High‐resolution photoabsorption cross‐section measurements of SO2 at 295 K between 198 and 220 nm

High‐resolution photoabsorption cross‐section measurements of SO2 at 295 K between 198 and 220 nm
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295 K 下 198 至 220 nm 之间 SO2 的高分辨率光吸收截面测量

DOI:
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发表时间:
1999
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影响因子:
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通讯作者:
G. Cox
G. Cox
中科院分区:
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文献类型:
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作者:
G. Stark;Peter L. Smith;J. Rufus;A. Thorne;J. Pickering;G. Cox

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二氧化硫是木卫一和金星大气的重要组成部分。精确的光吸收截面数据在这些行星大气的温度是必要的SO2观测和可靠的光化学模型的解释。作为计划的160-300 K范围内的一系列测量的一部分,SO2在295 K,在198-220 nm波长范围内的光吸收截面,已经从真空紫外傅里叶变换光谱仪记录的非常高的分辨率(分辨能力(λ/Δλ)<$450,000)的吸收光谱确定。这些新的测量结果进行了比较,较早的,较低的分辨率(λ/Δλ <$100,000)的光吸收测量在213 K跨越相同的波长区域,与较低的分辨率(λ/Δλ <$100,000)的测量在295 K在一个更有限的区域,并与最近的多普勒限制激光二极管测量在295 K在一个非常窄的波长区域。
SO2 is an important constituent of the atmospheres of Io and Venus. Accurate photoabsorption cross-section data at the temperatures of these planetary atmospheres are required for the interpretation of SO2 observations and for reliable photochemical models. As part of a planned series of measurements over the 160–300 K range, photoabsorption cross sections of SO2 at 295 K, in the wavelength region 198–220 nm, have been determined from very high resolution (resolving power (λ/Δλ) ≈ 450,000) absorption spectra recorded with a vacuum ultraviolet Fourier transform spectrometer. These new measurements are compared with earlier, lower-resolution (λ/Δλ ≈ 100,000) photoabsorption measurements at 213 K spanning the same wavelength region, with lower-resolution (λ/Δλ ≈ 100,000) measurements at 295 K in a more limited region, and with a recent Doppler-limited laser diode measurement at 295 K over a very narrow wavelength region.