Infrared spectroscopy and the terrestrial atmosphere

被引：16

作者：

Flaud, JM

Oelhaf, H

机构：

[1] Univ Paris 11, CNRS, Photophys Mol Lab, F-91405 Orsay, France

[2] Forschungszentrum Karlsruhe, Inst Meteorol & Klimaforsch, D-76021 Karlsruhe, Germany

来源：

COMPTES RENDUS PHYSIQUE | 2004年 / 5卷 / 02期

关键词：

molecular spectroscopy; infrared; atmospheric sounding; minor atmospheric constituents retrievals; stratospheric ozone; climate research;

D O I：

10.1016/j.crhy.2004.01.016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Fourier transform infrared spectroscopy is an extremely powerful technique for atmospheric remote sensing. In particular, on board a satellite and working in emission in the limb-viewing mode, it allows a global coverage during day and night. Based on this method the MIPAS experiment has been recently launched on ESXs Environmental satellite (ENVISAT). However, accurate retrievals require high quality spectroscopic parameters. It is the goal of this paper to show on a few selected examples the importance of using for the retrievals high quality spectral parameters derived from the best possible experimental and theoretical laboratory methods. To cite this article: J.-M. Flaud, H. Oelhaf, C. R. Physique 5 (2004). (C) 2004 Academie des sciences. Published by Elsevier SAS. All rights reserved.

引用

页码：259 / 271

页数：13

共 63 条

[1] NIGHTTIME REACTIVE NITROGEN MEASUREMENTS FROM STRATOSPHERIC INFRARED THERMAL EMISSION OBSERVATIONS [J].