Earth System Research Laboratory, Chemical Sciences Division, National Oceanic and Atmospheric Administration, 325 Broadway, Boulder, Colorado 80305-3328, USA.
J Phys Chem A. 2009 Dec 10;113(49):13711-26. doi: 10.1021/jp9065345.
The UV photolysis of Cl(2)O(2) (dichlorine peroxide) is a key step in the catalytic destruction of polar stratospheric ozone. In this study, the gas-phase UV absorption spectrum of Cl(2)O(2) was measured using diode array spectroscopy and absolute cross sections, sigma, are reported for the wavelength range 200-420 nm. Pulsed laser photolysis of Cl(2)O at 248 nm or Cl(2)/Cl(2)O mixtures at 351 nm at low temperature (200-228 K) and high pressure (approximately 700 Torr, He) was used to produce ClO radicals and subsequently Cl(2)O(2) via the termolecular ClO self-reaction. The Cl(2)O(2) spectrum was obtained from spectra recorded following the completion of the gas-phase ClO radical chemistry. The spectral analysis used observed isosbestic points at 271, 312.9, and 408.5 nm combined with reaction stoichiometry and chlorine mass balance to determine the Cl(2)O(2) spectrum. The Cl(2)O(2) UV absorption spectrum peaks at 244.5 nm with a cross section of 7.6(-0.5)(+0.8) x 10(-18) cm(2) molecule(-1) where the quoted error limits are 2sigma and include estimated systematic errors. The Cl(2)O(2) absorption cross sections obtained for wavelengths in the range 300-420 nm are in good agreement with the Cl(2)O(2) spectrum reported previously by Burkholder et al. (J. Phys. Chem. A 1990, 94, 687) and significantly higher than the values reported by Pope et al. (J. Phys. Chem. A 2007, 111, 4322). A possible explanation for the discrepancy in the Cl(2)O(2) cross section values with the Pope et al. study is discussed. Representative, atmospheric photolysis rate coefficients are calculated and a range of uncertainty estimated based on the determination of sigma(Cl(2)O(2))(lambda) in this work. Although improvements in our fundamental understanding of the photochemistry of Cl(2)O(2) are still desired, this work indicates that major revisions in current atmospheric chemical mechanisms are not required to simulate observed polar ozone depletion.
Cl(2)O(2)(过氧化二氯)的紫外线光解是催化破坏极地平流层臭氧的关键步骤。在这项研究中,使用二极管阵列光谱法测量了 Cl(2)O(2)的气相紫外线吸收光谱,并报告了波长范围为 200-420nm 的绝对截面 sigma。在低温(200-228K)和高压(约 700 托,氦气)下,使用 248nm 的脉冲激光光解 Cl(2)O 或 Cl(2)/Cl(2)O 混合物,通过三分子 ClO 自反应产生 ClO 自由基,随后通过三分子 ClO 自反应产生 Cl(2)O(2)。Cl(2)O(2)光谱是通过记录气相 ClO 自由基化学完成后获得的光谱获得的。光谱分析使用在 271、312.9 和 408.5nm 处观察到的等吸收点,结合反应化学计量和氯质量平衡来确定 Cl(2)O(2)光谱。Cl(2)O(2)紫外线吸收光谱在 244.5nm 处出现峰值,截面为 7.6(-0.5)(+0.8) x 10(-18)cm(2)分子(-1),其中引用的误差限值为 2sigma,并包括估计的系统误差。在 300-420nm 范围内获得的 Cl(2)O(2)吸收截面与 Burkholder 等人先前报道的 Cl(2)O(2)光谱(J. Phys. Chem. A 1990, 94, 687)非常吻合,并且明显高于 Pope 等人报道的数值(J. Phys. Chem. A 2007, 111, 4322)。对于与 Pope 等人研究中 Cl(2)O(2)截面值的差异,我们讨论了一种可能的解释。根据本工作中 sigma(Cl(2)O(2))(lambda)的确定,计算了具有代表性的大气光解速率系数,并估计了一定的不确定度范围。尽管我们仍然希望对 Cl(2)O(2)的光化学有更深入的基本了解,但这项工作表明,目前不需要对大气化学机制进行重大修订来模拟观察到的极地臭氧消耗。