EOS-Aura/OMI NO2 slant column retrieval:
stability & uncertainties

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TROPOMI : Introduction
OMI : Introduction

 

Introduction

An initial study into the stability and uncertainties of the EOS-AURA/OMI NO2 slant column density (SCD) retrieval was presented by Zara et al., 2018, which covers NO2 retrieval data up to 31 Dec. 2015.

These pages provide an update of that analysis as well as additional analysis results using NO2 data of the collection 4 (re)processed data, starting from 1 Oct. 2004 up to the end of 2022.

The results presented here are manually updated and currently
cover the NO2 SCD retrieval results up to: 31 Dec. 2025
Note: The data presented are from a preliminary version of the collection 4 data. The final version of the data, extending to the end of the OMI mission, will be presented here in due time -- differences are, however, expected to be small.

 

Contents

 

Data selection for the analysis

As in Zara et al., 2018 for OMI van Geffen et al., 2020 for TROPOMI, the analysis is based on orbits over the Pacific Ocean (i.e. away from anthropogenic sources of NO2): for each day the last orbit is selected, provided that orbit has a satellite (nadir viewing) equator crossings west of about -130°. Such a Pacific Ocean orbit is missing on several few days, in particular during the periods when OMI was measuring in zoom mode, and these days are therefore skipped.

Two latitude ranges are used, depending on the type of analysis:

Slant and vertical NO2 column values are given here in the SI unit mol/m2 (as in the OMI collection 4 data files) and in several places also in the more commenly unit molecules/cm2; the conversion factor between these two is 6.02214e19. For example, 10.0 μmol/m2 corresponds to 6.022+14 molecules/cm2, and 2.0e15 molecules/cm2 corresponds to 33.211 μmol/m2.

 


 

References

 


last modified: 26 June 2026
Contact: Jos van Geffen   < geffen [at] knmi [dot] nl >
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