The temperature dependent absorption cross sections of C4H2 at mid ultraviolet wavelengths

被引:21
|
作者
Smith, NS [1 ]
Bénilan, Y [1 ]
Bruston, P [1 ]
机构
[1] Univ Paris 12, LISA, F-94010 Creteil, France
基金
英国工程与自然科学研究理事会;
关键词
D O I
10.1016/S0032-0633(97)00206-7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have measured the mid UV (195-265 nm) absorption coefficients of diacetylene, C4H2, over the temperature range 193-293 K. An impurity involved in the synthesis of C4H2, namely C4H3Cl, can strongly influence the measured absorption coefficients. This impurity has a mid UV absorption approximately 300 times stronger than C4H2 and we demonstrate that its presence, at low levels, in previously published spectra has strongly influenced the published coefficients and their temperature dependence. We have obtained an ultra-pure sample of C4H2 by repeated distillation and show here its "clean" spectrum and temperature dependence. We confirm previous band assignments, but our superior resolution (0.02 nm) has shown the presence of other, previously undetected bands. These new results have wide implications for the modelling of Titan's atmosphere and the analysis of observational data. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:1215 / 1220
页数:6
相关论文
共 50 条