1(lim1), e(lim1,1),
. dlog10(gf(lim1)), atom1(lim1),
. xab, 1000.*widout(lim1)
lscreen = lscreen + 2
c call prinfo (lscreen)
write (nf2out,1004) wave1(lim1), e(lim1,1),
. dlog10(gf(lim1)), atom1(lim1),
. xab, 1000.*widout(lim1)
endif
c*****(re)compute the line optical depth at line center and the C_d curve
do i=1,ntau
kapnu(i) = kapnu0(lim1,i)
dummy1(i) = tauref(i)*kapnu(i)/(0.4343*kapref(i))
enddo
first = tauref(1)*kapnu(1)/kapref(1)
dummy2(1) = rinteg(xref,dummy1,taunu0,ntau,0.)
taunu0(1) = first
do i=1,ntau
taunu(i) = taunu0(i)
enddo
call cdcalc (2)
do i=2,ntau
taunu0(i) = taunu0(i-1) + taunu0(i)
enddo
write (nf2out,1010)
write (nf2out,1011) (i, rhox(i), xref(i), int(t(i)),
. pgas(i), rho(i), xdepth(i), taulam(i),
. taunu0(i), cd(i), i=1,ntau)
c*****compute layer where continuum optical depth > 1
do i=1,ntau
if (taulam(i) >= 1.) then
xdepthlam1 = xdepth(i-1) + (1.-taulam(i-1))*
. (xdepth(i)-xdepth(i-1))/(taulam(i)-taulam(i-1))
write (nf2out,1013) int(xdepthlam1), i
go to 10
endif
enddo
c compute layer where line center optical depth > 1
10 if (taunu0(ntau) < 1.) then
write (nf2out,1016)
go to 20
endif
do i=1,ntau
if (taunu0(i) >= 1.) then
xdepthnu01 = xdepth(i-1) + (1.-taunu0(i-1))*
. (xdepth(i)-xdepth(i-1))/(taunu0(i)-taunu0(i-1))
write (nf2out,1014) int(xdepthnu01), i
go to 20
endif
enddo
c compute layer where line center plus continuum optical depth > 1
20 do i=1,ntau
if (taunu0(i)+taulam(i) >= 1.) then
tautot1 = taulam(i-1) + taunu0(i-1)
tautot2 = taulam(i) + taunu0(i)
xdepthtot1 = xdepth(i-1) + (1.-tautot1)*
. (xdepth(i)-xdepth(i-1))/(tautot2-tautot1)
write (nf2out,1015) int(xdepthtot1), i
go to 30
endif
enddo
*****compute mean line-center formation level (weight: contribution function)
30 do i=1,ntau
dummy1(i) = xref(i)*dabs(cd(i))
enddo
xrefcdinteg = rinteg(xref,dummy1,dummy2,ntau,0.)
do i=1,ntau
dummy1(i) = dabs(cd(i))
enddo
cdinteg = rinteg(xref,dummy1,dummy2,ntau,0.)
xrefmean = xrefcdinteg/cdinteg
do i=1,ntau
if (xrefmean <= xref(i)) then
xdepthxrefmean = xdepth(i-1) + (xrefmean-xref(i-1))*
. (xdepth(i)-xdepth(i-1))/(xref(i)-xref(i-1))
write (nf2out,1017) int(xdepthxrefmean), i, tauref(i),
. taulam(i)
go to 40
endif
enddo
40 continue
enddo
c*****end the abundance computations
call finish (0)
return
c*****format statements
1001 format (/'wavelength EP logGF ident',
. ' Abund EWcalc')
1002 format (a80)
1003 format (f10.2,f10.2,f10.3,' ',a2,a3,f10.2,f10.1)
1004 format (f10.2,f10.2,f10.3,a10,f10.2,f10.1)
1010 format (' i', 2x, 'rhox', 5x, 'xref', 5x, 'T', 5x, 'Pgas',
. 6x, 'rho', 8x, 'X', 3x, 'taulam', 3x, 'taunu0',
. 8x, 'Cd')
1011 format (i3, 1pe9.2, 0pf6.2, i6, 1p5e9.2, e10.2)
1013 format (i7, 'km (layer ~', i3, ') = physical depth',
. ' for tau(cont) ~ 1')
1014 format (i7, 'km (layer ~', i3, ') = physical depth',
. ' for tau(line center) ~ 1')
1015 format (i7, 'km (layer ~', i3, ') = physical depth',
. ' for tau(cont)+tau(line center) ~ 1')
1016 format (7x,' NOTE: tau(line center) < 1 at deepest',
. ' atmosphere layer')
1017 format (i7, 'km (layer ~', i3, ') = line center ',
. 'formation mean depth; C_d weight'/
. 25x, 'where tauref, taulam =', 2f8.3)
end
|