Nitrogen oxides and PAN in plumes from boreal fires during ARCTAS-B and their impact on ozone: an integrated analysis of aircraft and satellite observations

• Published in: Atmospheric Chemistry and Physics
• Main Authors: Alvarado, M. J., Wennberg, P. O., Kurten, A., Crounse, J., St. Clair, J. M.
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: European Geosciences Union 2010
• Subjects: Arctic; Canada
• Online Access: https://doi.org/10.5194/acp-10-9739-2010

We determine enhancement ratios for NO_x, PAN, and other NO_y species from boreal biomass burning using aircraft data obtained during the ARCTAS-B campaign and examine the impact of these emissions on tropospheric ozone in the Arctic. We find an initial emission factor for NO_x of 1.06 g NO per kg dry matter (DM) burned, much lower than previous observations of boreal plumes, and also one third the value recommended for extratropical fires. Our analysis provides the first observational confirmation of rapid PAN formation in a boreal smoke plume, with 40% of the initial NO_x emissions being converted to PAN in the first few hours after emission. We find little clear evidence for ozone formation in the boreal smoke plumes during ARCTAS-B in either aircraft or satellite observations, or in model simulations. Only a third of the smoke plumes observed by the NASA DC8 showed a correlation between ozone and CO, and ozone was depleted in the plumes as often as it was enhanced. Special observations from the Tropospheric Emission Spectrometer (TES) also show little evidence for enhanced ozone in boreal smoke plumes between 15 June and 15 July 2008. Of the 22 plumes observed by TES, only 4 showed ozone increasing within the smoke plumes, and even in those cases it was unclear that the increase was caused by fire emissions. Using the GEOS-Chem atmospheric chemistry model, we show that boreal fires during ARCTAS-B had little impact on the median ozone profile measured over Canada, and had little impact on ozone within the smoke plumes observed by TES. © Author(s) 2010. This work is distributed under the Creative Commons Attribution 3.0 License. Published by Copernicus Publications on behalf of the European Geosciences Union. Received: 8 June 2010 – Published in Atmos. Chem. Phys. Discuss.: 22 June 2010. Revised: 7 October 2010 – Accepted: 8 October 2010 – Published: 18 October 2010. We thank all of the members of the ARCTAS Science Team and the TES Science Team for their work. We thank D. J. Jacob, J. A. Fisher, and ...