46
J. Orphal et al. / Chemical Physics Letters 458 (2008) 44–47
2.99 Â 10À17 cm moleculeÀ1
.
This value is about 27% lower
of the m4 band of BrONO2 illustrates the strong coupling between
the m3 (809 cmÀ1) and m4 (780 cmÀ1) bands of ClONO2 [22] where
the m4 band is much stronger due to anharmonic interactions.
Concerning the atmospheric detection of BrONO2, Burkholder et
al. [7] have estimated that the m3 band of bromine nitrate around
803 cmÀ1 would have a peak absorbance of 0.04% at an air mass
factor of 10, assuming a column abundance of 2 Â 1013 cmÀ2 at
night. Since the present study shows that the m3 band has the stron-
gest peak cross-section (see Fig. 1) and since it is the only band that
falls into an atmospheric absorption window, it will indeed be very
difficult to detect BrONO2 in the atmosphere by infrared spectros-
copy, even using instruments with high sensitivity, but it might
neverthelesss be useful to look for BrONO2 in atmospheric spectra
with very high signal-to-noise ratio.
No evidence for the existence of the bromine nitrate isomer
BrOONO (bromine peroxynitrite) [30] was found, in agreement
with previous studies. BrOONO is predicted to have strong charac-
teristic absorption bands in the mid-infrared, with the strongest
band in the region 1800–1900 cmÀ1 [31]. However, no absorption
was observed in this range (see Fig. 1), so that the relative amount
of BrOONO in the spectra of the present study must have been less
than 2% of BrONO2.
than the integrated band intensity at 296 K of the m2 band of
ClONO2 centered around 1292 cmÀ1 (3.80 Â 10À17 cm moleculeÀ1
)
[23–26].
The m5 band of BrONO2 centered around 559 cmÀ1 (see Fig. 4)
has an integrated cross-section of 1.02 Â 10À17 cm moleculeÀ1
and has a band contour that is very similar to the m5 band of chlo-
rine nitrate (centered at 563 cmÀ1 [27] with an integrated cross-
section of 1.16 Â 10À17 cm moleculeÀ1 at 296 K [28]). The m1 band
of BrONO2 around 1709 cmÀ1 (see Fig. 5) with an integrated band
intensity of 2.43 Â 10À17 cm moleculeÀ1 carries less than 50% of
the intensity of the m1 band in ClONO2 [23–26], 5.68 Â 10À17
cm moleculeÀ1, in disagreement with the ab initio calculations,
however the origin of this discrepancy remains unresolved. Further
experimental and theoretical work is required to investigate this
issue. The m8 and m4 bands of BrONO2 are very weak, with a progres-
sion of Q-branches around 722–725 cmÀ1 that is possibly due to
coupling of the m8 and m9 (torsional) modes. As already observed
for ClONO2 [29], the P-branch of the m8 band is extremely weak
due to a rather large Herman-Wallis effect. Note that the weakness
4. Conclusions
8.0x10-19
6.0x10-19
4.0x10-19
2.0x10-19
0.0
In this Letter, the integrated band intensities at 296 K of the m1,
m2, m4/m8 and m5 fundamental bands of bromine nitrate have been
determined for the first time. The results have been compared with
recent ab initio calculations and with the band intensities of
chlorine nitrate, ClONO2. No absorptions that would indicate the
presence of the isomer BrOONO (bromine peroxynitrite) were
observed. In conclusion, the data of this work are useful for future
laboratory studies of atmospheric chemistry and may be interest-
ing for the detection of atmospheric BrONO2 using infrared
spectroscopy.
530
540
550
560
570
580
References
Wavenumber in cm-1
[1] D.J. Lary, J. Geophys. Res. D 101 (1996) 1505.
[2] D.J. Lary, M.P. Chipperfield, R. Toumi, T. Lenton, J. Geophys. Res. D 101 (1996)
1489.
[3] D.J. Lary, J. Geophys. Res. D 102 (1997) 21515.
[4] M. Schmeisser, L. Taglinger, Chem. Ber. 94 (1961) 1533.
[5] J.E. Spencer, F.S. Rowland, J. Phys. Chem. 82 (1978) 7.
[6] W.W. Wilson, K.O. Christe, Inorg. Chem. 26 (1987) 1573.
[7] J.B. Burkholder, A.R. Ravishankara, S. Solomon, J. Geophys. Res. D 100 (1995)
16793.
Fig. 4. The m5 band of BrONO2 showing noise due to the limited sensitivity of the
infrared detector in this region. The position and overall contour of this band are
very similar to the corresponding fundamental band in chlorine nitrate [27].
1.2x10-18
1.0x10-18
8.0x10-19
6.0x10-19
4.0x10-19
2.0x10-19
[8] J. Orphal, Ph.D. Thesis, Université de Paris-Sud (Orsay), 1995.
[9] B. Deters, J.P. Burrows, J. Orphal, J. Geophys. Res. D 103 (1998) 3563.
[10] B. Casper, P. Lambotte, R. Minkwitz, H. Oberhammer, J. Phys. Chem. 97 (1993)
9992.
[11] S. Parthiban, T.J. Lee, J. Chem. Phys. 109 (1998) 525.
[12] S. Parthiban, T.J. Lee, J. Chem. Phys. 113 (2000) 145.
[13] P. Zou, A. Derecskei-Kovacs, S.W. North, J. Phys. Chem. A 107 (2003) 888.
[14] R. Soller, J.M. Nicovich, P.H. Wine, J. Phys. Chem. A 105 (2001) 1416.
[15] R. Soller, J.M. Nicovich, P.H. Wine, J. Phys. Chem. A 106 (2002) 8378.
[16] R. Bröske, Ph.D. Thesis, Fachbereich Chemie, Bergische Universität
Gesamthochschule (Wuppertal), 2000.
–
[17] B.J. Finlayson-Pitts, L.M. Wingen, A.L. Sumner, D. Syomin, K.A. Ramazan, Phys.
Chem. Chem. Phys. 5 (2003) 223.
[18] J.-F. Doussin, B. Picquet-Varrault, R. Durand-Jolibois, H. Loirat, P. Carlier, J.
Photochem. Photobiol. A 157 (2003) 283.
[19] H. Kelder et al. (Ed.), Operational Atmospheric Chemistry Missions, Final
Report for ESA Project 17237/03/NL/GS (CAPACITY), ESA-ESTEC, 2005.
[20] M. Schmeisser, W. Fink, K. Brändle, Angew. Chem. 69 (1957) 780.
[21] J. Orphal, M. Morillon-Chapey, A. Diallo, G. Guelachvili, J. Phys. Chem. A 101
(1997) 1062.
0.0
1670 1680 1690 1700 1710 1720 1730 1740
-1
Wavenumber in cm
[22] J.-M. Flaud, J. Orphal, W.J. Lafferty, M. Birk, G. Wagner, J. Geophys. Res. D 107
[23] A. Goldman, C.P. Rinsland, J.-M. Flaud, J. Orphal, J. Quant. Spectrosc. Rad.
Transf. 60 (1998) 875.
[24] G. Wagner, M. Birk, J. Quant. Spectrosc. Rad. Transf. 82 (2003) 443.
[25] J. Orphal, M. Morillon-Chapey, G. Guelachvili, J. Geophys. Res. D 99 (1994)
14549.
Fig. 5. The m1 band of BrONO2 corresponding to the antisymmetric N–O stretching
vibration with dominant b-type structure, and a less pronounced Q-branch from
weak a-type transitions. Part of the high-frequency structure is from the correction
for residual HNO3 absorption which is rather strong in this region. The overlap of
the bands of BrONO2 and HNO3 in this region is a potential source for systematic
errors, both for this work and for future quantitative studies.