Satellite-derived methanol emission estimates based on IASIv4 CH3OH columns (2008-2019)
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Top-down global methanol (CH3OH) distribution in 2019 (in 1010 molecules cm-2 s-1) with total emissions in Tg CH3OH from (i) biogenic and (ii) pyrogenic sources. The dry deposition sink is also shown.

About the data
Top-down emissions are estimated using an inverse modelling framework based on the chemistry–transport model MAGRITTE v1.2 and its adjoint (Müller et al., 2019; Bauwens et al., 2016; Müller and Stavrakou, 2005), constrained by methanol (CH₃OH) column observations from the Infrared Atmospheric Sounding Interferometer (IASI) (Franco et al., 2018; Clarisse et al., 2023). We use the latest version of the space-borne methanol retrievals (IASIv4) to derive global terrestrial methanol emissions for the period 2008–2019. The IASIv4 dataset is bias-corrected using airborne observations.
More details can be found in the companion paper of Müller et al. (submitted to ACP).
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Global monthly top-down data (in 1010 molecules cm-2 s-1) are available in NetCDF format at a resolution of 2°x2.5° from 2008 to 2019.
- Biogenic source:
- Pyrogenic source:
- Dry deposition sink:
Cite this as (APA format)
Müller, J.-F. & Stavrakou, T. (2026). Global top-down methanol emissions based on IASI data (2008-2019) (Version 1) [Data set]. Royal Belgian Institute for Space Aeronomy. https://doi.org/10.18758/5fmk39fw.
Acknowledgements
This study was supported by the GLANCE project (http://glance.aeronomie.be/) funded by the European Space Agency (ESA) under the “eo science for society" programme and by the CONCERTO project (https://www.projectconcerto.eu/) funded by the European Commission under the Horizon Europe programme (grant agreement no. 101185000).