Infrared collision-induced and far-line absorption in dense CO2 atmospheres

被引:123
作者
Wordsworth, R. [1 ]
Forget, F. [1 ]
Eymet, V. [2 ]
机构
[1] Inst Pierre Simon Laplace, Meteorol Dynam Lab, Paris, France
[2] Univ Toulouse 3, Lab Plasma & Convers Energie, F-31062 Toulouse, France
关键词
Radiative transfer; Spectroscopy; Mars; Extrasolar planets; CARBON-DIOXIDE CLOUDS; SURFACE-TEMPERATURE; EARLY MARS; CLIMATE; GREENHOUSE; VENUS; SIMULATION; SCATTERING; WINGS;
D O I
10.1016/j.icarus.2010.06.010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Collision-induced absorption is of great importance to the overall radiative budget in dense CO2-rich atmospheres, but its representation in climate models remains uncertain, mainly due to a lack of accurate experimental and theoretical data. Here we compare several parameterisations of the effect, including a new one that makes use of previously unused measurements in the 1200-1800 cm(-1) spectral range. We find that a widely used parameterisation strongly overestimates absorption in pure CO2 atmospheres compared to later results, and propose a new approach that we believe is the most accurate possible given currently available data. (C) 2010 Elsevier Inc. All rights reserved.
引用
收藏
页码:992 / 997
页数:6
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