Photoabsorption cross-section measurements of 32S, 33S, 34S, and 36S sulfur dioxide for the B1B1-X1A1 absorption band

被引:38
|
作者
Danielache, Sebastian O. [1 ,2 ]
Hattori, Shohei [3 ,4 ]
Johnson, Matthew S. [5 ]
Ueno, Yuichiro [2 ]
Nanbu, Shinkoh
Yoshida, Naohiro [3 ,4 ]
机构
[1] Sophia Univ, Fac Sci & Technol, Dept Mat & Life Sci, Chiyoda Ku, Tokyo 1028554, Japan
[2] Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 152, Japan
[3] Tokyo Inst Technol, Interdisciplinary Grad Sch Sci & Engn, Dept Environm Sci & Technol, Yokohama, Kanagawa 227, Japan
[4] Tokyo Inst Technol, Interdisciplinary Grad Sch Sci & Engn, Dept Environm Chem & Engn, Yokohama, Kanagawa 227, Japan
[5] Univ Copenhagen, Dept Chem, Copenhagen Ctr Atmospher Res, DK-2100 Copenhagen, Denmark
关键词
MASS-INDEPENDENT FRACTIONATION; FOURIER-TRANSFORM MEASUREMENTS; ISOTOPIC FRACTIONATION; TEMPERATURE-DEPENDENCE; 295; K; SO2; NM; PHOTOLYSIS; REGION; MODEL;
D O I
10.1029/2012JD017464
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
We report measurements of the ultraviolet absorption cross-sections of (SO2)-S-32, (SO2)-S-33, (SO2)-S-34 and (SO2)-S-36 recorded from 250 to 320 nm at 293 K with a resolution of 8 cm(-1). This is the first reported measurement of the (SO2)-S-36 cross-section. This work improves earlier measurements of the (SO2)-S-32, (SO2)-S-33 and (SO2)-S-34 cross-sections and is in good agreement concerning fine structure and peak widths, with localized differences at the peak maxima when isotope effects are taken into account. SO2 samples were produced in an identical process via combustion of isotopically enriched S-0, eliminating effects due to variation in oxygen isotopic composition. Peak positions for the rare isotopologues are red shifted relative to the (SO2)-S-32 isotopologue. Starting at the origin the shift increases linearly through the band. A linear shift model based on the spectrum of (SO2)-S-32 was used to estimate the cross-sections of (SO2)-S-33,34,36; the average of the wavelength resolved absolute difference between the modeled and experimental spectra is 77.4, 107 and 139 parts per thousand respectively. While the peak-to-valley amplitude of (SO2)-S-36 tends to be smaller than the other isotopologues throughout the spectrum, integrated band intensities for all isotopologues are conserved to within 4% relative to (SO2)-S-32. The cross-sections were used in a photochemical model to obtain fractionation constants to compare with photochemical chamber experiments. We conclude that planetary atmospheres will exhibit isotopic fractionation from both photoexcitation and photodissociation, and that experiments in the literature have isotopic imprints arising from both the (BB1)-B-1-X(1)A(1) and the (CB1)-B-1-X(1)A(1) bands. Citation: Danielache, S. O., S. Hattori, M. S. Johnson, Y. Ueno, S. Nanbu, and N. Yoshida (2012), Photoabsorption cross-section measurements of S-32, S-33, S-34, and S-36 sulfur dioxide for the (BB1)-B-1-X(1)A(1) absorption band, J. Geophys. Res., 117, D24301, doi: 10.1029/2012JD017464.
引用
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页数:11
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