PURE ROTATIONAL ATMOSPHERIC LINES OF HYDROXYL

被引：23

作者：

KENDALL, DJW ^{[1
]}

CLARK, TA ^{[1
]}

机构：

[1] UNIV CALGARY,DEPT PHYS,CALGARY T2N 1N4,ALBERTA,CANADA

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 1979年 / 21卷 / 06期

关键词：

D O I：

10.1016/0022-4073(79)90092-X

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Pure rotational line positions of the hydroxyl radical (OH) have been calculated for all vibrational levels expected in the earth's atmosphere (v = 0-9) and for lower rotational quantum numbers J″=0.5-12.5. These positions have been tabulated and compared with those derived from energy levels obtained from precise near-i.r. vibration-rotation bands and show good agreement for low J″ values. A tentative identification has been made of three v = 0 lambda-type doublets in a high-resolution far-i.r. (30-120 cm-1) emission spectrum of the atmosphere obtained at 30 km from a balloon-borne platform. Line strength (SJ′J″) and integrated intensity (Sq cm-2atm-1) values have been derived for these pure rotational transitions as an aid to further work and instrument design. © 1979.

引用

页码：511 / 526

页数：16

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