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Title: Development and characterisation of a state-of-the-art GOME-2 formaldehyde air-mass factor algorithm
Authors: Hewson, W.
Barkley, M. P.
Gonzalez Abad, G.
Bösch, H.
Kurosu, T.
Spurr, R.
First Published: 27-Jan-2015
Publisher: European Geosciences Union (EGU), Copernicus Publications
Citation: Atmospheric Measurement Techniques Discussions, 8, 1109–1150, 2015
Abstract: Space-borne observations of formaldehyde (HCHO) are frequently used to derive surface emissions of isoprene, an important biogenic volatile organic compound. The conversion of retrieved HCHO slant column concentrations from satellite line of sight measurements to vertical columns is determined through application of an air mass factor (AMF), accounting for instrument viewing geometry, radiative transfer, and vertical profile of the absorber in the atmosphere. This step in the trace gas retrieval is subject to large errors. This work presents the AMF algorithm in use at the University of Leicester (UoL), which introduces scene specific variables into a per-observation full radiative transfer AMF calculation, including increasing spatial resolution of key environmental parameter databases, input variable area weighting, instrument specific scattering weight calculation, and inclusion of an ozone vertical profile climatology. Application of these updates to HCHO slant columns from the GOME-2 instrument is shown to typically adjust the AMF by ±10%, compared to a~reference algorithm without these advanced parameterisations. Furthermore, the new UoL algorithm also incorporates a full radiative transfer error calculation for each scene to help characterise AMF uncertainties. Global median AMF errors are typically 50–60%, and are dominated by uncertainties in the HCHO profile shape and its corresponding seasonal variation.
DOI Link: 10.5194/amtd-8-1109-2015
ISSN: 1867-8610
eISSN: 1867-8610
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © Author(s) 2015. This work is distributed under the Creative Commons Attribution 3.0 License (CC BY 3.0) (
Description: The Supplement related to this article is available online at doi:10.5194/amtd-8-1109-2015-supplement.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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