A new photometric ozone reference in the Huggins bands: the absolute ozone absorption cross section at the 325 nm HeCd laser wavelength

被引:8
|
作者
Janssen, Christof [1 ]
Elandaloussi, Hadj [1 ]
Grobner, Julian [2 ]
机构
[1] Sorbonne Univ, Univ PSL, Observ Paris,LERMA IPSL, CNRS,Lab Etud Rayonnement & Matiere Astrophys & A, F-75005 Paris, France
[2] Phys Meteorol Observ Davos, World Radiat Ctr, Davos, Switzerland
关键词
GROUND-BASED FTIR; 10; MU-M; STRAIGHT-LINE; UV SPECTROSCOPY; COEFFICIENTS; PARAMETERS; DEPENDENCE; EQUATIONS; O-3;
D O I
10.5194/amt-11-1707-2018
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
The room temperature (294.09 K) absorption cross section of ozone at the 325 nm HeCd wavelength has been determined under careful consideration of possible biases. At the vacuum wavelength of 325.126 nm, thus in a region used by a variety of ozone remote sensing techniques, an absorption cross-section value of sigma = 16.470 x 10(-21) cm(2) was measured. The measurement provides the currently most accurate direct photometric absorption value of ozone in the UV with an expanded (coverage factor k = 2) standard uncertainty u (sigma) = 31 x 10(-24) cm(2), corresponding to a relative level of 2 parts per thousand. The measurements are most compatible with a relative temperature coefficient c(T) = sigma(-1) partial derivative(T)sigma = 0.0031 K-1 at 294 K. The cross section and its uncertainty value were obtained using generalised linear regression with correlated uncertainties. It will serve as a reference for ozone absorption spectra required for the long-term remote sensing of atmospheric ozone in the Huggins bands. The comparison with commonly used absorption cross-section data sets for remote sensing reveals a possible bias of about 2 %. This could partly explain a 4 % discrepancy between UV and IR remote sensing data and indicates that further studies will be required to reach the accuracy goal of 1 % in atmospheric reference spectra.
引用
收藏
页码:1707 / 1723
页数:17
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