Abstract

Abstract. Formic acid (HCOOH) concentrations are often underestimated by models, and its chemistry is highly uncertain. HCOOH is, however, among the most abundant atmospheric volatile organic compounds, and it is potentially responsible for rain acidity in remote areas. HCOOH data from the Infrared Atmospheric Sounding Interferometer (IASI) are analyzed from 2008 to 2014 to estimate enhancement ratios from biomass burning emissions over seven regions. Fire-affected HCOOH and CO total columns are defined by combining total columns from IASI, geographic location of the fires from Moderate Resolution Imaging Spectroradiometer (MODIS), and the surface wind speed field from the European Centre for Medium-Range Weather Forecasts (ECMWF). Robust correlations are found between these fire-affected HCOOH and CO total columns over the selected biomass burning regions, allowing the calculation of enhancement ratios equal to 7.30 × 10−3 ± 0.08 × 10−3 mol mol−1 over Amazonia (AMA), 11.10 × 10−3 ± 1.37 × 10−3 mol mol−1 over Australia (AUS), 6.80 × 10−3 ± 0.44 × 10−3 mol mol−1 over India (IND), 5.80 × 10−3 ± 0.15 × 10−3 mol mol−1 over Southeast Asia (SEA), 4.00 × 10−3 ± 0.19 × 10−3 mol mol−1 over northern Africa (NAF), 5.00 × 10−3 ± 0.13 × 10−3 mol mol−1 over southern Africa (SAF), and 4.40 × 10−3 ± 0.09 × 10−3 mol mol−1 over Siberia (SIB), in a fair agreement with previous studies. In comparison with referenced emission ratios, it is also shown that the selected agricultural burning plumes captured by IASI over India and Southeast Asia correspond to recent plumes where the chemistry or the sink does not occur. An additional classification of the enhancement ratios by type of fuel burned is also provided, showing a diverse origin of the plumes sampled by IASI, especially over Amazonia and Siberia. The variability in the enhancement ratios by biome over the different regions show that the levels of HCOOH and CO do not only depend on the fuel types.

Highlights

  • Formic acid (HCOOH) is one of the most abundant carboxylic acids present in the atmosphere

  • A total of 7 years of HCOOH data measured by Infrared Atmospheric Sounding Interferometer (IASI) over seven different fire regions around the world were analyzed (AMA, Amazonia; AUS, Australia; IND, India; SEA, Southeast Asia; NAF, northern Africa; SAF, southern Africa; SIB, Siberia)

  • By taking into account the surface wind speed and by characterizing each Moderate Resolution Imaging Spectroradiometer (MODIS) fire hotspot with a value of HCOOH and carbon monoxide (CO) total columns, this work established enhancement ratios for the seven biomass burning areas and compared them to previously reported values found in literature

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Summary

Introduction

Formic acid (HCOOH) is one of the most abundant carboxylic acids present in the atmosphere. Other studies have used the solar occultation Atmospheric Chemistry Experiment–Fourier Transform Spectrometer (ACE-FTS), which measures the atmospheric composition in the upper troposphere (e.g., Rinsland et al, 2006; Gonzalez Abad et al, 2009; Tereszchuk et al, 2011, 2013), and the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) limb instrument, which is sensitive to around 10 km (Grutter et al, 2010) These infrared (IR) sounders have limited vertical sensitivity as compared to ground-based or airborne measurements, but their spatial coverage represents a major advantage, which allows observation of remote regions which are sparsely studied by field measurements, like the biomass burning regions.

The IASI mission
The CO retrieval characteristics
The HCOOH retrieval characteristics
The selected areas
The IASI data used
Importance of the meteorological conditions
General analysis
Analysis over each region
Analysis based on the type of vegetation
Findings
Conclusions
Full Text
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