Diode-laser spectrum of isotopic carbonyl sulfide OC34S in the region of 847 cm−1

Diode-laser spectrum of isotopic carbonyl sulfide OC34S in the region of 847 cm−1

JOURNAL OF MOLECULAR SPECTROSCOPY 123, 14-25 (1987) Diode-Laser Spectrum of Isotopic Carbonyl Sulfide 0C34S in the Region of 847 cm-’ GHISLAIN BLA...

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JOURNAL

OF MOLECULAR

SPECTROSCOPY

123, 14-25 (1987)

Diode-Laser Spectrum of Isotopic Carbonyl Sulfide 0C34S in the Region of 847 cm-’ GHISLAIN BLANQUET,F%I?DI?RICDERIE, AND JACQUES WALRAND Laboratoire de Spectroscopic Mol&daire, Fact&b Universitaires Notre-Dame de la Paix, Rue de Bruxelies, 61, B-5000-Namur, Belgium

The Y, band of OC% and its associated hot bands have been measured in the wavenumber range 800-880cm-’ using an enriched sample and a diode-laser spectrometer. Seven bands were assigned to ‘60’2C34Sand three bands to ‘60’2C36S,‘60’3C34S,and ‘sO’2C34Sisotopic species. 0 1987 Academic Press. Inc. I. INTRODUCTION Several authors have studied the spectrum of carbonyl sulfide (OCS) in the microwave and infrared regions. A list of references is found in Jolma et al. (I). Recently, in our laboratory new wavenumber measurements were made with a diode-laser spectrometer in the region of the fundamental v1 for the isotopic form enriched in 34S. Our purpose was to give accurate vibrational and rotational constants to complement previous results. II. EXPERIMENTAL DETAILS

The rovibrational spectra of OCS enriched in 34Swere measured in the region 800880 cm-’ with a tunable diode-laser (TDL) spectrometer. This apparatus has been described in detail in Refs. (2, 3). The absorption cell used in the present work is a multipass White-type cell with 1 m between mirrors. The absorption path length chosen was 52 m. The sample from Isotec-Ohio was enriched in 34S at 90% and the pressure used was usually 0.05 and 0.3 mbar for high-J values. At such low pressure, the pressure broadening of the lines was negligible, so the resolution is given by the Doppler width of the observed lines (N 1.35 X 10e3 cm-‘). The wavenumbers of the observed lines were calibrated by using Maki’s data (4)’ for the vl fundamental band of OCS. The relative calibration of the absorption lines is obtained with a Fabry-Perot etalon with a free range of 0.02985 1 cm-‘. In a previous paper (5), the absolute precision of our wavenumber measurements was estimated to be 0.00 1 cm-‘. A portion of the recorded spectrum near 860 cm-’ is shown in Fig. 1. III. EXPERIMENTAL RESULTS AND ANALYSIS The investigated region, 800-880 cm-‘, was covered with three Pb-Sn-Te diodes. One hundred and seven spectra with a mean range of 0.4 cm-’ were recorded and ’ A. G. Maki, private communication, 0022-2852187 $3.00 Copyright 0

1987 by Academic Press, Inc.

AU rights of reproduction in any form resewed.

1983. 14

DIODE-LASER SPECTRUM

I

-r

I

11

I

I I

15

OF OC%

I

I

II

III

IIIII

3

FICHIER: 229805 DIODE: 4 TEMP

:

1.0624 COURANT: i

I1

6259

DIAL

:

178 RUN ImA)

:

170

2

AEFER : OCS MOLECULE ocs

34

1

FREQUENCE: 859.7747

‘j

, /’ , , j(‘)( , , , ,‘I, / / / , , , ,’ , /

, , ,I ; , I, ,I / ) I, I, j

FIG. 1. Example of a treated spectrum: (1) Spectrum of OC3“S. (2) Smoothed etalon fringes. (3) Reference spectrum (OCS) with true profile.

more than 1500 lines measured. Almost all the lines were assigned to the transitions given in Table I. The remaining lines belong to transitions of normal isotopic species; these lines are not reported here. The identification of the bands and the assignment TABLE I Statistics for the Measured OCS Bands

16

BLANQUET, DERIE, AND WALRAND TABLE II Wavenumbers (cm-‘) for ‘60’2C%3 Transitions

-6 7

66 -66 c,

DIODE-LASER SPECTRUM OF 0C34S TABLE III Wavenumbers (cm-‘) for ‘60’2CwS Transitions

17

18

BLANQUET, DERIE, AND WALRAND TABLE IV Wavenumbers (cm-‘) for ‘60’2C’4STransitions

* -2 3

-7 8

-44

-2 -:: 4,

DIODE-LASER

TABLE

SPECTRUM

19

OF 0C”S

IV-Continued

of J quantum numbers were performed with the help of microwave data and also constants calculated by Fayt2 Loomis-Wood diagrams were very helpful in extending the assignment especially to lines belonging to very weak transitions. Approximately 95% of the measured lines were identified. Tables II-VIII list the observed wavenumbers of the assigned lines and also the differences between the calculated and the observed values. The diodes used cover practically the entire region studied except for small gaps in frequency where no laser modes were available. This explains most of the missing J values in the tables. The wavenumbers of the v, lines of OC34S have been given by Jolma et al. (6) and are not presented here. For the analysis of the transitions, we used a least-squares program based on the relation T”=G”+B”[J(J+

l)-Z’]k($qvJ(J+

1)~D”[J(J+

1)-12]2~(f)qj~J2(J+

1)’

(1)

where G, is the vibrational term, B, is the rotational constant, D, is the centrifugal *J. G. Lahaye,

R. Vandenhaute,

and A. Fayt, private communication,

1986.

20

BLANQUET,

DERIE, AND

WALRAND

TABLE V Wavenumbers (cm-‘) for OCS Transitions

0.0003 -0.000,

0.0002 0.000, 0.0006

distortion constant, and the I-doubling constants qvand qtiare the differences between the B and D constants for the component levels of the 1 doublets. In accordance with the convention of Brown el al. (7) the positive sign applies to theflevels and the negative sign to the e levels. The band center of the observed transition is given by

The rovibrational parameters v. , A B, and AD were determined for the fundamental zq and associated hot bands of 0C34S and are listed in Table IX. The rovibrational constants derived from the fits of other isotopic bands are presented in Table X. For this analysis, the rotational constants B” and D” of the molecule in the lower state

DIODE-LASER

SPECTRUM OF OC34S TABLE VI

Wavenumbers (cm-‘) for “O’%“S Transitions

4; ‘2 ‘3 “

‘5 ‘6 ‘7 :: 50 ::

21

22

BLANQUET,

DERIE, AND WALRAND TABLE VII

Wavenumbers (cm-‘)

have been

for ‘60’2C”STransitions

constrained to values obtained previously by various authors from microwave and heterodyne measurements (see footnotes to tables). In these tables, the constants B, AB, and 0, AD are given respectively in 10e5 and lo-* cm-‘. The effect of the higher order distortion constant (-I&) was found to be negligible in the fitting of experimental data. This is due to the fact that not very high J values have been observed and actually the H contribution is included in Beff and Deff constants. For the + transition, only a few lines have been measured, explaining the relatively poor precision of the analysis.

DIODE-LASER SPECTRUM OF 0C34S TABLE VIII Wavenumbers (cm-‘) for OCS Transitions

23

24

BLANQUET, DERIE, AND WALRAND TABLE IX Rovibrational Constants (cm-‘) Determined for Carbonyl Sulfide ‘60’2C34S Transition

El"(10-5&')

vo(cm -1)

lo”o-oo”o

a47.739319

a

F lllo-oooo 20°0-OOOO

6D(lo-acm-')

19789.8034b

-5a.9a77

4.1405b

0.07909

19a34.3754b

-53.564'

4.2099b

0.1212'4

F

F

E

la

i9ai4.1321b

-54.9919

4.196ab

0.1044

a41.0va412

19730.8073'

-60.143 10

4.2186'

0.0816 la

a34.a4536'4

19759.1025'

-56.272

4.2592'

0.109364

197a0.ai02c

-54.aa321

4.3009=

0.1177

f9a5a.4092d

-50.571'9

5.0312d

0.2944

E 1220-0220

D"(l0-acm-')

a41.1066oa E

21'0-11'0

bB(l0-5cn-')

15

834.96808

23

20

51 43

19a55.4092d

-50.592

4.2900d

0.11204a

12°0-0200

a34.5i03020

,9a51.2709d

-51.746 22

3.5014d

-0.0612 46

1330-0330

829.24178 27

19892.2222'

-47.339952

4.60820d

0.2208 187

a The standard deviation in the last digit. b From Jolma et al. (I). ’ From Wells et al. (8). d From Tanaka et al. (9).

For OC34S, the comparison with levels reported in the literature is given in Table XI and it shows a good agreement. Since previous values were obtained by very precise methods, such as heterodyne techniques and Fourier transform spectroscopy, the agreement confirms the good precision of our measurements. For 0C34S, our results have already been included by Fayt* in his general rovibrational analysis and the values calculated by Fayt are very close to our experimental results. TABLE X Rovibrational Constants (cm-‘) Determined for ‘6012C33S,‘6012C36S,‘60’3C34S,and ‘sO’2C3% Isotopic

form

16012C33S

Transition

vo(cm -I)

a53.2007a(11)a

loOo-OOOO F

B"u0-5cm-'~

6Ex10-5cm-'>

D*~uO-acm-'l

6D(10-8cm-')

20030.2446b

-59.740(14,

4.23a7b

0.0822(28)

20075.4674b

-53.958(20)

4.3134b

0.1501~62~

846.42611~11~

11'0-OOOO

20054.7533b

-55.490(21)

4.2999b

0.1259(62)

20°0-lo00

846.36622(19)

19970.5119b

-60.902(40)

4.3234b

0.0820(150)

16012C36S

loOo-OOOO

837.56641(15)

l9345.6903'

-57.575<14)

3.9654'

0.0709(27)

16013C34S

~o"o-ooOo

843.1312(15)

19719.4191=

-58.646<13,

4.1291'

o.oaa4<21)

la012t34S

loOo-ooOo

826.65071(33)

18546.0543C

-52.695(54)

3.5954C

0.0450~173~

E

The standard deviation in the last digit is given in parentheses following each value. b Burenin et al. (10). ’ Burenin et al. (11). '

DIODE-LASER

SPECTRUM

OF 0C34S

25

TABLE XI

Comparison with Previously Observed Values TRANSITION

lo%oo"

11'0-01'0

20%lODO

CONSTANTa

JKHb

UPMC

This

work

yo

847.73932

847.73936

8’

19730.818

19730.807

19730.816

D’

4.2228

4.2186

4.2195

yo

a41.10678

841.10660

E’F

19780.810

~9780.811

B’E

19759.102

19759.141

D’F

4.3010

4.3311

D’E

4.2592

4.3010

a41 .oi751

841.01784

“Q 8’ D’

au.73931

19670.692

19670.664

4.2186

4.2195

* Band center (cm-‘), upper level constant 3’ (IO-’ cm-‘), upper level constant D’ (IO-’ cm-‘) b Jolma, Kauppinen, and Homeman (6). ’ Wells, Petersen, and Maki (8).

ACKNOWLEDGMENTS

The authors thank Dr. M. Dang-Nhu for suggesting valuable modifications in our analysis program and Dr. A. Fayt for helpful discussions and providing his calculations prior to publication. RECEIVED:

July 2 1, 1986 REFERENCES

1. K. JOLMA,V. M. HORNEMAN,AND J. KAUPPINEN,J. Mol. Specfrosc. 113, 167-174 (1985). 2. P. HERBIN,G. BLANQUET,J. WALRAND, AND C. P. COURTOY,J. Mol. Spectrosc. 104,262-270 (1984). 3. G. BLANQUETAND J. WALRAND, Computer Enhanc. Spectrosc. 2, 135-140 (1984). 4. J. S. WELLS, F. R. PETERSEN,A. G. MAKI, AND D. J. SUKLE,Appl. Optics 20, 1676-1684 (198 I). 5. E. BAETEN,G. BLANQUET,J. WALRAND, AND C. P. COURTOY,Canad. J. Phys. 62,1286-1292 (1984). 6. K. JOLMA,J. KAUPPINEN,AND V. M. HORNEMAN,J. Mol. Spectrosc. 101, 300-305 (1983). 7. J. M. BROWN, J. T. HOUGEN, K. P. HUBER, J. W. C. JOHNS,I. KOPP, H. LEFEBVRE-BRION, A. J. MERER,D. A. RAMSAY,J. ROSTAS,AND R. N. ZARE, J. Mol. Spectrosc. 55, 500-503 (1975). 8. J. S. WELLS,F. R. PETERSEN,AND A. G. MAKI, J. Mol. Spectrosc. 98,404-412 (1983). 9. K. TANAKA, H. ITO, K. HARADA, ANDT. TANAKA, J. Chem. Phys. 80,5893-5905 (1984). 10. A. V. BURENIN, A. N. VAL’DOV, E. N. KARYAKIN, A. F. KRUPNOV, AND S. M. SHAPIN, J. Mol. Speclrosc. 87, 3 12-3 15 ( I98 I). II. A. V. BURENIN, E. N. KARYAKIN, A. F. KRUPNOV, S. M. SHAPIN, AND A. N. VAL’DOV, J. Mol. Spectrosc. 85, l-7 ( 198 I ).