2005
DOI: 10.1364/ao.44.007218
|View full text |Cite
|
Sign up to set email alerts
|

Retrievals for the atmospheric chemistry experiment Fourier-transform spectrometer

Abstract: SCISAT-1, also known as the Atmospheric Chemistry Experiment, is a satellite mission for remote sensing of the Earth's atmosphere, launched on 12 August 2003. The primary instrument on the satellite is a 0.02 cm(-1) resolution Fourier-transform spectrometer operating in the mid-IR (750-4400 cm(-1)). We describe the approach developed for the retrieval of atmospheric temperature and pressure from the troposphere to the lower thermosphere as well as the strategy for the retrievals of volume-mixing ratio profiles… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

0
360
0

Year Published

2007
2007
2016
2016

Publication Types

Select...
7

Relationship

4
3

Authors

Journals

citations
Cited by 425 publications
(360 citation statements)
references
References 37 publications
0
360
0
Order By: Relevance
“…The irregular retrieval grid is defined by the tangent altitudes. The retrieval setup is reported by Boone et al (2005) for versions 2.1 and 2.2. For version 3.0 the changes in the retrieval setup are described in Boone et al (2013) and chiefly address temperature issues.…”
Section: Ace-ftsmentioning
confidence: 99%
“…The irregular retrieval grid is defined by the tangent altitudes. The retrieval setup is reported by Boone et al (2005) for versions 2.1 and 2.2. For version 3.0 the changes in the retrieval setup are described in Boone et al (2013) and chiefly address temperature issues.…”
Section: Ace-ftsmentioning
confidence: 99%
“…The retrieval approach is similar to the one adopted by ACE [24] and the method of Carlott [25]. It is based on nonlinear least squares fitting of spectra for the target molecule and interfering molecules.…”
Section: Analysis and Comparison With Model Predictionsmentioning
confidence: 99%
“…It is based on nonlinear least squares fitting of spectra for the target molecule and interfering molecules. Our analysis combines the COClF lines from the 1995 ATMOS supplemental linelist [18], the ACE solar spectra, and spectral parameters for other molecules from HITRAN 2004 [20] with the retrieved profiles of temperature, pressure, and tangent altitude for individual ACE occultations [24]. A refractive ray tracing program was used with the ACE-derived temperature profile and tangent heights to calculate airmass-weighted pressures, temperatures, and atmospheric ray paths for individual ACE occultations.…”
Section: Analysis and Comparison With Model Predictionsmentioning
confidence: 99%
See 2 more Smart Citations