ANALYSIS OF SMALL-SCALE AND LARGE-SCALE INCREASES OF REACTIVE NITROGEN OBSERVED DURING THE 2ND AIRBORNE ARCTIC STRATOSPHERIC EXPEDITION

Citation
J. Zheng et al., ANALYSIS OF SMALL-SCALE AND LARGE-SCALE INCREASES OF REACTIVE NITROGEN OBSERVED DURING THE 2ND AIRBORNE ARCTIC STRATOSPHERIC EXPEDITION, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 101(D22), 1996, pp. 28805-28816
Citations number
28
Categorie Soggetti
Metereology & Atmospheric Sciences
Volume
101
Issue
D22
Year of publication
1996
Pages
28805 - 28816
Database
ISI
SICI code
Abstract
An analysis of the data obtained during AASE II was made to characteri ze small- (delta x < 24 km) and large-scale (30 < delta x < 260 km) in creases of reactive nitrogen species. By using the NOx/NOy ratio, the increases were classified into fresh emissions and aged air parcels. T he sources of the NOy increases were then assessed by the freshness of the increases and by examining the correlation (or absence thereof) b etween NOy and other trace species including tracers of various NOx so urces: for example, aircraft emissions, lightning, the stratospheric s ource, and sources in the boundary layer. We found that the majority ( 43%) of NOy increases in the upper troposphere and lower stratosphere were due to displacement of constant mixing ratio surfaces relative to isobaric flight paths. Aircraft emissions were the second most abunda nt (17%). The next significant contributor was surface emissions, incl uding fossil fuel combustion and biomass burning. Only two lightning s pikes were found, apparently due to the winter season and emphasis on high latitudes in the AASE II experiment. The relative contribution fr om each source to the increases (or positive variability) represents a measure of the relative source strength. However, it is important to note that our findings on the relative contribution of each source to the NOy increases should not be applied directly to estimating the rel ative source strength of the ambient or background NOy abundance. Know ledge of the detailed temporal and spatial distribution of the relativ e contribution of each source is needed. This requires a substantially higher precision for the instruments of tracer gases than those used in this study.