IMPROVED LINE PARAMETERS FOR OZONE BANDS IN THE 10-MU-M SPECTRAL REGION

被引:27
|
作者
FLAUD, JM
CAMYPEYRET, C
RINSLAND, CP
DEVI, VM
SMITH, MAH
GOLDMAN, A
机构
[1] COLL WILLIAM & MARY,DEPT PHYS,WILLIAMSBURG,VA 23185
[2] UNIV DENVER,DEPT PHYS,DENVER,CO 80208
[3] CNRS,MOLEC & ATMOSPHER PHYS LAB,F-75252 PARIS 05,FRANCE
[4] NASA,LANGLEY RES CTR,DIV ATMOSPHER SCI,HAMPTON,VA 23665
来源
APPLIED OPTICS | 1990年 / 29卷 / 25期
关键词
D O I
10.1364/AO.29.003667
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
A complete update of spectroscopic line parameters for the 10-/xm bands of ozone is reported. The listing contains calculated positions, intensities, lower state energies, and air- and self-broadened halfwidths of more than 53, 000 lines. The results have been generated using improved spectroscopic parameters obtained in a number of recent high resolution laboratory studies. A total of eighteen bands of 1603 (sixteen hot bands plus the v\ and v3 fundamentals) are included along with the vx and v3 fundamentals of both 160160180 and i6oi8()160. As shown by comparisons of line-by-line simulations with 0.003-cm-1 resolution balloon-borne stratospheric solar spectra, the new parameters greatly improve the accuracy of atmospheric calculations in the 10-yum region, especially for the isotopic 160160180 and 160180160 lines. © 1990 Optical Society of America.
引用
收藏
页码:3667 / 3671
页数:5
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