Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/38418
Title: New and improved infra-red absorption cross sections and ACE-FTS retrievals of carbon tetrachloride (CCl<inf>4</inf>)
Authors: Harrison, Jeremy J.
Boone, C. D.
Bernath, P. F.
First Published: 6-May-2016
Presented at: Satellite Remote Sensing and Spectroscopy: Joint ACE-Odin Meeting, October 2015
Publisher: Elsevier for Pergamon
Citation: Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 186, January 2017, Pages 139–149
Abstract: Carbon tetrachloride (CCl4) is one of the species regulated by the Montreal Protocol on account of its ability to deplete stratospheric ozone. As such, the inconsistency between observations of its abundance and estimated sources and sinks is an important problem requiring urgent attention (Carpenter et al., 2014) [5]. Satellite remote-sensing has a role to play, particularly limb sounders which can provide vertical profiles into the stratosphere and therefore validate stratospheric loss rates in atmospheric models.This work is in two parts. The first describes new and improved high-resolution infra-red absorption cross sections of carbon tetrachloride/dry synthetic air over the spectral range 700-860cm-1 for a range of temperatures and pressures (7.5-760Torr and 208-296K) appropriate for atmospheric conditions. This new cross-section dataset improves upon the one currently available in the HITRAN and GEISA databases. The second describes a new, preliminary ACE-FTS carbon tetrachloride retrieval that improves upon the v3.0/v3.5 data products, which are biased high by up to ~20-30% relative to ground measurements. Making use of the new spectroscopic data, this retrieval also improves the microwindow selection, contains additional interfering species, and utilises a new instrumental lineshape; it will form the basis for the upcoming v4.0 CCl4 data product.
DOI Link: 10.1016/j.jqsrt.2016.04.025
ISSN: 0022-4073
Links: http://www.sciencedirect.com/science/article/pii/S002240731630108X
http://hdl.handle.net/2381/38418
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © 2016 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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