Specfrochimica
kf0.
VOI.
378.
NO
2. PP.
14.(-M.
058c9(47/~2/02014~~3.~/0
1982
PereamonPressbd.
Prinlcdin Great Rricsin
Iron spectrum in the 200-300 nm range emitted by an inductively coupled argon plasma E.
MICHAUD
and J. M. MERMET
Laboratoire de Physicochimie Industriel!e. bt 401. Institut National des Sciences Appliquees. 20. Avenue A. Einstein, 69621 Villeurbanne Cedex, France (Received 3 August 1981) Abstract-In order to make a comparison with the available wavelength tables, the iron spectrum has been studied in the 200-300nm range in ICP-AES. About a hundred lines have been found that have, so far, been unreported. Examples of spectral interferences and conclusions on the field covered by the various tables are given.
1. INTR~DIJ~~I~N THE INDUCTIVELY coupled plasma (ICP) is now sufficiently widespread throughout the world to justify the publication of several wavelength or spectral interference tables[ l-31. It is well known that the level of physical or chemical interferences is usually weak. On the other hand, spectral interferences are important because of the richness of the emitted spectra and the line broadening[4-6]. We have already indicated that a minimum wavelength separation between an interfering line and the analytical line is necessary in order to avoid a partial overlap of the two lines. Two tables have been published dealing with spectral interferences in ICP-AES. One [4] is based on the MIT tables 173and other 131on the NBS tables [8]. In this latter case, BOUMANS has adopted the line intensities determined with the NBS copper arc to the ICP. The choice of the NBS tables results from the homogeneity of the line intensities which facilitates the adaptation to the ICP. On the other hand, the NBS tables are certainly not as complete as the MIT tables. A wavelength table especially devoted to the ICP is in progress [9], but at present, no publication is available. That is why we have thought it useful to study the spectrum of one element in order to check the field covered by the different tables in terms of wavelengths. Iron has been selected because of its rich spectrum. Moreover, Fe is a very common matrix. The 200-3OOnm wavelength range has been chosen because most of the sensitive lines are located in this area. 2. EXPERIMENTAL FACILHTB~ In order to obtain a useful table, a classical ICP system has been used. A 27 MHz Plasmatherm generator has been combined with a pneumatic nebulizer. The only modification is the setting up of a sheathing gas at the exit of the spray chamber UOI [l] R.
K. WINGE.V. J. PEIZIZSON and V. A. FASSEL. Appl. Spectrosc. 33.206 (1979). [2] M. L. PARSONS,A. FOILVTER and D. ANDERSON. An Atlas of Spectral Interferences in ICP Spectroscopy. Plenum, New York (1980). 131 P. W. J. M. BOUMANS, Line Coincidence Tables for Inductively Coupled Plasma Atomic Emission Spectroscopy. Pergamon Press, Oxford (1980). 141 G. F. LARSONand V. A. Fassn~, Appi. Spectrosc. 33,592 (1970). [5] J. M. MERMET and C. TRASSY.Spectrochim. Acta 36B, 269 (1981). 161 A. BATALand J. M. MERMET.Spectrochim. Actu 36B, 993 (1981). [7] G. R. HARRISON, M.J.7’. Wuvefength Tables. MIT Press, Cambridge, Mass./London (1969). 181 W. F. MEGGERS.C. H. CORLISSand B. F. SCRIBNER,Tables of Spectral Line Intensities: Part I, Arranged by Eiernents. Part II, Arranged by Wuveiengths, N.B.S. Monograph 145, U.S. Government Printing Office, Washington, CD. (1975). [91 R. K. WINGE. V. PETERSON,V. A. FASSELand M. FLOYD,Abstracts of the Pittsburgh Conference, Atlantic City, Paper No. 397 (1981). [IO) J. M. MERMET, C. TRASSY and P. RIPOCHE.Developments in Atomic Plasma Spectrochemicat Analyses, Heyden, London/Philadelphia (in press). 145
146
E. MlCHAUDand J. M. MERMET
allowing us the possibility to work a long time with a high salt concentration (> 1 g I-‘). In this case, no deposit is observed in the injector made of alumina. Several iron solutions have been used, especially when non-reported lines have been observed. The different facilities and operating parameters are stated in Table 1. The salt concentration was 1 gl-‘. 3. WAVELENGTH ASSIGNMENT Several wavelength tables have been used to determine the wavelength of the observed lines: the MIT tables [7], the Zaidel tables [ll] and the NBS tables [12], the later one dealing with the wavelengths of 18 elements below 300nm. More than a thousand lines have been observed under compromise conditions for analyses and for a concentration of 1 gl-‘. Among them 100 lines are not reported in the previous tables. On the other hand, several lines reported in the MIT tables have not been observed in this experiment. An example of non-reported lines is shown in Fig. 1. It must be noted that lines of this type always have low intensity.
Table 1. Operating parameters of the ICP system
-
11288.370 1288.373
-
11288 076
Fig. 1. Example of iron spectrum (1 gl-‘) obtained with the operating parameters described in Table 1. including some non-reported lines. [ll] A. N. ZAIDEL, V. K. PROKOFJEV, S. M. RAISKLI,V. A. SLAVNYIand E. A. SHREIDER,Tables of Spectral Lines, IFI/Plenum, New York/London (1970). [I21 C. d. MOORE.An U/trmiolef Muitiplet Table. Circular of the NBS No. 488, Section 2. U.S. Government Printing Office, Washington, D.C. (1952).
iron spectrum in the 200-300 nm range
147
We have only indicated a rough value of the intensity (based on a 1-5 scale) because of the difficulty of establishing an absolute scale of intensities. This scale depends on the excitation temperature for the lines in the same ionization stage, on the electron number density and the observation height for the lines in different ionization stages. Nevertheless, we have given a tentative scale mainly to indicate which lines are intense or weak. An example of a classification is given in Fig. 2. 4. EXPLANATIONOF TABLEOF IRONSPECTRUM The first column indicates the ionization stage and the wavelength in nm when available from a table. If not, the wavelength has been determined by interpolation. The second column gives the intensity with the l-5 scale, the third column indicates the wavelength table used as the reference, with Z for the Zaidel tables, M for the MIT tables, N for the NBS tables and ? for a non-reported line. The order of priority has been the ZAIDEL table, then the MIT table and finally the NBS table. The last column gives the possible interferences (within 0.05 nm) on the sensitive lines from Ref. [l]. An asterisk indicates a line whose wavelength separation with the interfering line is below 0.02nm which means that at least a partial overlap will be observed whatever the resolving power 161. 5. EXAMPLESOF APPLICATIONS We have selected several elements (Mn, Si, Co) whose sensitive wavelengths taken from Ref. [l] are located in the 200-300 nm range. In Tables 2, 3 and 4, we have listed the possible interferences that are observed with an iron solution of 1 gl-’ under the same conditions as mentioned in Section 4, i.e. a separation of up to 0.05 nm with an asterisk for AA ~0.02 nm. From Tables 2, 3 and 4 it may be seen that usually the coverage of the MIT tables is almost complete; only some lines given by these tables
\
293.7810
c
293.690
@.. . ____
Fii. 2. Example of iron spectrum to illustrate the 1-S intensity scale. Table 2. Spectral interference of a matrix of iron (1 gl-‘) according to various tables for prominent lines of Mn Uavelength
(ti)
This work
Ref
17I
Ref 121
II 257.610
I
237.574
+
+
II 259.373
II 259.373 f
+
+
Ref 131
*
* II 260.569
{ I II 260.566 260.530
::I
II 294.920
II 293.930
I
II 293.951 * I 293.908 *
+ +
0 0
279.482 :
II 293.306 I
279.827
I
280.106
0 I
279.778
+
0 0
+ the same interferent wavelength is reported, - no wavelength is reported, 0 this wavelength range is not covered.
l
E. MICHAUD and J. M. MERMET
148
Table 3. Spectral interference of a matrix of iron (1 gl-‘) according to various tables for prominent lines of Si (see footnotes of Table 2 for meaning of symbols) h’avelength
1
251.611
I
212.L12
Thls
(51)
work
Ref
(7
Ref
1
121
ftef
13j
1 25’.657
1
288.158
7
288.16
1
250.690
II
250.701*
1
252.851
{I
25i.625
{I
2h.625
-
*
0 0 1: 252.888
252.817 I
251.432
II
251.438
x
+
0
I
252.411
I
252.429
*
+
0
1
221.667
11
221.706
1
251.920
I
221.0?9
+
0 0 0
II 221.095 *
0 I
221.069 221.110 -
tI I
243.515
II 243.494"
I
220.798
II
I
205.813
I
+
+
220.842
(
0
220_80,
0
205.810”
0
Table 4. Spectral interference of a matrix of iron (1 gl-‘) according to various tables for prominent lines of Co (see footnotes of Table 2 for meaningof symbols) Wavelength
(Co)
This
11 238.892 II
228.616
II
237.862
I1
230.786
II
236.379
wrt
Ref
II 238.863
II
237.853
231.160
Ref
121
+
4
228.615
0
+
*
131
+
+
0
I
{
23i.363
II 231.122 II 231.203 231.129
+
0
+ +
0 0
II 238.146
II 238.324
+
0
II 231.405
II 231.396 *
+
0
II 235.342
II
235.368
II
234.428
II
Ref
0
236.3g4 II
171
+
0
238.636
II
234.426
Ii
231.198
,I
234.739
x
+ 231.484
0 0 0
not observable under our operating conditions. On the other hand, the tables from Ref. [2] cover a small number of lines. In the Line Coincidence Tables [3], based on the NBS tables [8], a great number of lines are not reported as a result of the excitation conditions of the copper arc. Although the MIT tables are more complete in terms of wavelengths, the intensities indicated for arc and spark are not applicable to ICP-AES and, in addition, are not as consistent as the intensities in the NBS tables, which explains BOUMANS’ preference for using the latter as a basis for the first edition of the Line Coincidence Tables. Thus a rather uniform intensity scale could be preserved, but completeness as to the listing of wavelengths had to be sacrificed. There is certainly a need for comprehensive wavelength tables or publications devoted to the ICP SO that tables such as the Line
Iron spectrum in the 20&300 nm range
149
Coincidence Tables [3] may be completed in the next few years. BOUMANS [13] has recently communicated that work aimed at a substantial extension and updating of the Line Coincidence Tables is in progress in his laboratory. In addition to collecting more data on the wavelengths of lines emitted by ICPs, it is necessary to study and classify the hitherto not reported lines that are observed in line-rich spectra and to propose excitation mechanisms for these lines.
r
Table of iron soectrum emitted
a
hm)
I ref
spect.
interf.
by an
argon ICP (I gl-’ iron)
T
Xhm)
Iref
I
300.095
i
2
II 297.051
i
z
I
300.045
I
z
1. 297.010
5
Z
z
I
296.936
i
Z
2
I
296.848
1
z
II 300.006 I
299.951
i
I
299.639
!
299.584 299.60
.
1
?
z
296.690
5
z
M
I
296.626
1N
?
I
296.581
2
z
296.526
i
Z
b II 297.056 x
g I
296.728
N
299.443
i
2
II 296.504
i
Z
299.38
L
?
II 296.463
3
z
r II 296.452 L
II 296.413
2
2
,r II 296.452
299.241
LM
I
299.164
!
z
296.356
LM
I
299.039
s
z
296.259
1M
296.212
1H
II 298.936
1
N
I
298.894
L
M
II 296.127
2
I
298.847
1
Z
I
296.066
1z
I
298.729
3
2
I
296.030
1z
I
298.646
2
Z
I
295.599
3
z
I
z
I
295.968
3
z
II 298.483
j
Z
295.934
1z
I
298.357
5
Z
I
295.737 5
2
I
298.185
3
z
I
295.670 2
Z
2
I
295.465 2
z
I
295.394 i
z
I
295.349 3
z
298.144
5
II 298.096
LM
I
2
298.054 297.987
II 297.935
z
295.23
IM 3
297.805
1z
l?
295.156 1z
z
295.11 I
lb 295.088
l?
295.024 3
z
297.69
1
?
I
297.655
1
z
294.970
I
297.613
2
z
II 294.918 3 294.895 1z 294.843 3
z
294.788 5
z
2
z
I
297.57
1
?
I
297.53
1
?
I
II 297.594
294.713
12 z
In II 294.920 * In II 294.920
1M
I
297.478
1z
I
297.324
5
z
I
297.228
2
z
I
297.19
1
?
II 294.440 4
[13] p. W. J.M.
a II 296.513
z
II 298.555
I
interf.
I
299.527 I
296.81 I
z
II 299.730
-I
spect.
294.570 1z 294.505
2
Z Z ;a I
294.418
BOUMANS, Proc. 9th Int. Conf. Atomic Spectrosc. and 22nd Coil. Spectrosc. Int., Tokyo 1981, Plenary and Invited Lectures, Pure Appl. Chem. to be published.
150
E.Mrc~au~and J.M.MERMET
294.357
1
z
Ga I
294.364 n
[I 291.709 1 z
294.30
1
?
Th II 294.286 x
II 291.615 1 Z
294.263
1
2
Th II 294.286
I
[ 294.134
4
z
1 294.059
2
Z
I
291.216 4 Z
Z
I
291.092 1 2
[I 293.951
2
I 293.908
12
291.430 1 z 291.38 1 ?
kin
II 293.930
Mn II 293.930
II 291.076 1 M Er II 291.036
Z
290.986 1 M Er II 291.036
I 293.690 5
z
t-lg
290.950 2 z
293.645 2
Z
Mg II 293.654 %
L 293.781 3
II 293.602 2
I
293.55
l?
293.437
12
II 293.654 I
290.886 2 Z V II 290.882 x
II 290.786 1 Z
z
I
290.752 2 z 290.72
1 ?
293.381 1M
290.642 1 M
293.181
1z
II 290.612 1 M
293.143
1z
290.538 1 M
293.066
1M
290.416 1 Z
I
292.962 1z
II 290.246 1 Z
r
292.901 4
I I
I
I
292.810
I
I
12
292.788
1M
Ib II 292.781 n
292.755
12
Ib II 292.781
290.191 2 z 290.138 2 Z 290.08
1 ? Cu 11'290.003
290.02 1 ? cu II 290.003 *
2
I
292.579 2
2
II 289.873 1 M
292.536 2
Z
II 289.726 2 Z
292.435
M
II 292.659 4
I
I
z
1
292.385 3
289.941 3 Z
II
292.464
289.669 1 Z
I II
292.402
289.60 1 ?
I
2 40 II 292.339
I
289.504 3 Z Cu II 289.484 e
I
292.329 3
2 40 II 292.339 n
11 289.478 2 Z Cu II 289.484 x
I
292.262 2
2
I
289.450 3 Z Cu II 289.450
I
289.376 1 Z V
II 292.202 292.16C 292.099 I I I
12 1r
289.343 1 M V
12
II 289.283 2 Z V
292.069 2 292.029 291.984
289.248 2 Z
lr?
289.173 1 Z Yb II 289.138
12
I
289.141 1 N Yb II 289.138 H
n rl I 291.832
12
I
291.835 2
z rl I 291.832 R
I
291.802 3
2
2
z
II 291.747
II 289.332 R II 289.332
I
291.904 2 291.882
I
2
II 289.332
:, iii,
;iV
II 288.963
Iron spectrum in the 200-300 nm range
151
Table u
2 Z
286.06
l?
II 288.731
1M
285.97
l?
I
12
I
288.781
288.632
II 288.593 288.54
2
285.948 1H Z
I?
I
285.890 12
II
285.834 3
I
288.373
II 288.370 288.28 288.16
II 288.076
I
3 Z Z l? l?
!, z 1M
287.864
2 H
II 287.680
2 z
287.530
3 z
I
287.488 1z 287.417
3 z 3 z
II 287.238
Z
II 287.234
3 z
II 287.106
II
285.717 2
II
285.693 3
z
Si I 288.158 x
II
285.639 2
z
Na II 288.114
II
285.614 2
z
Na II 288.114
II
285.567 3
z
z
I
285.368 2
I
285.295 1z
Cr II 285.568 I+
II
285.286 1N
I
285.180 4
II
285.064 1N
z Na I 285.301 st Na 1285.281 n
Nb II 287.539 w
Na I 285.301 H Na
Nb II 287.539
II 287.340
287.19
285.741 1N
V II 288.274 P
z
I
I
II
285.43 l?
287.912
287.730 3
z
285.781 12
II 288.478 12
Ga I
287.424 x
285.00 l?
MO II 287.151
2 Z
MO II 287,151
II 287.060
1z
I
286.983
1z
I
286.931
3 z
Tm II 286.923 SE Tm II 286.923
Th II 287.041 )t
II 286.887
3 z 2
I
286.825
1z
I
286.756
1z
286.731
1z
I
286.663
2 z
286.63
l?
Hg I 285.212
Cr II
284.984
E
II 284.961 2
z
Cr II 284.984 Ir I 284.972 s
I
284.871 2
z
II 284.833 2
z
MO II 284.823 BE
II 284.805 3
z
MO IL 284.823 x
II 284.779 2
N
Ko II 284.823
II 284.721 1N
z
I
I 285.281 e
Ir I 284.972
l?
I,lI 286.845
z
I
284.683 1z
I
284.554 3
284.65
l?
Cr II 286.674 w
II 284.497 1N 284.46
z Ta II 284.446
l?
Ta II 284.446 x
II 286.547
1N
Cr II 286.511
I
284.398 4
z
TalI
286.498
1z
Cr II 286.511 n
I
284.363 3
z
Cr II 284.325
286.386
2 z
286.343
2 z
Sn I 286.533 n
286.249
1z
Cr
II 286.190
1N
284.25
II 286.119
1z
II 284.207 1
II 284.332 2 N
II 286.257 R
Cr It 284.325 x ThH
II 284.268 1N
284.446
284.281
ThlI 284.281 I+
l?
ThlI 284.281 N
I52
E. MICHAUD and J. M. MERMET
Table cont.
II
284.135
1
N
I
281.751
2
i
II
284.065
3
2.
II
281.711
1
I
I
284.043
3
z
Sn
I
283.999
281.666
12
II
283.982
3
z
Sn I
283.999
281.59
1
:
II
283.953
3
2
Sn I
283.999
I
281.551
1
I
283.93
2?
I
281.502
1
I
I
283.845
1
M
II
281.361
12
I
283.812
3
2
I
281.329
5
II
283.730
2
2
I
281.231
lk
283.70
l?
II
281.127
1)
I
283.632
2
z
281.08
l?
II
283.572
3
z
281.026
2
2
I
283.546
2
z
280.981
2
2
I
283.475
1N
280.862
12
I
I
283.418
1z
283.38
2?
283.340
IZ
ThlI
283.730
ThlI
283.730
Cr II
n
%
283.563
+
II
I
Pb I
283.306
280.833
12 ll"
I
280.698
4
II
283.310
2
2
Pb I
283.306 x
I
280.607
12
283.244
4
z
ThlI
283.231
II
280.579
12
II
283.156
4
z
II
280.531
12
II
2
283.096
1z
I
280.486
2
2
283.04
I?
I
280.452
4
2
283.01
l?
I
280.402
1M
I
280.362
2
1
280.317
z
280.312
'l z
282.94
l?
I
282.881
2
z
I
282.789
2
2 z
II
282.743
2
I
282.650
12
I
282.599
2
z
I
282.556
4
11
282.459
1
282.43
l?
2
280.27
l?
280.225
1
z
280.19
I?
N
280.028
2
z
I
279.915
2
2
I
279.778
2
z
I
282.328
4
z
II
282.267
1
N
282.23
l?
MO II 281.615
2
280.785
I
N
MO II 281.615
M
Mg II 280.270 Pb I
280.199
Pb I
280.199
Mn I
279.827
MS II 279.806 II
279.665
1M
279.585
12
279.555
1z
282.163
1M
282.101
I
282.022
1M
Hf It 282.022
281.990
IM
Hf II 282.022
I
281.951
L
N
I
279.501
I
281.929
2
z
I
279.470
281.88
l?
M
Mg II 279.553 RU
R
I
279.535
Mg II 279.553
)f
RU
279.535
n
1z
RU
279.535
IZ
Mn I
279.482
n
153
Iron spectrum in the 200-300 nm range
Table cont.
II
279.309 2:
2
II
279.205
I4
II
1
279.146
1
2
279.101
1
H
279.056
1 n
278.980
I
278.948 1
z
I
278.810 4I
z
II
279.394
n
278.726 I
I4
278.678 1
M
278.521 2!
z
L 276.277
z
t II 276.259 n r II 276.259 R
[I 276.244
H
c 276.203
z
[I 276.181
Z
276.090
2
II 275.933
M
lg II 279.079
1 z
I
II
’ II
-
c 275.786
Z
C 275.732
2
LI 275.702
Z
L 275.627
I
2
1
z
!
z
I
278.435 II
z
LI 275.574
II
278.370
i
z
II 275.491
I
278.184
1
z
I
I
278.070
1
z
is I
278.022
II
277.930
b
z
e I
277.983
I
277.884 11 z
I
277.822
1
z
II
277.692
1
2
II
?
275.90
z
275.443
:e I
275.459
:e I
275.459 )t
.u II 275.417 I
275.403
!
z
I
275.369
!
z
I
z
.u II 275.417 n [n I Ln 1
277.640
1
z
II 275.329
277.617
1
z
275.209
1
M
277.5
11
?
275.181
1
z
275.388
.u II 275.417 275.388 x
5r II 275.221 + rh II 275.217 JE
%D II 277.540
II
277.469
1
I
277.323
12
I
275.088
t 2
I
277.283
1 z
I
275.072
!
z
Ib II 275.048
1 z
I
275.014 i
2
ib II 275.048
217.251
2.
II 274.932 5 2
2
I
277.212
I
277.208 3 2
I
II
277.118
I,II 274.698 5 2
II
277.051 12
I
I 12 276.96e
274.582 12
I
) 2 276.93C
2
274.50.E 1
2
II
L 3 276.892
2
I
274.45: 2
2
1 1 1 276.844
I
274.403 3
i
276.811 11
II 274.32C 5
i
I
274.20; 4
i
Cr 11 276.654
II 274.14( 1
i
Cr II 276.654 x
I
1
i
3 11 276.47f
II 273.951 5
;
I
i li 276.43:
I
273.82
I
276.311 -
I
273.76~ 4 -
I
12
! 4 I,II 276.75i I
276.691 L li
i 276.66( II
II 274.648 5
i
1 i
1
rh II 274.756
274.756 12
274.11:
1:
2 Zr II 274.586 *
Zr II 274.256
LU I
274.118 +
E. MICHAUD
154
and J. M. MERMET
Table cont. L
273.731
I
z
t
270.601
!
z
273.548
k
2
II
270.399
i
2
273.489
1
2
Zr II 273.486
L
270.245
1
2
c
273.427
L
z
MIXI
I
270.191
1
2
L
273.400
1
z
@in11 273.435
L
273.358
i
2
Pt I
L
273.435 x
273.396
269.977
1
M
I
269.911
!
z
269.816
1
2 2
273.294
LM
I
II
273.245
LZ
II
269.746
1
11
273.200
LM
I
269.702
12
I
269.628 2 z
273.135
1M
II
273.074
f+ 2.
I
272.882
2
I
272.802
2 z
II
272.754
5
I
272.605 2
II
272.4ae 3 272.42
l?
I
272.3%
4
II
272.27l
269.599
z
~~ II 272.778
I
269.504 1 2
~~ II 272.778
I
269.454 12
ra 11 269.452 K tr I
2. Zr II 272.649 z
z
I
12
Zr II 272.261 R
L,II272.204 12
Nb II 272.198 I
11
Nb II 272.182 R
272.18; LM
269.284 2
2
269.26C 3
2
MIXIT 269.206 w
I
268.98: 12 268.94i 12
272.OYC 5
2
272.02C
I
z
I
271.90; 5
i!
268.78C 1 b
z
268.74
271.841 2 271.77! 12
II
271.65;
II
271.62; 2 271.53;
11
271.44: 5 271.33
I
271.23: 12 271.18~ 2
IX 268.796
II
2
268.475 3
2
Ta
Nb II 271.622
I
268.403 1
I
MO II 268.414
268.29f 1
P
Mn II 271.241 H 2
I
268.15: li
I
268.04: li
I
268.Olf 1
i
I
267.906 3
i i
271.05!
1 2 1n I 271.026
I
270.991
I
If
270.93'
1r
II
270.901 2
2
I
270.85' 2
2
I
270.75
12
II
270.71:
12
I
3
I
z
In I
271.026
267.80: I
Ge I
270.963
267.681: 1) 267.611 1E
Mn If 267.876
Au I
267.595 n
Ta II 267.590 w 267.52( 1
I
268.517
268.221 12
2
I
I,X 270.65
v
1';
II
l?
II
2
Nb II 271.662 x
12
II
268.921 3
268.671 12
1N
I
Th II 269.242 n
269.145 12
I
I
269.423
269.386 1P
I
I
JJ II 270.171 *
12
269.553 12
II
270.651
gb II 269.706
I
z
in I
i
267.32: I i 266.954 1:
-
Iron spectrum
266.90
L
?
T
in the 20&3&l
nm range
11
263.007 2
z z z
I
266.792
1
z
I,ll262.959 3
I
266.697
1
i!
II
II
266.663
3
II
266.466
3 2
II
266.421
262.829 5 262.724 1z
2
II
262.650 2
z
LP,
II
262.567 5
z
12
I
262.337 3
Z
266.256
12
II
262.167 5
z
266.231
12
II
262.069 2
z
266.206
12
II
262.041 3
z
I
266.120
12
II
261.908 2
z
I
266.040
12
I
261.871 12
II
265.825
12
II
261.762 5
I
265.679
12
I
261.542 12
Lu II 261.542 n
I
265.615
12
261.50
Lu II 261.542
266.378 II
265.427
11
II
265.257
11
I
265.171
11
tr
I
266.479 K
in II 266.161
2
l?
I
261.449 12
Pb I
II
261.382 5
Hg I
265.204
I
261.277 12
Ge I
265.158 P
II
261.187 5
2
Be I
265.045 n
2
2
II
265.049
1
I
261.075 3
II
264.946
li
II
260.987 1F
264.843
li
II
260.944 1P
I
264.756
li
II
260.912 12
II
264.508
1)
I
260.858 2
2
II
260.709 5
2
260.683 2
2
i
261.418
I
264.400 2
II
264.201
1)
I
264.165
Ii
Hf II 264.141
II
264.113
11
Hf II 264.141
I
260.566 2
2
Mn II 260.569 x
II
263.955
1
Ir I
II
260.530 2
2
Mn II 260.569
263.764
! 2
II
260.504 12
263.710
1M
I
I
263.648
12
I
263.581
! 2
II
II
263.539
i
I
i
263.971 s
260.631 12
260.487 IZ 260.405 1M
1
ra II 263.558
I
260.356 1z
u II 263.553
II
259.940 5
la II 263.558 %
II
259.857 5 z
Ta II 260.349 x z 259.80915
259.543 IM
263.485
1M
II
263.319
12
I
263.259
12
I
259.404 1z
I
263.224
! Z
II
259.373 3
z
II
263.132
2
II
259.278 3
z
II
263.105
j Z -
SAB Vol. 37, No. 2-E
Sb I
259.643 1M
u II 263.553 it
259.51
l?
Mn II 259.373 n
156
E. MICHAUD
and
J.M.
MERMET
Table cont.
I
259.229
Ge
12
I
259.254
.
2
255.95
l?
255.848
12 1M
II
259.154
4
II
259.054
IM
II
255.750
II
258.879
1M
I
255.686 1z
I
258.798
I
255.630
z z
2
1z
258.795
3
z
I
255.565 2
II 258.588
5
z
II
255.545 2
II
255.41
l? 1z
I
258.454
3
z
II
258.258
4
z
II
255.373
I
258.221
3
z
I
255.318 2
z
P
z
I
255.283
Z
SC II 255.237
II I
258.096
2
257.984
1z
257.941 257.927
255.277 1z
1M
255.266
Z
1z
I
255.109 2
z
II
257.792
4
II
255.068 3
z
z
II
255.002 3
z
I
254.961 4
z
II
254.892 2
z
II
254.859 3
Z
254.808 2
z
II
254.733 2
z
I
254.687 3
z
254.667 3
z
I
257.669
2
z
I
257.574
2
z
II
II
257.437
3
257.321
1M
257.297
2
257.13
l?
Mn
II
257.610
z
M
Zr II 257.139 Y
II 257.084
2
z
II
257.052
2
z
I
254.598 4
z
Z
II
254.521 2
z
z
II
254.497 2
z
Zr II 256.887 n
I
254.471 3
z
Zr II 256.887
I
254.392 3
z
Zr II 256.764
II
254.338 3
z
II
254.273 1z
1z
I
254.210 3
z
256.546
1M
II
254.183 2
z
I
256.456
1z
II
256.347
5
II II
256.977 2
I
256.974
I
256.886 1z
II
256.840
2
I
256.787
1z
II
256.691
4
II
256.622
z
z
z
256.253
5
z
II 256.209
2
z
II
I II
I
254.097 4
z
Se II 256.321
II
254.067 2
z
L
I
253.936 1z
II 256.254
II
253.881 4
z
1M
II
253.850 2
z
256.027
2
z
SC II 256.025 x
II
253.820 2
z
In I 255.991
2
z
256.127
255.328 R
SC II 255.237
I
257.882 1M
I
SC II 255.237
SC II 254.522 x
Ir I
254.397 w
I
253.717 3
z
SC II 256.025
II
253.682 4
Z
In I
I
253.561 4
2 P 1253.565 x
256.015 x
256.015
HgI 253.652
Ironspectruminthe 200-3OOnm range
Tablecont.
z
:I
253.442
I
:I
253.363
/
:
253.401
PI
I
157
251.083
i
251.00
Z
Rh II 251.103 n
1
?
253.314
M
II 250.912
1
z
'noII 250.908 N
253.288
M
I
250.875
1
z
'pmII 250.908
250.849
1
H
2
253.253
z
253.144
M
I
250.790
2
z
II 250.701
1
H
[
253.069
!
z
:I
253.010
!
z
1
252.984
I
2
II 250.643
1M
LI 252.955
b
z
II 250.609
2 2
LI 252.908
I
2
1
z
252.817
I
250.549
12
Sb I
252.852
I
250.507
1z
Si I
252.851
II 250.388
! 2
I
252.744
i
Z
II 250.356
2 2
II
252.710
2
2
II 250.332
2 2
11
252.683
1
n
II 250.239 2 2
t1 252.629 3 2 II
252.539
k 2
L
252.502
2 2
I
252.429 3 2
I
252.367
3 2
I
252.285
5 2
I
IJ1249.889 G Si
I
si I
250.690 R
si I
250.690
Ga I
250.070
2
II 250.093 4 2 2
252.411
Mn II 249.857 Mn II 249.842
249.821 11 II 249.782 2
II 252.219 lk
2
B
I
249.773 it
2
B
I
249.678
249.730 lb
II 252.181 2
2
II 252.109 2
2
I I Rh II 252.053 Y
II 252.068 lk 252.03
250.169 2
Ru II 250.701 1z
l?
249.699 12 249.653 2 249.607
11
Rh II 252.053
LIL249.586 2
2
251.963 2
1
si I
251.920
II 249.523 1E
Be I
249.473
II 251.904 2
2
si I
251.920 I
II 249.489 11
Be I
249.473 n
I
251.810 4
2
I
I
251.766 2
i
II 249.318 4
i
II 251.712 2
i
I
i
I
I
251.657 li
Si I
251.611
Si I
251.432 n
II 251.491 li II 251.438 ? 251.37
i
1 ?
249.394 li
249.198 2 249.17
17
I
249.115 5
i
Rh II 249.077
I
249.064 5
i
Rh II 249.077 e
I
248.975
i Z
I 251.333 1 z
Hf II 251.303
II 248.948
? H
W
L 251.236 !
Hf II 251.269
I
248.895
2 2
Pd II 248.892 x
Rh II 251.103
I
248.814
5 2 -
2
LI 251.176 i Z CI 251.137 lp! -
II 248.923
Ta II 248.870
158
E. MICHAUD and J. M. MERMET
Table cont.
:
248.706
1
z
?t
I
248.111
L
248.669
2
z
?t
I
248.717
L
248.631
)
LI 240.634
Pd II
248.653
3s
248.624
II
n
A
II
246.591
2
M
I
246.515
3
Z
II
246.490
2
Z
LI
246.390
2
Z
246.351
1
2
2 II
246.328
2
z
248.598
s z
I
246.264
4
z
248.57
i
?
I
246.218
2
z
LI 248.507
1
M
II
246.186
3
z
I
I
2
II
246.128
3
Z
246.045
L
248.419
2
I
248.327
j
Z
II
2
M
II
248.265
!
2
II
245.878
3
2
II
248.211
3
Z
I
245.760
3
2
II
248.157
1
M
II
245.664
1
M
II
248.105
1
M
I
247.977
3
Z
I
247.948
‘(
Z
II
247.812
4
M
II
247.748
1
M
I
267.686
2
M
II
241.627
2
M
241.59
1
?
247.57
1
?
247.52
1
?
3
z 2
II
c
I
247.856
Pb I
247.642
+
Pb I
247.638
n
Pb I
247.638
245.589
1
2
Rh II
246.104
Ru 245.651
)t
Ru 245.644
)t
245.556
1
El
II
245.457
2
2
II
245.375
1
2
I
245.34%
2
2
II
245.292
1
I”
245.254
1
r
245.21
1
?
245.16
1
?
II
245.11C
1
F
II
245.02C
2
k
Ga I
245.007
x
II
244.99f
2
F
Ga I
245.007
n
Pd I
244.191
I
I
247.481
II
247.476
I
247.316
2
2
II
244.91E
1
k
I
247.28C
4
2
II
244.87:
1
k
I
247.234
2
Z
244.835
1
F
247.211
1
Z
I
244.111
2
2
II
247.06f
3
2
II
244.72C
2
k
II
247.041
1
M
II
244.64C
2
i
Pd 11 244.618
II
246.971
1
Z
II
244.61C
1
F
Pd II
246.951
2
M
II
244.556
3
2
246.888
i!
Z
II
244.511
1
z
246.811
1I
M
II
244.451
3
z
246.19
1L
?
t
244.387
1
,Il 246.713
II
Z
II
244.384
Z Z
LI 246.667
)
Z
I
244.257
2
z
244.15
1
?
I
244.618
x
Ironspectrum
in the
200-300nm range
159
Tablecont.
II
244.113
1N
II
244.042
2
11 241.331 5 Z ~8 11 241.318 so 241.17 1 ?
t4
I
244 .Oll
2
2
II 241.107 5 Z
I
243.974
2
z
II 241.052 S Z
II
243.930
3
z
II 240.865 1 M
I
243.818
1
z
It
243.710
Ag II 243.779
lZ
240.758 1 M
Z
.iI 243.699 II
243.661 1z
II 240.666 5 Z
I
243.634 1z
II 240.569 1 N
243.586
II 240.488 5 Z lM
II
243.581
Z
II
243.494 2
z
II
243.473 2
II
243.423 12
II
II 240.443 4 Z Si I
243.514 )c
II 240.260 2 Z :u II 240.272 n II 240.225 1 N :u 11 240.272
z
240.152 1 M II 240.027 2 M 'a II 240.063
243.349 1M 243.287 2
t-l
II 239.924 s z
II
243.227 2
z
II 239.866 1 M
I
243.102 12
II 239.671 2 M II 239.562 5 Z
II
243.088 12
II
243.007 3
z
II
242.915 2
Z
II
242.897 1z
II
242.879 1M
II 239.490 2 M Sn I
242.949
I
II 239.709
Ii I
239.452
239.43 1 ? Ii I
239.452
239.31 1 ? If XI 239.336 239.27 1 ?
II
242.837 2
II
242.719 1 M
Z
242.631 1 M
Au I
242.795
Rh II 242.711
II 239.147 3 M II 239.077 1 I
238.997 2 z 238.940 1 M
II
242.568 1M
II
242.536 1 M
II 238.863 5 Z :o II 238.892
II
242.458 2
M
II 238.743 2 M 'y II 238.736 w
II
242.414 3
z
'a II 238.706
II
242.321 2
M
II 238.640 1 M :o II 238.636 t
II
242.268 2
n
I
238.598 1 z :o II 238.636 :e I
I,JI241.988 1M 241.941 1M II II
241.844 1M
11 238.439 4 z
241.787 2
II 238.324 5 Z :o II 238.346
II
z
l?
'e I
241.671 1M
II 238.207 5 Z .r I
241.58
I?
II 238.076 5 Z
241.506
1z
II 237.927 5 z :a 11 237.969
241.70 II
238.578 x
II 238.501 3 Z
238.326 t 238.162
160
E. MICHAUD and J. M. MERMET
Table
II
237.853
M
237.787
cont.
,
:o II 237.862 %
M
234.98
?
4s I
234.984 E
234.94
?
is I
234.984
z
Be I
234.861
2
[I
234.030
II
237.643
I
2
C
234.810
2
II
237.519
i
2
[I
234.629
M
I
237.452
L
2
II
234.533
1
z
Ni I
234.554
ClI
237.362
i
z
234.508
!
2
Ni I
234.554
234.428
i
2
Co II 234.426 R
237.723
Al I I
237.312
II
Al I
237.312
II
234.396
i
II I
237.277 x
II
234.349
i
Z
M
Al
II
237.263
II
234.225
1
237.050
i
z
II
234.196
1 2
236.996
!
2
I
234.157
L N
234.093
LM
234.045
1N
233.958
!
Z
233.800
5
Z
Ga
Rh II 233.47!
II
II
Co II 234.426
2
237.143
I
2
!
I
II
!
237.335
i
236.946
1
2
II
236.93
5
?
II
236.859
5
2 II
236.659
!, Z
236.61C
l?
233.453
1
M
236.585
ll"
233.39
1
?
236.483
5
II
233.280
5
z
236.394
2
2
II
233.131
5
z
11
236.202
4
2
I
232.964
12
II
236.172
2
E
II
232.795
1r
II
236.025
II
232.739
5
5
2 2
II
232.635
1r
232.58
l?
II
II
II
235.995
2
co
II
236.379
x
II
235.955
2
P
II
235.91c
5
2
II
232.557
1F
E
II
232.233
1r
11
I
235.701
2
235.64
1;
235.591
1)
II
232.169
lh
2
I
232.036
3
231.977
1F
231.853
1E
231.76
1
II
231.396
1r
Pb II 235.134
I
231.310
2
Hf II 235.122
II
231.203
1P
235.52
:
235.481
4
i
11
235.44;
3
i
11
II
235.361
11
235.241
11
235.16;
11
235.12!
Sn I
II
237.484
Co II 235.342
231.129
Pb II 235.134 n Hf II 235.122 x
I
233.828
Ag II 233.137
%
2
w II 232.609
Hf II 232.247 w Sr II 232.235 x
11
11
I
235.04( J
II
231.122
I
230.899
2
232.003 232.003
Co II 231.405 n i
Cd I
231.284
Co II 231.160 Co II 231.160 i
-
I
Ni I
s
1) 2
Ni
i
Sb I
231.147 n
Ironspectrum
in the 200-300
nm range
161
Table cont.
1n
I
227.282 1z
230.638
12
In
I
227.207 2
I, II 230.473
12
Ba II 230.424
230.731 I
II
230.606
I
227.178
I
227.086 1z
I
226.910 1z
2
LZ
I
230.358
I
230.342
I
230.168
2
I
230.117
12
II 226.885 1 M Al I
226.922
I
230.059 12
Al I
226.910
I
230.014
2
z
Sn I
226.891 w
I
229.922 2
z
Sn I
226.891
2
I
229.866 1z
II
229.823
I
229.817
I
229.693 1z
II
Ni II 230.300
Z
II 226.856 1M
z Z
I
229.385 1z
I
229.252 2
226.922 %
Al I
226.910 %
I
226.747 3
z
I
226.690 2
z
II 226.625 1M II 226.599 2 Pd II 229.651
1M
229.441 2
Al I
II 226.814 1M
229.667 1z 229.611
I
4
z 2
z
Re I
I
M
226.505 1z
226.555
Te I
226.555
Cd II 226.502 K
229.449 I
226.440 2
z
II 226.323 1M
z
Te I
Al I
226.346
l?
II 226.268 2
I
229.112 1z
II 226.085 2
z
I
229.054 1z
II 226.008 3
z
I
229.006 12
I
z
Te I
I
228.903 1z
z
1s II 225.585 n
229.14
Ta II 228.916 H Rh I
I
228.763 1z
I
228.725 2
z
I
228.409 2
z
I
225.951 2
2
II 225.690 1z
As I
228.812
II 225.643 1M
Cd I
228.802
II 225.569 2
Re I
228.751 H
Re I
228.751
Te I II 225.490 1M
225.548
Ba II 225.473 w
II 225.439 1M
228.366 1z
II 225.407 1z II 225.312 3
z
I
z
1z
I,ll227.792 3
225.902
II 225.779 1z
228.857
228.330 1z 228.308
Ta II 226.230
z
225.187 2
Ni II 225.386
II 225.156 1M
I
227.767 1z
II 225.093 2
z
I
227.710 1z
II 225.017 2
z
I
227.602 3
II 224.906 3
z
I
227.559 1z
Re II 227.525
I
227.519 1z
Re II 227.525 I
I
227.419 12
z
W
II 224.875
Ag II 224.874 224.83
I?
II 224.769 17.
162
E.
MICHAUD
and J.M.
MERMET
Table cont.
II
224.691
Cu II 224.700 R
I
221.406 2
Pb I
II
221.095 12 1
?
II
220.905 I
z
II
220.842 12
224.688 n
Ag II 224.641 11
224.550
1
2
II
224.461
1
M
I
224.391
LM
224.322
12
224.315
LM
224.29
l?
II
Pt 11 224.552 I
221.05
z
Re II 221.426 n Si I
221.089 x
Al I
221,006
Sb I
220.845 x
Si 220.798 220.801 12 Y
II 224.306 H
II
220.615 12
Yr II 224.268
II
220.159 12
Y
II 224.306 e
I
220.072 2
z
Yr II 224.268 n
I
220.039 2
2
224.143
12
I
219.604 3
2
Ta II 219.603 n
224.063
LM
I
219.184 3
2
Cu II 219.226
II
224.034
LM
I
219.120 12
II
223.905
17.
Ta
223.781
l??
Tl I
223.782 I
I
218.918 12
223.75
I?
Tl I
223.782 )t
II
218.768 12
II 223.948
219.077 17.
w
218.935
Sb I
217.581
Be I
217.510
Be I
217.499
Be I
217.510
Be I
217.499 w
223.668
1 r
I
218.719 3
223.631
12
I
218.689 12
II
223.391
2 F
I
218.648 3
II
223.208
1 r
II
218.398 12
II
223.151
12
I
217.809 4
I
223.121
12
II
222.876
12
I
222.817
12
Bi I
222.825
11
222.762
). P OS I
222.798
Cu I
222.778 n
II
222.741
1E
Cu I
222.778
II
222.446
1r
Yb II 222.446 w
II
222.349
It
Ni II 217.467 w
I
222.276
12
Pt I
II
222.249
lb
11
222.116
1 r
II
222.039
2
II
221.989
12
II
221.829
12
cu 11 221.810 w
II
221.706
1P
Si I
221.550
1
II
221.509
12
11
221.441
lt+
II
Pd .I 223.159 R
2
2
2
I,IL217.684 17. 217.640 1 M II
II
II
217.545 3
2
217.485 12
217.372 12
I,II217.321 12
2
II
217.299 12
11
217.268 12
I
217.130 2
221.667
?
217.054 12 II II
cu I 221.458 n Re II 221.426
216.995 12 216.892 12 216.838 12
II
216.788 12
2
217.467 n
Iron spectrum
in the 20&300
nm range
163
Table cont.
II
216.740
1
2
II
216.677
4
2
w
II
216.632
I
216.585
2
2
w
11
216.632
Ni
11 216.556
I,II
_
gn
214.147
1
2
214.09
1
?
213.97c
2
2
216.456
2
2
II
216.434
2
2
I
213.859
1
2
I
216.386
1
Z
II
213,773
1
2
&II
216.337
1
Z
II
213.652
1
2
II
216.202
3
Z
213.596
1
2
I,P
216.158
1
Z
II
216.116
1
Z
I
215.989
1
Z
11
213.399
1
z
I
215.965
1
Z
II
213.202
2
z
I
215.892
1
M
II
213.096
1
2
I,lt
215.848
1
2
Ir
I
215.805
II
213.055
1
z
I
215.779
2
2
Ir
I
215.805
II
213.026
1
z
II
215.647
1
Z
212.797
1
z
II
215.584
1
Z
212.501
1
z
212.47
1
?
II
215.50
1
?
I
215.446
1
Z
P
I
215.408
I
215.300
1
Z
P
I
215.294
Sr
II
II
215.249
1
Z
215.224
1
Z
215.170
1
Z
II
215.284
II
211.905
1
z
*
II
211.819
1
z
x
11
211.696
1
z
Ir
II
215.268
I
211.517
1
z
P
I
215.294
I
211.459
1
z
Sr
II
215.284
I
211.297
1
z
Ir
II
215.268
II
211.072
2
Z
Ir
II
215.268
R
I,lI
211.023
1
z
I
210.986
1
z
I
210.896
2
z
1,lI
215.110
2
Z
II
215.062
2
Z
I
215.018
1
Z
II
214.850
1
z
II
214.772
1
z
Te I
214.725
I$
210.814
1
z
II
214.704
1
z
Te I
214.725
II
210.755
1
z
214.671
1
M
210.713
1
M
II
214.606
1
z
I
210.626
2
z
II
214.519
1
z
Sb I
214.486
I
210.305
1
z
214.445
1
z
Sb I
214.486
I
210.235
2
z
Cd 11
214.438
I
210.080
2
z
Pt
II
214.423
I
210.014
1
z
Cd II
214.438
209.96
1
?
Pt
214.423
209.895
1
2
214.390
1
z
II
n
I
v
II
214.009
Sb I
213.969
n
Zn I
213.856
x
P
I
213.618
P
I
213.618
Cu II
213.598
P
I
213.547
Bi
I
213.363
Yb II
211.667
Ru II
211.068
Bi
211.026
I
Au II I
211.026
Bi
I
211.026
Nb II
210.942
Nb II
210.942
Pt I
210.333
II
n
211.068
Bi
W
x
209.860
n
164
E. MICHAUD and J. M. MERMET
I
209.808
1
II
209.751
1z
II
209.699
1N
II
209.498
1N
II
209.464
1N
II
209.368
I
209.366
3
z
Sb I
209.841
II 202.918 12 II 202.779 202.55
i
w
II 209.475
w
II 209.475
12
1 ?
II 202.074 2 *
201.99
l?
II 201.877 2
z 2
2
MO II 202.030 z
II 201.785 1N
I
209.086 12
LIc 201.709
I
209.038
12
I
208.97
l?
II 201.609 1z
208.90
l?
1 z
201.651 1 z
II 201.550 2
I,JI 208.752 3
2
II 201.327 1z
I
208.412 3
2
II 201.069 2
II
208.091 2
2
II
207.816
1z
II 200.742 1z
II
207.751
1 2
II 200.701 12
2
II 200.771 12
7.
W
207.568 1
II
207.419
12
200.45
1 ?
II
207.315
12
200.30
l?
1 ?
I
II
207.182
12
200.15
207.033
12
II 200.037 2
II
'206.995 1z 206.792
12
206.600
IZ
II
206.367 2 206.20
2
l?
si I
I
205.810
1N
II
205.733
2
z
II
205.527
2
2
II
205.103
3
2
II
204.849
12
204.75
l?
204.724
L
N
204.36
1
?
204.32
1
?
204.069
3
2
203.95
1 ?
203.643
!
203.58
l?
II
203.446
LN
II
203.241
3
I
II
II
2
z
205.813
II 200.807
200.626 12
II
II
MO II 201.511
2
II
II
MO II 202.030
z
As I
200.334
Au I
200.081