SO2 通过 G̃1B1 状态的光解动力学:O(1D2) 和 O(1S0) 产物通道。

Yucheng Wu, Jitao Sun, Zhenxing Li, Zhaoxue Zhang, Zijie Luo, Yao Chang, Guorong Wu, Weiqing Zhang, Shengrui Yu, Kaijun Yuan, Xueming Yang
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引用次数: 0

摘要

二氧化硫(SO2)由自然界和人类活动产生,是地球大气层中的一个重要物种。在太阳系其他行星和卫星的大气中也发现了二氧化硫。几十年来,人们一直在研究二氧化硫的光吸收截面和光解离。本文报告了 SO2 通过 G̃1B1 态光解动力学的实验结果。通过分析时间切片速度图离子成像法的图像,我们得到了 O(1D2) + SO(X3Σ-、a1Δ、b1Σ+) 和 O(1S0) + SO(X3Σ-) 信道,并确定了 O(1D2) + SO(X3Σ-)、O(1D2) + SO(a1Δ)和 O(1D2) + SO(b1Σ+)信道的分支率为 ∼0.3、∼0.6 和∼0.1。SO 产物以电子激发态和振荡激发态为主,它们在行星上层大气中的作用可能尚未被认识到。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Photodissociation dynamics of SO2 via the G̃1B1 state: The O(1D2) and O(1S0) product channels.
Produced by both nature and human activities, sulfur dioxide (SO2) is an important species in the earth's atmosphere. SO2 has also been found in the atmospheres of other planets and satellites in the solar system. The photoabsorption cross sections and photodissociation of SO2 have been studied for several decades. In this paper, we reported the experimental results for photodissociation dynamics of SO2 via the G̃1B1 state. By analyzing the images from the time-sliced velocity map ion imaging method, the vibrational state population distributions and anisotropy parameters were obtained for the O(1D2) + SO(X3Σ-, a1Δ, b1Σ+) and O(1S0) + SO(X3Σ-) channels, and the branching ratios for the channels O(1D2) + SO(X3Σ-), O(1D2) + SO(a1Δ), and O(1D2) + SO(b1Σ+) were determined to be ∼0.3, ∼0.6, and ∼0.1, respectively. The SO products were dominant in electronically and rovibrationally excited states, which may have yet unrecognized roles in the upper planetary atmosphere.
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