Simulation of source intensity variations from atmospheric dust for solar occultation Fourier transform infrared spectroscopy at Mars-Reference-Cited by-同舟云学术

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Simulation of source intensity variations from atmospheric dust for solar occultation Fourier transform infrared spectroscopy at Mars

Published:2016-05 Issue: Volume:323 Page:78-85
ISSN:0022-2852
Container-title:Journal of Molecular Spectroscopy
language:en
Short-container-title:Journal of Molecular Spectroscopy

Author:

Olsen K.S.,Toon G.C.,Strong K.

Funder

CSA

Natural Sciences and Engineering Research Council of Canada

Publisher

Elsevier BV

Subject

Physical and Theoretical Chemistry,Spectroscopy,Atomic and Molecular Physics, and Optics

Reference25 articles.

1. Atmospheric chemistry experiment (ACE): mission overview;Bernath;Geophys. Res. Lett.,2005

2. Retrievals for the atmospheric chemistry experiment Fourier-transform spectrometer;Boone;Appl. Opt.,2005

3. Fourier transform spectroscopy;Brault,1985

4. MARCI and MOC observations of the atmosphere and surface cap in the north polar region of Mars;Cantor;Icarus,2010

5. Cloud detection in the upper troposphere-lower stratosphere region via ACE imagers: a qualitative study;Dodion;J. Geophys. Res.,2007

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