IASI measurements of reactive trace species in biomass burning plumes

This work presents observations of a series of short-lived species in biomass burning plumes from the Infrared Atmospheric Sounding Interferometer (IASI), launched onboard the MetOp-A platform in October 2006. The strong fires that have occurred in the Mediterranean Basin – and particularly Greece –...

Full description

Bibliographic Details
Main Authors: P.-F. Coheur, L. Clarisse, S. Turquety, D. Hurtmans, C. Clerbaux
Format: Article
Language:English
Published: Copernicus Publications 2009-08-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/9/5655/2009/acp-9-5655-2009.pdf
id doaj-14441f8330a94da6b2ce5c243fcb3173
record_format Article
spelling doaj-14441f8330a94da6b2ce5c243fcb31732020-11-25T02:35:42ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242009-08-0191556555667IASI measurements of reactive trace species in biomass burning plumesP.-F. CoheurL. ClarisseS. TurquetyD. HurtmansC. ClerbauxThis work presents observations of a series of short-lived species in biomass burning plumes from the Infrared Atmospheric Sounding Interferometer (IASI), launched onboard the MetOp-A platform in October 2006. The strong fires that have occurred in the Mediterranean Basin – and particularly Greece – in August 2007, and those in Southern Siberia and Eastern Mongolia in the early spring of 2008 are selected to support the analyses. We show that the IASI infrared spectra in these fire plumes contain distinctive signatures of ammonia (NH<sub>3</sub>), ethene (C<sub>2</sub>H<sub>4</sub>), methanol (CH<sub>3</sub>OH) and formic acid (HCOOH) in the atmospheric window between 800 and 1200 cm<sup>−1</sup>, with some noticeable differences between the plumes. Peroxyacetyl nitrate (CH<sub>3</sub>COOONO<sub>2</sub>, abbreviated as PAN) was also observed with good confidence in some plumes and a tentative assignment of a broadband absorption spectral feature to acetic acid (CH<sub>3</sub>COOH) is made. For several of these species these are the first reported measurements made from space in nadir geometry. The IASI measurements are analyzed for plume height and concentration distributions of NH<sub>3</sub>, C<sub>2</sub>H<sub>4</sub> and CH<sub>3</sub>OH. The Greek fires are studied in greater detail for the days associated with the largest emissions. In addition to providing information on the spatial extent of the plume, the IASI retrievals allow an estimate of the total mass emissions for NH<sub>3</sub>, C<sub>2</sub>H<sub>4</sub> and CH<sub>3</sub>OH. Enhancement ratios are calculated for the latter relative to carbon monoxide (CO), giving insight in the chemical processes occurring during the transport, the first day after the emission. http://www.atmos-chem-phys.net/9/5655/2009/acp-9-5655-2009.pdf
collection DOAJ
language English
format Article
sources DOAJ
author P.-F. Coheur
L. Clarisse
S. Turquety
D. Hurtmans
C. Clerbaux
spellingShingle P.-F. Coheur
L. Clarisse
S. Turquety
D. Hurtmans
C. Clerbaux
IASI measurements of reactive trace species in biomass burning plumes
Atmospheric Chemistry and Physics
author_facet P.-F. Coheur
L. Clarisse
S. Turquety
D. Hurtmans
C. Clerbaux
author_sort P.-F. Coheur
title IASI measurements of reactive trace species in biomass burning plumes
title_short IASI measurements of reactive trace species in biomass burning plumes
title_full IASI measurements of reactive trace species in biomass burning plumes
title_fullStr IASI measurements of reactive trace species in biomass burning plumes
title_full_unstemmed IASI measurements of reactive trace species in biomass burning plumes
title_sort iasi measurements of reactive trace species in biomass burning plumes
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2009-08-01
description This work presents observations of a series of short-lived species in biomass burning plumes from the Infrared Atmospheric Sounding Interferometer (IASI), launched onboard the MetOp-A platform in October 2006. The strong fires that have occurred in the Mediterranean Basin – and particularly Greece – in August 2007, and those in Southern Siberia and Eastern Mongolia in the early spring of 2008 are selected to support the analyses. We show that the IASI infrared spectra in these fire plumes contain distinctive signatures of ammonia (NH<sub>3</sub>), ethene (C<sub>2</sub>H<sub>4</sub>), methanol (CH<sub>3</sub>OH) and formic acid (HCOOH) in the atmospheric window between 800 and 1200 cm<sup>−1</sup>, with some noticeable differences between the plumes. Peroxyacetyl nitrate (CH<sub>3</sub>COOONO<sub>2</sub>, abbreviated as PAN) was also observed with good confidence in some plumes and a tentative assignment of a broadband absorption spectral feature to acetic acid (CH<sub>3</sub>COOH) is made. For several of these species these are the first reported measurements made from space in nadir geometry. The IASI measurements are analyzed for plume height and concentration distributions of NH<sub>3</sub>, C<sub>2</sub>H<sub>4</sub> and CH<sub>3</sub>OH. The Greek fires are studied in greater detail for the days associated with the largest emissions. In addition to providing information on the spatial extent of the plume, the IASI retrievals allow an estimate of the total mass emissions for NH<sub>3</sub>, C<sub>2</sub>H<sub>4</sub> and CH<sub>3</sub>OH. Enhancement ratios are calculated for the latter relative to carbon monoxide (CO), giving insight in the chemical processes occurring during the transport, the first day after the emission.
url http://www.atmos-chem-phys.net/9/5655/2009/acp-9-5655-2009.pdf
work_keys_str_mv AT pfcoheur iasimeasurementsofreactivetracespeciesinbiomassburningplumes
AT lclarisse iasimeasurementsofreactivetracespeciesinbiomassburningplumes
AT sturquety iasimeasurementsofreactivetracespeciesinbiomassburningplumes
AT dhurtmans iasimeasurementsofreactivetracespeciesinbiomassburningplumes
AT cclerbaux iasimeasurementsofreactivetracespeciesinbiomassburningplumes
_version_ 1724803919069052928