Relationship between ATSR fire counts and CO vertical column densities retrieved from SCIAMACHY onboard ENVISAT
Abstract
SCIAMACHY (Scanning Imaging Absorption spectroMeter for Atmospheric ChartographY) is the first instrument to allow retrieval of CO by measuring absorption in the near infrared from reflected and scattered sunlight instead of from thermal emission. Thus, in contrast to thermal-infrared satellites (MOPITT), SCIAMACHY is highly sensitive to the lower layers of the troposphere where the sources, such as biomass burning, are located, and where the bulk of the CO is usually found. In many regions of the world, the burning of vegetation has a repeating seasonal pattern, but the amount of CO emitted from biomass burning varies considerably from place to place. Here we present a study on the relationship between fire counts and CO vertical column densities (VCD) in different regions. These results are compared with the CO VCD from MOPITT, aerosol index, and NO_2 tropospheric VCD (TVCD) from SCIAMACHY, and the coupled chemistry climate model (CCM) ECHAM5/MESSY.
Additional Information
© SPIE 2008. We would like to thank ESA (European Space Agency) and the DLR (Deutsches Zentrum Fur Luft- und Raumfahrt) for providing us with the L1b SCIAMACHY data files. Also, ESA provide the active fire counts from the Along-Track Scanning Radiometer (ATSR) sensor on board the ERS-2 satellite which could be downloaded from http://dup.esrin.esa.it/ionia/projects/projectsALPHA.asp. We thank the TEMIS project for providing us with FRESCO+ data. The data were downloaded from: http:/www.temis.nl/. We thank Space Science Division of the Canadian Space Agency for providing Measurements Of Pollution In The Troposphere (MOPITT) data. The data were downloaded from: http://eosweb.larc.nasa.gov/PRODOCS/mopitt/.Attached Files
Published - Frankenberg_2008p70890I.pdf
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- Eprint ID
- 57391
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- CaltechAUTHORS:20150508-151516563
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2015-05-11Created from EPrint's datestamp field
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2021-11-10Created from EPrint's last_modified field
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- Division of Geological and Planetary Sciences
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- Proceedings of SPIE
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- 7089