posted on 2006-09-13, 10:32authored byN. Brough, C.E. Reeves, Stuart A. Penkett, D.J. Stewart, K. Dewey, J.M. Kent, H. Barjat, Paul S. Monks, H. Ziereis, P. Stock, H. Huntrieser, H. Schlager
In the summer 2000 EXPORT aircraft campaign
(European eXport of Precursors and Ozone by long-Range Transport), two comprehensively instrumented research aircraft measuring a variety of chemical species flew wing tip
to wing tip for a period of one and a quarter hours. During this interval a comparison was undertaken of the measurements of nitrogen oxide (NO), odd nitrogen species (NOy), carbon monoxide (CO) and ozone (O3). The comparison was
performed at two different flight levels, which provided a 10-fold variation in the concentrations of both NO (10 to 1000
parts per trillion by volume (pptv)) and NOy (200 to over 2500 pptv). Large peaks of NO and NOy observed from the Falcon 20, which were at first thought to be from the exhaust of the C-130, were also detected on the 4 channel NOxy instrument aboard the C-130. These peaks were a good indication
that both aircraft were in the same air mass and that the Falcon 20 was not in the exhaust plume of the C-130. Correlations
and statistical analysis are presented between the instruments used on the two separate aircraft platforms. These
were found to be in good agreement giving a high degree of correlation for the ambient air studied. Any deviations from the correlations are accounted for in the estimated inaccuracies of the instruments. These results help to establish that the instruments aboard the separate aircraft are reliably able to measure the corresponding chemical species in the range
of conditions sampled and that data collected by both aircraft can be co-ordinated for purposes of interpretation.
History
Citation
Atmospheric Chemistry and Physics, 2003, 3, pp.2127-2138
Published in
Atmospheric Chemistry and Physics
Publisher
European Geosciences Union
Available date
2006-09-13
Notes
This article is licensed under a Creative Commons License and is also available from http://www.copernicus.org/EGU/acp/acp.html, along with further discussion.